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The model has image packed into the blend file. good model for medical school, colleges and biology.\nThe formats 3mf, ply, obj, fbx, USDZ,GLTZ \u0026 GLB with applied uv mapped textures have also been included in the downloads along with  stl.\n\nI have included the various formats needed by various customer for the various 3d modelling softwares they may be using. \nThe following formats are compressed in rar formats :-\n1.\tblend\n2.\t3mf\n3.\tstl\n4.\tobj\n5.\tfbx\n6.\tglb\n7.\tgltz\n8.\tusdz\nThe downloaded files have to unpacked using any rar unpacker. After unpacking, the folder content of the respective formats will be as follows :-.\n1.\tblend :- single file with all applied and packed textures.\n2.\t3mf :- single file with all applied and packed textures.\n3.\tstl :- single file with only geometry data\n4.\tobj :- mutiple files including .obj,.mtl, images textures.\n5.\tfbx :- single file with all applied and packed textures.\n6.\tglb :- single file with all applied and packed textures.\n7.\tgltz :- mutiple files including .bin, images textures.\n8.\tusdz :- single file \n\nThe native file is blend so the open source software blender opens mostly all the files, with textures (packed with the files). The best way is to open the files named blend with blender. Other files have to be imported in blender by clicking within blender \"File \u003e\u003eImport\u003e\u003eselect the type of file you want to import\u003e\u003eopen file location of the downloaded unzipped files\u003e\u003eselect the file\u003e\u003ethe model would open in the 3d viewport of the software.\nThe other files including blender can be opened with most of the free and paid 3d modelling software. The files obj \u0026 fbx are compatible with other 3d modeling software, example maya. These software's have the open/import options similar to blender. The files stl and 3mf are compatible with 3d printing software's. The built in \"3d builder \" windows software opens all of these files including glb, \u0026 gltz. In case you don't have 3d builder installed just download it free from Microsoft store for free. \nFor 3d builder 3mf, fbx, stl, glb are standalone files (right click the model file\u003e\u003eselect open with\u003e\u003e3d builder). For obj,ply, \u0026 gltz 3d builder will prompt you to select the model files .mtl and image textures (these are packed in the rar files).\nThe textures files have been separately supplied additionally; in case one needs them.","imageAlt":"3D model Breast duct sites and diseases","url":"https://www.cgtrader.com/3d-models/science/medical/breast-duct-sites-and-diseases","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/YX9RfeLZf1nBz7kW6zCVvLsb/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/0001.jpg","gridUrl":"https://media.cgtrader.com/variants/YX9RfeLZf1nBz7kW6zCVvLsb/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/0001.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/science/medical/breast-duct-sites-and-diseases","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":21,"name":".blend","is_native":true},{"id":127,"name":".usdz","is_native":false},{"id":117,"name":".gltf","is_native":false},{"id":189,"name":".ply","is_native":false},{"id":null,"name":null,"is_native":false},{"id":51,"name":".stl","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":129,"name":".3mf","is_native":false}],"categorySlug":"science","subcategorySlug":"medical","categoryTitle":"Science","subcategoryTitle":"Medical","schemaImageUrl":"https://img-new.cgtrader.com/items/4713659/f178eb4c3e/breast-duct-sites-and-diseases-3d-model-f178eb4c3e.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"979901","type":"listingItem","attributes":{"id":979901,"title":"hepatic liver lobule","price":79.0,"description":"The formats 3mf, obj, fbx, USDZ,GLTZ \u0026 GLB with applied uv mapped textures have also been included in the downloads along with ply \u0026 stl.\nThis a model of hepatic lobule depicting the structure of the blood vessels and bile duct along with the flow of fluid within a lobule. The structure has been labelled with texts on the view port itself. The materials are based on cycles render. I have used the array modifier, curve modifier along with empties to design the structures. In the .blend file most of the modifiers have not been applied to leave space for further modification by the designers downloading the model. Rest of the extensions (OBJ,FBX,3DS, DAE) have been exported from blender after applying modifiers\nThe blend file has 2 layers\nFirst layer :- a complete lobule\nSecond layer :- 1/6 part of a lobule\nThe short forms in outliner stand for:-\nBC :- Bezeir curve\nCyto :- mesh/ material of cytoplasm\nNuc:- mesh/ material of nucleus\nSecond layer :-\nEach structural unit has 2 meshes and a Bezier curve :- cyto (mesh), nucleus (mesh), BC (Bezier curve)\n1.\tPortal vein:-\na.\tportal v cyto\nb.\tportal v nuc\nc.\tBC portal v\n2.\tPortal branch 1\na.\tportal br 1 cyto\nb.\tportal br 1 nucleus\nc.\tBC portal br 1\n3.\tPortal branch 2\na.\tportal br2cyto\nb.\tportal br2 nucleus\nc.\tBC portal br 2\n4.\tPortal branch 3\na.\tportal br3cyto\nb.\tportal br3 nucleus\nc.\tBC portal br 3\n5.\tLobule vein \na.\tlobule v cyto\nb.\tlobule v nuc\nc.\tBC lobule v hep\n6.\tCentral vein\na.\tCentral  vcyto\nb.\tCentral  vnuc\nc.\tBC Central vein\n7.\tHepatocytes around lobule vein\na.\tlobule hep v cyto\nb.\tlobule hep v nuc\nc.\tBC lobule hep v\n8.\tHepatic artery\na.\thep art cyto\nb.\thep art nuc\nc.\tBC hepatic art\n9.\tHepatic artery br 1\na.\tHepatic art br 1 cyto\nb.\tHepatic art br 1 nuc\nc.\tBC hepatic art br 1\n10.\tHepatic artery br 2\na.\tHepatic art br2cyto\nb.\tHepatic art br2nuc\nc.\tBC hepatic art br2\n11.\tLobule artery\na.\tlobule art cyto\nb.\tlobule art nuc\nc.\tBC lobule art \n12.\tHepatocytes around lobule artery\na.\tlobule hep artcyto\nb.\tlobule hep artnuc\nc.\tBC lobule arthep\n13.\tBile duct\na.\tBile duct cyto\nb.\tBile duct nuc\nc.\tBC bile duct\n14.\tLobule bile duct\na.\tLobule bile duct cyto\nb.\tLobule bile duct nuv\nc.\tBC lobule bile duct\n15.\tArrow labels for flow\na.\tArrow bile duct \nb.\tArrow central vein \nc.\tArrow hep art \nd.\tArrow junction vein art \ne.\tArrow junction vein art label\nf.\t Arrow portal vein\n\nFirst layer :-\n\tHas similar nomenclature in outliner but with extension in name as for example\n1.\tPortal vein:-\na.\tportal v cyto (.001,.002,.003,.004,.005,.006)\nb.\tportal v nuc (.001,.002,.003,.004,.005,.006)\nc.\tBC portal v (.001,.002,.003,.004,.005,.006)\n\nThe formats 3mf, ply, obj, fbx, USDZ,GLTZ \u0026 GLB with applied uv mapped textures have also been included in the downloads along with  stl.\n\nI have included the various formats needed by various customer for the various 3d modelling softwares they may be using. \nThe following formats are compressed in rar formats :-\n1.\tblend\n2.\t3mf\n3.\tstl\n4.\tobj\n5.\tfbx\n6.\tglb\n7.\tgltz\n8.\tusdz\nThe downloaded files have to unpacked using any rar unpacker. After unpacking, the folder content of the respective formats will be as follows :-.\n1.\tblend :- single file with all applied and packed textures.\n2.\t3mf :- single file with all applied and packed textures.\n3.\tstl :- single file with only geometry data\n4.\tobj :- mutiple files including .obj,.mtl, images textures.\n5.\tfbx :- single file with all applied and packed textures.\n6.\tglb :- single file with all applied and packed textures.\n7.\tgltz :- mutiple files including .bin, images textures.\n8.\tusdz :- single file \n\nThe native file is blend so the open source software blender opens mostly all the files, with textures (packed with the files). The best way is to open the files named blend with blender. Other files have to be imported in blender by clicking within blender \"File \u003e\u003eImport\u003e\u003eselect the type of file you want to import\u003e\u003eopen file location of the downloaded unzipped files\u003e\u003eselect the file\u003e\u003ethe model would open in the 3d viewport of the software.\nThe other files including blender can be opened with most of the free and paid 3d modelling software. The files obj \u0026 fbx are compatible with other 3d modeling software, example maya. These software's have the open/import options similar to blender. The files stl and 3mf are compatible with 3d printing software's. The built in \"3d builder \" windows software opens all of these files including glb, \u0026 gltz. In case you don't have 3d builder installed just download it free from Microsoft store for free. \nFor 3d builder 3mf, fbx, stl, glb are standalone files (right click the model file\u003e\u003eselect open with\u003e\u003e3d builder). For obj,ply, \u0026 gltz 3d builder will prompt you to select the model files .mtl and image textures (these are packed in the rar files).\nThe textures files have been separately supplied additionally; in case one needs them.\n\n","imageAlt":"hepatic liver lobule 3D","url":"https://www.cgtrader.com/3d-models/science/medical/hepatic-liver-lobule","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/cjC6dSALPL4GEZ6AvNZab93P/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/hepatic-liver-lobule-3d-model-blend.jpg","gridUrl":"https://media.cgtrader.com/variants/cjC6dSALPL4GEZ6AvNZab93P/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/hepatic-liver-lobule-3d-model-blend.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/science/medical/hepatic-liver-lobule","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":21,"name":".blend","is_native":true},{"id":117,"name":".gltf","is_native":false},{"id":127,"name":".usdz","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":129,"name":".3mf","is_native":false},{"id":51,"name":".stl","is_native":false}],"categorySlug":"science","subcategorySlug":"medical","categoryTitle":"Science","subcategoryTitle":"Medical","schemaImageUrl":"https://img-new.cgtrader.com/items/979901/2d35411dd5/hepatic-liver-lobule-3d-model-2d35411dd5.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5005684","type":"listingItem","attributes":{"id":5005684,"title":"Liver histology anatomy labelled","price":59.0,"description":"A blend model of liver depicting its microscopic details as well as its direction of blood and bile flow along with its anatomical lobule, functional lobule , portal triad, bile duct and fibrous boundries.\n\nThe formats 3mf, ply, obj, fbx, USDZ,GLTZ \u0026 GLB with applied uv mapped textures have also been included in the downloads along with  stl.\n\n\n\nI have included the various formats needed by various customer for the various 3d modelling softwares they may be using. \n\nThe following formats are compressed in rar formats :-\n\n1.    blend\n\n2.    3mf\n\n3.    stl\n\n4.    obj\n\n5.    fbx\n\n6.    glb\n\n7.    gltz\n\n8.    usdz\n\nThe downloaded files have to unpacked using any rar unpacker. After unpacking, the folder content of the respective formats will be as follows :-.\n\n1.    blend :- single file with all applied and packed textures.\n\n2.    3mf :- single file with all applied and packed textures.\n\n3.    stl :- single file with only geometry data\n\n4.    obj :- mutiple files including .obj,.mtl, images textures.\n\n5.    fbx :- single file with all applied and packed textures.\n\n6.    glb :- single file with all applied and packed textures.\n\n7.    gltz :- mutiple files including .bin, images textures.\n\n8.    usdz :- single file \n\n\n\nThe native file is blend so the open source software blender opens mostly all the files, with textures (packed with the files). The best way is to open the files named blend with blender. Other files have to be imported in blender by clicking within blender \"File \u003e\u003eImport\u003e\u003eselect the type of file you want to import\u003e\u003eopen file location of the downloaded unzipped files\u003e\u003eselect the file\u003e\u003ethe model would open in the 3d viewport of the software.\n\nThe other files including blender can be opened with most of the free and paid 3d modelling software. The files obj \u0026 fbx are compatible with other 3d modeling software, example maya. These software's have the open/import options similar to blender. The files stl and 3mf are compatible with 3d printing software's. The built in \"3d builder \" windows software opens all of these files including glb, \u0026 gltz. In case you don't have 3d builder installed just download it free from Microsoft store for free. \n\nFor 3d builder 3mf, fbx, stl, glb are standalone files (right click the model file\u003e\u003eselect open with\u003e\u003e3d builder). For obj,ply, \u0026 gltz 3d builder will prompt you to select the model files .mtl and image textures (these are packed in the rar files).\n\nThe textures files have been separately supplied additionally; in case one needs them.\n\n\n\n","imageAlt":"3D Liver histology anatomy labelled","url":"https://www.cgtrader.com/3d-models/science/medical/liver-histology-anatomy-labelled","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/MwpWLCPU5Skd3BMRGyRd15J7/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Screenshot%20%2825%29.jpg","gridUrl":"https://media.cgtrader.com/variants/MwpWLCPU5Skd3BMRGyRd15J7/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Screenshot%20%2825%29.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/science/medical/liver-histology-anatomy-labelled","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":21,"name":".blend","is_native":true},{"id":117,"name":".gltf","is_native":false},{"id":127,"name":".usdz","is_native":false},{"id":129,"name":".3mf","is_native":false},{"id":null,"name":null,"is_native":false},{"id":12,"name":".obj","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":51,"name":".stl","is_native":false},{"id":189,"name":".ply","is_native":false}],"categorySlug":"science","subcategorySlug":"medical","categoryTitle":"Science","subcategoryTitle":"Medical","schemaImageUrl":"https://img-new.cgtrader.com/items/5005684/f73aad51b6/liver-histology-anatomy-labelled-3d-model-f73aad51b6.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"2874957","type":"listingItem","attributes":{"id":2874957,"title":"Liver lobule histology","price":69.0,"description":"A blend model of liver depicting its microscopic details as well as its direction of blood and bile flow along with its anatomical lobule, portal triad, bile duct and fibrous boundries.\nThe formats 3mf, ply, obj, fbx, USDZ,GLTZ \u0026 GLB with applied uv mapped textures have also been included in the downloads along with  stl.\n\nI have included the various formats needed by various customer for the various 3d modelling softwares they may be using. \nThe following formats are compressed in rar formats :-\n1.\tblend\n2.\t3mf\n3.\tstl\n4.\tobj\n\n6.\tglb\n7.\tgltz\n8.\tusdz\nThe downloaded files have to unpacked using any rar unpacker. After unpacking, the folder content of the respective formats will be as follows :-.\n1.\tblend :- single file with all applied and packed textures.\n2.\t3mf :- single file with all applied and packed textures.\n3.\tstl :- single file with only geometry data\n4.\tobj :- mutiple files including .obj,.mtl, images textures.\n\n6.\tglb :- single file with all applied and packed textures.\n7.\tgltz :- mutiple files including .bin, images textures.\n8.\tusdz :- single file \n\nThe native file is blend so the open source software blender opens mostly all the files, with textures (packed with the files). The best way is to open the files named blend with blender. Other files have to be imported in blender by clicking within blender \"File \u003e\u003eImport\u003e\u003eselect the type of file you want to import\u003e\u003eopen file location of the downloaded unzipped files\u003e\u003eselect the file\u003e\u003ethe model would open in the 3d viewport of the software.\nThe other files including blender can be opened with most of the free and paid 3d modelling software. The files obj \u0026 fbx are compatible with other 3d modeling software, example maya. These software's have the open/import options similar to blender. The files stl and 3mf are compatible with 3d printing software's. The built in \"3d builder \" windows software opens all of these files including glb, \u0026 gltz. In case you don't have 3d builder installed just download it free from Microsoft store for free. \nFor 3d builder 3mf, fbx, stl, glb are standalone files (right click the model file\u003e\u003eselect open with\u003e\u003e3d builder). For obj,ply, \u0026 gltz 3d builder will prompt you to select the model files .mtl and image textures (these are packed in the rar files).\nThe textures files have been separately supplied additionally; in case one needs them.\n\n\n","imageAlt":"3D model Liver lobule histology","url":"https://www.cgtrader.com/3d-models/science/medical/liver-lobule-histology","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/vaAScw37q1KdnVpFcxFWpQpG/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/0001.jpg","gridUrl":"https://media.cgtrader.com/variants/vaAScw37q1KdnVpFcxFWpQpG/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/0001.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/science/medical/liver-lobule-histology","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":21,"name":".blend","is_native":true},{"id":127,"name":".usdz","is_native":false},{"id":189,"name":".ply","is_native":false},{"id":117,"name":".gltf","is_native":false},{"id":51,"name":".stl","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":129,"name":".3mf","is_native":false}],"categorySlug":"science","subcategorySlug":"medical","categoryTitle":"Science","subcategoryTitle":"Medical","schemaImageUrl":"https://img-new.cgtrader.com/items/2874957/da1ba35b26/liver-lobule-histology-3d-model-da1ba35b26.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"2411692","type":"listingItem","attributes":{"id":2411692,"title":"Apple set 2 with slice taken out of it","price":10.99,"description":"Apple set\n- Three models of whole apple.\n- Three models of half of apple.\n- Three models of quarter of apple.\n- Three types of texture for each sets of models (by sort: golden, simirenko, gala).\n\n- The models was created separately for the Vray and Corona render.\n- All materials and objects in the scene have logical names in English, so you can easily understand what material you need to apply to which object.\n- All objects in the scene were prepared for smoothing.\n- All models have unwrapUVs.\n\nPolycount: without smoothing - 15461; with smoothing (two iterations) - 491880.\n\nWho works in the V-Ray version lower than 3.1, be careful, in the materials in the BRDF section there is Microfaset GTR (GGX), if your version is older than 3.1, then the BRDF field will be empty. Choose Blinn, Phong or Ward - which is preferable for you.\nFor Corona render, it is recommended to install a version of at least 1.5, since the glossiness of materials is configured with PBR in mind.","imageAlt":"Apple set 2 with slice taken out of it 3D","url":"https://www.cgtrader.com/3d-models/food/fruit/apple-set-c0a599b5-ba92-482c-b4f7-236e92d35dec","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/69EV2rzV37qedam7LNE12htY/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/all.jpg","gridUrl":"https://media.cgtrader.com/variants/69EV2rzV37qedam7LNE12htY/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/all.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/food/fruit/apple-set-c0a599b5-ba92-482c-b4f7-236e92d35dec","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":185,"name":".mat","is_native":false},{"id":null,"name":null,"is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false}],"categorySlug":"food","subcategorySlug":"fruit","categoryTitle":"Food","subcategoryTitle":"Fruit","schemaImageUrl":"https://img-new.cgtrader.com/items/2411692/11564f7acc/apple-set-2-with-slice-taken-out-of-it-3d-model-11564f7acc.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"3457244","type":"listingItem","attributes":{"id":3457244,"title":"Tangerines in a tall bowl","price":29.0,"description":"Tangerines in a tall bowl\n\nBowl approximate size: 200mm\n\nModels made using photogrammetry, retopologized, texture 4096x4096px\n\nInstance models\n\nModels have a light mesh density\nThe weight of all models is about 1.6mb\n\nEditable mesh\nmax2013 Corona + Vray\nFBX2009 Corona + Vray\n\nPolys - 114224\nVerts - 57159\n\nVray + Corona materials\n\nSuitable for kitchen, cafe, bar, restaurant, shop. 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For the psychologist, see Star Vega (psychologist). For other uses, see Vega (disambiguation). Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years (7.7 parsecs) from the Sun, and one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed arguably the next most important star in the sky after the Sun. Vega was the northern pole star around 12,000 BCE and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system. Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their main sequence lifetimes. Compared with the Sun, Vega has a lower abundance of elements heavier than helium. Vega is also a variable star—that is, a star whose brightness fluctuates. It is rotating rapidly with a speed of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles. Based on observations of more infrared radiation than expected, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars. 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It is now thought that a typical Bok globule contains about 10 solar masses of material in a region about a light-year or so across, and that Bok globules most commonly result in the formation of double- or multiple-star systems.\n\nTexture Resolution: 700 x 700","imageAlt":"3D Bootes Void","url":"https://www.cgtrader.com/3d-models/space/other/bootes-void","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/ELau3mYurgSMj97ki4NDiTeb/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/bo%C3%B6tes%20void.jpg","gridUrl":"https://media.cgtrader.com/variants/ELau3mYurgSMj97ki4NDiTeb/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/bo%C3%B6tes%20void.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/bootes-void","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5801932/7ee165cfda/bootes-void-3d-model-7ee165cfda.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5744641","type":"listingItem","attributes":{"id":5744641,"title":"tv wall 2024","price":7.0,"description":"mur tv \nmobile\nmobile tv","imageAlt":"tv wall 2024 3D print model","url":"https://www.cgtrader.com/3d-print-models/house/decor/tv-wall-2024","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/hTV3fJT62inBQmMZLD8gdLeL/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/WhatsApp%20Image%202024-12-03%20%C3%A0%2019.06.42_3f3267ea.jpg","gridUrl":"https://media.cgtrader.com/variants/hTV3fJT62inBQmMZLD8gdLeL/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/WhatsApp%20Image%202024-12-03%20%C3%A0%2019.06.42_3f3267ea.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-print-models/house/decor/tv-wall-2024","isCgtVerified":false,"types":{"printReady":true,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":14,"name":".skp","is_native":false}],"categorySlug":"house","subcategorySlug":"decor","categoryTitle":"Home \u0026 Living","subcategoryTitle":"Home decor","schemaImageUrl":"https://img-new.cgtrader.com/items/5744641/0a62b1c8f3/tv-wall-2024-3d-model-0a62b1c8f3.webp","saleOffDiscount":50,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":true}},{"id":"4108130","type":"listingItem","attributes":{"id":4108130,"title":"HD HEAD BOBBLE HEAD","price":9.0,"description":"'HD HEADS' ARE A COLLECTION OF MODELS  THAT  ARE HIGHLY DETAILED  RIGHT DOWN TO  THE  FINE WRINKLES AND PORES, GIVING YOU A CHANCE TO TEST BOTH YOURSELF AND YOUR PRINTER TO SEE WHAT KIND OF  DETAILED RESULTS YOU CAN ACHIEVE. THE MODELS ARE  OF A SIMILAR  SCALE  AND STYLE AND POSED WITH AN EXPRESSIVE LOOK ON THE FACE TO ADD BOTH CHARACTER AND EMOTION TO EACH MODEL.\n\n\n ALL FILES ARE CLEAN AND READY TO GO, ALL OF THE MESH'S HAVE BEEN RUN THROUGH MESHMIXERS 'ANALYSIS/INSPECTOR'  TOOLS TO FIX ANY BAD TOPOLOGY AFTER SCULPTING (NON-MANIFOLD); AND ALL OF THE OBJ/STL FILES WERE GENERATED WITHIN MESHMIXER.\n    \n          1.    THE MODELS ARE IN BOTH STL \u0026 OBJ FORMATS\n\n\t2. EACH  MODEL SIZE IS 150MM TALL AS STANDARD, THIS CAN OBVIOUSLY BE RE-SCALED IN YOUR OWN SLICER SOFTWARE TO YOUR OWN PREFERENCES.\n\t\n\t3. THE MODELS ARE IDEAL FOR PEOPLE WITH HD RESIN PRINTERS, BUT EXCELLENT DETAILED RESULTS CAN ALSO BE ACHIEVED WITH FDM PRINTERS IF THE MODELS ARE PRINTED IN A LARGER SCALE  SO THE DETAILS OF THE MODELS CAN STILL BE CAPTURED WITHIN THE SLICING SOFTWARE.\n\t\n\t4. THE MODELS ARE HIGH-RES, TOTALING APPROX 1,000,000 POLYS  SO THERE.S NO LOSS OF DETAIL AND THE MODELS CAN BE PRINTED LARGE SCALE WITH NO FLAT FACETING.\n\nHOPE YOU ENJOY PRINTING THEM, IF THERE'S A GOOD RESPONSE I'LL ADD MORE.\n","imageAlt":"3D printable model HD HEAD BOBBLE HEAD","url":"https://www.cgtrader.com/3d-print-models/miniatures/other/hd-head-bobble-head","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/7YM1Rf9T3sF3szDAyvV6z9YB/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/BOBBLE%20HEAD%20HD%201.jpg","gridUrl":"https://media.cgtrader.com/variants/7YM1Rf9T3sF3szDAyvV6z9YB/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/BOBBLE%20HEAD%20HD%201.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-print-models/miniatures/other/hd-head-bobble-head","isCgtVerified":false,"types":{"printReady":true,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":51,"name":".stl","is_native":false},{"id":12,"name":".obj","is_native":false}],"categorySlug":"miniatures","subcategorySlug":"other","categoryTitle":"Miniatures","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/4108130/bda4253ad4/hd-head-bobble-head-3d-model-bda4253ad4.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6765028","type":"listingItem","attributes":{"id":6765028,"title":"Tidal Power Double Turbine","price":69.0,"description":"- This model contains 120 separate objects.\n- Each object consists of 35,816 polygons with MeshSmooth OFF.\n- This asset contains a total of 141,315 polygons with MeshSmooth set to 1 iteration (applied to all objects, each mesh ready for subdivision).\n- This product includes 3ds Max 2017 versions for V-Ray 5.\n- The mesh consists of 99% quadrilateral polygons and does not contain Ngons or poles.\n- Marmoset renderings with Subdivision level 0\n- Turntable made with Marmoset\n\n- Thumbnails Scene Totals:\n- Scene Totals:\n- Objects: 121\n- Shapes: 0\n- Cameras: 1\n- Lights: 5\n- Helpers: 2\n- Space Warps: 0\n- Total: 129\n\n- Mesh Totals:\n\n- Verts: 149892\n- Faces: 143391\n\n**- IITEXTURESII**\n\n- 4096 x 4096 x 20\n- PBR - Metallic/Roughness/Base Color/Normal/AO maps.\n\n**- || GENERAL ||**\n\n- The model is built to real-world scale.\n- Units used: Centimeters. The model is 2529 cm high.\n- Scene objects are organized by layers and groups.\n\n**- || ADDITIONAL NOTES **||\n\n- FBX and OBJ file formats do not have textures/materials applied and will not render like the preview images.\n- File formats other than 3ds Max are exported as the base mesh (not smoothed).","imageAlt":"Tidal Power Double Turbine 3D asset","url":"https://www.cgtrader.com/3d-models/industrial/industrial-machine/tidal-power-double-turbine","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/yqp1gaf0n8y2fgqielpiz6hfzcbe/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/tidal-power-double-turbine-3d-model-6766174561.jpg","gridUrl":"https://media.cgtrader.com/variants/yqp1gaf0n8y2fgqielpiz6hfzcbe/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/tidal-power-double-turbine-3d-model-6766174561.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/industrial/industrial-machine/tidal-power-double-turbine","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":true}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":215,"name":".png","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false}],"categorySlug":"industrial","subcategorySlug":"industrial-machine","categoryTitle":"Industrial","subcategoryTitle":"Machine","schemaImageUrl":"https://img-new.cgtrader.com/items/6765028/6766174561/tidal-power-double-turbine-3d-model-6766174561.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5801879","type":"listingItem","attributes":{"id":5801879,"title":"Giant GRB Ring","price":3.0,"description":"Description\n\nGiant GRB Ring. The Giant GRB Ring is like a rock or cloud. The Giant GRB Ring is a ring of 9 gamma-ray bursts (GRBs) that may be associated with one of the largest known cosmic structures. It was discovered in July 2015 by a team of Hungarian and American astronomers led by L.G. Balazs while analyzing data from different gamma-ray and X-ray telescopes, in particular the Swift Spacecraft. The ring of GRBs lies at a distance of about 2.8 gigaparsecs (9.1 billion light years) from Earth at the redshift between 0.78 and 0.86 and measures about 1.72 gigaparsecs (5.6 billion light years) in diameter, making it one of the largest structures known. Typically, the distribution of GRBs in the universe appears in the sets of less than the 2σ distribution, or with fewer than two GRBs in the average data of the point-radius system. Thus, such a concentration as this appears extremely unlikely, given accepted theoretical models. Proposals include the existence of a giant supergalactic structure. This would be an extremely huge structure of the universe, with a mean size of about 5.6 billion light years. Such a supercluster can explain the significant distribution of GRBs because of its tie to star formation. 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Studies of the motion of these clusters show that they have no interaction to each other, meaning the density of the clusters is very low resulting in weak gravitational interaction. The void's location in the sky is close to the Boötes Void. 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It is featuring a pink and white checkered scarf.\nThe 3D Model is part of the Polygonal Miniatures Remastered collection, which has been optimized with better shaders, correct scaling (meters) and centered position.\nWe use multi camera capturing in the 3D scanning process. The scan data is cleaned and processed in Zbrush and Photoshop. \nIn the end, the low poly product contains unwrapped UV's, textures and normals maps. Detailed specifications can be found below:\n\nModel Info:\n\n- **Polygons**: 30,032\n- **Vertices**: 15,170\n- **File Formats**: .fbx, .usd, .glb, .obj, .dae, .blend\n- **Real-World Scale**: meters\n\nMap Info:\n\n- **Diffuse**: 4,096 x 4,096 (.jpg)\n- **Normal**: 4,096 x 4,096 (.jpg)\n\nIf you experience any issue with this model after purchase, feel free to contact me. \n\nEnjoy, and have a nice day!","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/character/clothing/headscarf-double-a2e304a7-b72e-4604-9b2d-df9dfff43a94","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/LBYTzfKhyuxeRubScWT5aL2p/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Headscarf_Double_00.jpg","gridUrl":"https://media.cgtrader.com/variants/LBYTzfKhyuxeRubScWT5aL2p/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Headscarf_Double_00.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/character/clothing/headscarf-double-a2e304a7-b72e-4604-9b2d-df9dfff43a94","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":true}},"metaverseFormatsList":[{"id":21,"name":".blend","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":117,"name":".gltf","is_native":false},{"id":25,"name":".dae","is_native":false},{"id":216,"name":".jpg","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":207,"name":".usd","is_native":false}],"categorySlug":"character","subcategorySlug":"clothing","categoryTitle":"Character","subcategoryTitle":"Clothing","schemaImageUrl":"https://img-new.cgtrader.com/items/5657106/4116f5acfd/headscarf-double-3d-model-4116f5acfd.webp","saleOffDiscount":50,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5819160","type":"listingItem","attributes":{"id":5819160,"title":"Boss Great Wall","price":3.0,"description":"Description\nDescription\n\nThe Boss Great Wall. The Boss Great Wall is like a spider web. The Boss Great Wall contains nebulas, including saturn nebula, hourglass nebula, cat eye nebula, stingray nebula, eskimo nebula, ring nebula, dumbbell nebula, twin-jet nebula, shrimp nebula, red spider nebula and etc. The Boss Great Wall also includes galaxies. The BOSS Great Wall is a supercluster complex that was identified, using the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey (SDSS), in early 2016. It was discovered by a research team from several institutions, consisting of: Heidi Lietzen, Elmo Tempel, Lauri Juhan Liivamägi, Antonio Montero-Dorta, Maret Einasto, Alina Streblyanska, Claudia Maraston, Jose Alberto Rubiño-Martín and Enn Saar. The BOSS Great Wall is one of the largest superstructures in the observable universe, though there are even larger structures known. The large complex has a mean redshift of z ~ 0.47 (z times Hubble length ≈ 6.8 billion light years). It consists of two elongated superclusters, two large superclusters, and several smaller superclusters as well. The elongated superclusters form galaxy walls, with the larger of the two having a diameter of 186/h Mpc (supercluster A in the figure); the second wall's being 173/h Mpc (supercluster B). The other two main superclusters are moderately large, having diameters of 91/h Mpc and 64/h Mpc (superclusters D and C, respectively). The superstructure is roughly 1 billion light years in diameter, and has a total mass approximately 10,000 times the Milky Way galaxy. It contains at least 830 visible galaxies (represented in the figure within their respective superclusters), as well as many others that are not visible (dark galaxies). The researchers used Minkowski functionals to verify the structure's overall shape and size; the first three quantifying the thickness, width, and length followed by the fourth determining the structure's overall curvature. The research team compared the luminosities and stellar masses within the superstructure to known high stellar mass galaxies within the SDSS's 7th data release, DR7. This allowed the team to scale the data using known values, from local superclusters, to determine the overall morphology of the BOSS Great Wall. It is currently debated amongst astronomers if the BOSS Great Wall may be considered a structure, due to the intricacies of its shape and overall size. The question of whether the supercluster complex is moving together or being slowly separated by the expanding universe is a key factor to this discussion. Nevertheless, when compared to several other chain structures, such as the Sloan Great Wall, the BOSS Great Wall's superclusters are far richer, containing more dense, high stellar mass galaxies. The BOSS Great Wall's discovery, and the data gained therein, should prove very beneficial for astronomers who study the overall structure of the cosmic web.\n\nTexture Resolution: 736 x 915","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/boss-great-wall-90b806b7-8c8e-4c4f-8628-896ac03518dc","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/kD2yZ8QTWn3Tq8JW1XVoVzvj/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/boss%20great%20wall-2.jpg","gridUrl":"https://media.cgtrader.com/variants/kD2yZ8QTWn3Tq8JW1XVoVzvj/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/boss%20great%20wall-2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/boss-great-wall-90b806b7-8c8e-4c4f-8628-896ac03518dc","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5819160/c93b8fb9c1/boss-great-wall-3d-model-c93b8fb9c1.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"1004148","type":"listingItem","attributes":{"id":1004148,"title":"Double Head Dragon Bracelet 2","price":40.0,"description":"Recommended material - silver or gold! \nApproximate metal weight (for lenght 180 mm): \ngold 14k – 58.3 grams; \ngold 18k – 69.8 grams; \nsilver 925 Sterling – 56.9 grams.\n\nModel avalible in STL format for prototyping. \nGeometry is healed, and fixed all the bad with RP Magics software \nYou can check out my other products by clicking on the author name \"artchagur\". \nAny questions? Please contact me. \nThank you!","imageAlt":"Double Head Dragon Bracelet 2 3D printable 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Sierra AT4X double cab 2022","price":159.0,"description":"---------------------------------------------------------------------------------------\n\n\n\t\tHigh detailed model created by SQUIR team.\n\n\n---------------------------------------------------------------------------------------\n\n\n\n\nReady to render at 3dsmax with VRAY 3 and also Corona 2\n\n\nTwo rendering studios are included for VRAY3 and Corona2, with all lightning, materials, background setups\n\n\n3dsmax 2010 format is also included, but without lightning/rendering studio setups and with standard materials only.\n\nOther than 3dsmax files (3ds,fbx,lwo,c4d,obj) include only standard materials without advanced shadders or background setup.\n\n3dsmax format is editable, with uncollapsed smoothing modifier. \nMaya format is editable with uncollapsed smoothing modifier.\nAll other formats are exported as a hipoly only!\n\n\nThe lowest available meshsmooth level for 3dsmax and Maya formats is shown at the wire view, next to the hipoly wire view.\n\n\nFor this product there's 3 different 3dsmax files included.\n\"Set\" is uncollapsed, it's a file where you can make changes at the model. \n\"Hipoly\" is collapsed to hipoly with all the modifiers history cleaned to make it trouble free  while using at other programs\n\"Studio\" is the file with all rendering setups that we used to make the previews renderings.\n\n\nBecause different computers have different disks topology, it might be necessary to change the textures patches on the destination computer.\n\n\n---------------------------------------------------------------------------------------\n\n\n\t\tThank you for buying SQUIR models\n\n\n---------------------------------------------------------------------------------------","imageAlt":"GMC Sierra AT4X double cab 2022 3D model sierra","url":"https://www.cgtrader.com/3d-models/car/car/gmc-sierra-at4x-double-cab-2022","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/CZyoJR5w4kMctT9t2Me4jVty/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/GMC_Sierra_AT4X_double_cab_2022_0000.jpg","gridUrl":"https://media.cgtrader.com/variants/CZyoJR5w4kMctT9t2Me4jVty/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/GMC_Sierra_AT4X_double_cab_2022_0000.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/car/car/gmc-sierra-at4x-double-cab-2022","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":5,"name":".fbx","is_native":false},{"id":8,"name":".lwo","is_native":false},{"id":2,"name":".3ds","is_native":false},{"id":11,"name":".ma","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":6,"name":".c4d","is_native":false},{"id":21,"name":".blend","is_native":false}],"categorySlug":"car","subcategorySlug":"car","categoryTitle":"Car","subcategoryTitle":"Standard","schemaImageUrl":"https://img-new.cgtrader.com/items/3536231/30c7442441/gmc-sierra-at4x-double-cab-2022-3d-model-30c7442441.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"4162973","type":"listingItem","attributes":{"id":4162973,"title":"Ferro Back Panel Double and Back Panel Water","price":7.0,"description":"Product includes a Ferro Back Panel Double \u0026 Back Panel Water\n\n\nBack Panel Double Pouch:\nhttps://ferroconcepts.com/products/adapt-back-panel-double-pouch\n\u003e The Back Panel Double Pouch adds substantial carry ability to the FCPC V5 by providing two large stacked general-purpose pockets. Full width zippers allow easy access and navigation of contents with or without gloves. Both top and bottom pouches are partially lined with loop Velcro for optional organizational solutions.\n\n7,834 Tris\n4k PBR textures\n\n\nBack Panel Water:\nhttps://ferroconcepts.com/products/adapt-back-panel-water\n\u003e The Back Panel Water provides storage for up to 1.75L hydration bladders/reservoirs. Equipped with side attachment zippers for quick and secure attachment to the FCPC V5 plate carrier and with a second set of zippers allowing it to be layered in between other ADAPT back panels for additional adaptability. See that’s why we name things the way we do.\n\n3,720 Tris\n4k PBR textures\n\n\nBack Panels compatible with eachother\nBack Panels fitted for the FCPC V5: https://payhip.com/b/ImwCt or https://www.cgtrader.com/3d-models/character/clothing/ferro-concepts-fcpc-v5\nFBX files.\nModel NOT scaled for printing.\nContact me on discord for support.","imageAlt":"Ferro Back Panel Double and Back Panel Water 3D asset","url":"https://www.cgtrader.com/3d-models/military/military-character/ferro-back-panel-double-and-back-panel-water","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/Z5yxcL7CnMU4Vy8kJ3xYQdzK/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Render1.jpg","gridUrl":"https://media.cgtrader.com/variants/Z5yxcL7CnMU4Vy8kJ3xYQdzK/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Render1.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/military/military-character/ferro-back-panel-double-and-back-panel-water","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":true}},"metaverseFormatsList":[{"id":5,"name":".fbx","is_native":false},{"id":216,"name":".jpg","is_native":false},{"id":215,"name":".png","is_native":false}],"categorySlug":"military","subcategorySlug":"military-character","categoryTitle":"Military","subcategoryTitle":"Character","schemaImageUrl":"https://img-new.cgtrader.com/items/4162973/092adb039e/ferro-back-panel-double-and-back-panel-water-3d-model-092adb039e.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5971725","type":"listingItem","attributes":{"id":5971725,"title":"GRB 090423","price":3.0,"description":"Description\nGRB 090423. This GRB 090423 is like a comet that's passing through the supernova explosion. GRB 090423 was a gamma-ray burst (GRB) detected by the Swift Gamma-Ray Burst Mission on April 23, 2009, at 07:55:19 UTC whose afterglow was detected in the infrared and enabled astronomers to determine that its redshift is z = 8.2, making it one of the most distant objects detected at that time with a spectroscopic redshift (GN-z11, discovered in 2016, has a redshift of 11). A gamma-ray burst is an extremely luminous event flash of gamma rays that occurs as the result of an explosion, and is thought to be associated with the formation of a black hole. The burst itself typically only lasts for a few seconds, but gamma-ray bursts frequently produce an \"afterglow\" at longer wavelengths that can be observed for many hours or even days after the burst. Measurements at these wavelengths, which include X-ray, ultraviolet, optical, infrared, and radio, enable follow-up study of the event. The finite speed of light means that GRB 090423 is also one of the earliest objects ever detected for which a spectroscopic redshift has been measured. The universe was only 630 million years old when the GRB occurred, and its detection confirms that massive stars were born and dying even very early on in the life of the universe. GRB 090423 and similar events provide a unique means of studying the early universe, as few other objects of that era are bright enough to be seen with today's telescopes. On April 23, 2009, at 07:55:19 UTC the Swift satellite detected a burst that lasted about 10 seconds and was located in the direction of the constellation Leo. Swift localized the field in which GRB 090423 occurred, and 77 seconds after the burst, the Swift UVOT Photometric System took a 150-second exposure of the field, but was unable to detect an optical or ultraviolet afterglow. A few minutes after its discovery, ground-based telescopes began observing the field. Within 20 minutes of the burst, Nial Tanvir and his team found an infrared source at the Swift position using the United Kingdom Infrared Telescope (UKIRT) on Mauna Kea, Hawaii. The initial observations taken by UKIRT were triggered autonomously via the eSTAR Project. They observed a drop off in flux beyond 1.13 micrometres with the VLT. Attributing this drop off to Lyman alpha absorption by neutral hydrogen in the intergalactic medium, they calculated a redshift of 8.2 for GRB 090423. The team of C.C. Thöne and Paolo D'Avanzo observed the afterglow of GRB 090423 using the Italian TNG 3.6m telescope located in the Canary Islands, Spain. They obtained two hours of spectra, which when combined, suggested a very weak signal at the position of the afterglow. They too saw a drop off in flux near 1.1 micrometres, and reported a redshift of 8.1 for GRB 090423, which is consistent, within error, of the redshift reported by Tanvir et al. The redshift of 8.1 suggest the burst may have lasted approximately 1.2 seconds in the local frame of the emitter, its duration being redshifted accordingly to the observed 10 seconds. The intergovernmental astronomy organisation, European Southern Observatory (ESO) operates the Very Large Telescope that obtained the spectrum reported by Tanvir et al. The GRB was not visible in Chile when Swift first detected the burst at 07:55 UTC, but was the following day at 03:00 UTC, which enabled the Gamma-Ray Burst Optical/Near-Infrared Detector (GROND) at La Silla Observatory to make observations of the burst, and find a photometric redshift consistent with the value reported elsewhere. The last observers to gather data during the event was the Combined Array for Research in Millimeter-wave Astronomy (CARMA) observatory. The observation of GRB 090423 by CARMA was taken at a frequency of 92.5 GHz. 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Henize 70 was first observed in 1950 in a survey of bright planetary nebulae. Based on appearance it was proposed that it might be a supernova remnant. In 1956, it was added to a catalogue of Hα emission stars and nebulae by Karl Gordon Henize, where it was described as an emission nebula rather than a planetary nebula. A paper published in 1978 proposed that the formations of Henize 70 and other emission nebulae could be due to stellar winds. Later in 1981, a scientific article mentioned a higher likeliness of a supernova explosion forming the nebula instead of stellar winds. A 2014 study measured that Henize 70 featured high SII and Hα ratios, indicating that it is not a supernova remnant. 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The Southern Local Supervoid is like a fish. The Southern Local Supervoid is a tremendously large, nearly empty region of space (a void). It lies next to the Local Supercluster, which contains our galaxy the Milky Way. Its center is 96 megaparsecs away and the void is 112 megaparsecs in diameter across its narrowest width. Its volume is very approximately 600 billion times that of the Milky Way. 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For the psychologist, see Star Vega (psychologist). For other uses, see Vega (disambiguation). Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years (7.7 parsecs) from the Sun, and one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed \"arguably the next most important star in the sky after the Sun\". Vega was the northern pole star around 12,000 BCE and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system. Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their main sequence lifetimes. Compared with the Sun, Vega has a lower abundance of elements heavier than helium. Vega is also a variable star—that is, a star whose brightness fluctuates. It is rotating rapidly with a speed of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles. Based on observations of more infrared radiation than expected, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars. Observations by the James Webb Space Telescope show that the disk is exceptionally smooth, with no evidence of shaping by massive planets, though there is some evidence that there may be one or more Neptune-mass planets closer to the star.\n\nTexture Resolution: 1014 x 1024","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/vega-cluster","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/XV4Xk8tcAggxH7Ji2j1e6xqJ/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/vega%20cluster.jpg","gridUrl":"https://media.cgtrader.com/variants/XV4Xk8tcAggxH7Ji2j1e6xqJ/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/vega%20cluster.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/vega-cluster","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5811055/1356515d6d/vega-cluster-3d-model-1356515d6d.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5801727","type":"listingItem","attributes":{"id":5801727,"title":"Bok Globules","price":3.0,"description":"Description\n\nBok Globules. The Bok Globules is like a boot or sock. In astronomy, Bok globules are isolated and relatively small dark nebulae containing dense cosmic dust and gas from which star formation may take place. Bok globules are found within H II regions, and typically have a mass of about two to 50 solar masses contained within a region about a light year or so across (about 4.5×1047 m3). They contain molecular hydrogen (H2), carbon oxides and helium, and around 1% (by mass) silicate dust. Bok globules most commonly result in the formation of double- or multiple-star systems. An analysis of near-infrared observations published in 1990 confirmed that stars were being born inside Bok globules. Further observations have revealed that some Bok globules contain embedded warm sources, some contain Herbig–Haro objects, and some show outflows of molecular gas. Millimeter-wave emission line studies have provided evidence for the infall of material onto an accreting protostar. It is now thought that a typical Bok globule contains about 10 solar masses of material in a region about a light-year or so across, and that Bok globules most commonly result in the formation of double- or multiple-star systems.\n\nTexture Resolution: 800 x 800","imageAlt":"Bok Globules 3D model","url":"https://www.cgtrader.com/3d-models/space/other/bok-globules","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/VWThTHDR28a5DJk3dk7bZmkz/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/bok%20globules.jpg","gridUrl":"https://media.cgtrader.com/variants/VWThTHDR28a5DJk3dk7bZmkz/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/bok%20globules.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/bok-globules","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5801727/c509a8c3f4/bok-globules-3d-model-c509a8c3f4.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5809251","type":"listingItem","attributes":{"id":5809251,"title":"Hercules Corona Borealis Great Wall","price":3.0,"description":"Description\nDescriptionDescription\n\nHercules Corona Borealis Great Wall. The Hercules Corona Borealis Great Wall is like a blue space sky with stars and white large dots. The Hercules–Corona Borealis Great Wall (HCB) or simply the Great Wall is a galaxy filament that is the largest known structure in the observable universe, measuring approximately 10 billion light-years in length (the observable universe is about 93 billion light-years in diameter). This massive superstructure is a region of the sky seen in the data set mapping of gamma-ray bursts (GRBs) that has been found to have a concentration of similarly distanced GRBs that is unusually higher than the expected average distribution. It was discovered in early November 2013 by a team of American and Hungarian astronomers led by István Horváth, Jon Hakkila and Zsolt Bagoly while analyzing data from the Swift Gamma-Ray Burst Mission, together with other data from ground-based telescopes. It is the largest known formation in the universe, exceeding the size of the Huge-LQG by about a factor of two. The overdensity lies at the Second, Third and Fourth Galactic Quadrants (NGQ2, NGQ3 and NGQ4) of the sky. Thus, it lies in the Northern Hemisphere, centered on the border of the constellations Draco and Hercules. The entire clustering consists of around 19 GRBs with the redshift ranges between 1.6 and 2.1. Typically, the distribution of GRBs in the universe appears in the sets of less than the 2σ distribution, or with less than two GRBs in the average data of the point-radius system.[clarification needed] One possible explanation of this concentration is the Hercules–Corona Borealis Great Wall. The wall has a mean size in excess of 2 billion to 3 billion parsecs (6 to 10 billion light-years). Such a supercluster can explain the significant distribution of GRBs because of its tie to star formation. Doubt has been placed on the existence of the structure in other studies, positing that the structure was found through biases in certain statistical tests, without considering the full effects of extinction. 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For the psychologist, see Star Vega (psychologist). For other uses, see Vega (disambiguation). Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years (7.7 parsecs) from the Sun, and one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed arguably the next most important star in the sky after the Sun. Vega was the northern pole star around 12,000 BCE and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system. Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their main sequence lifetimes. Compared with the Sun, Vega has a lower abundance of elements heavier than helium. Vega is also a variable star—that is, a star whose brightness fluctuates. It is rotating rapidly with a speed of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles. Based on observations of more infrared radiation than expected, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars. 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For the psychologist, see Star Vega (psychologist). For other uses, see Vega (disambiguation). Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years (7.7 parsecs) from the Sun, and one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed arguably the next most important star in the sky after the Sun. Vega was the northern pole star around 12,000 BCE and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system. Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their main sequence lifetimes. Compared with the Sun, Vega has a lower abundance of elements heavier than helium. Vega is also a variable star—that is, a star whose brightness fluctuates. It is rotating rapidly with a speed of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles. Based on observations of more infrared radiation than expected, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars. Observations by the James Webb Space Telescope show that the disk is exceptionally smooth, with no evidence of shaping by massive planets, though there is some evidence that there may be one or more Neptune-mass planets closer to the star.\n\nTexture Resolution: 1001 x 1024","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/vega-cluster-60665dd8-2c1e-4d89-a543-3d0f73f9c9c0","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/Zo3YziS9yzpd6aXE92qN92EA/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/vega%20cluster-2.jpg","gridUrl":"https://media.cgtrader.com/variants/Zo3YziS9yzpd6aXE92qN92EA/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/vega%20cluster-2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/vega-cluster-60665dd8-2c1e-4d89-a543-3d0f73f9c9c0","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5811547/305c95866d/vega-cluster-3d-model-305c95866d.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"2415293","type":"listingItem","attributes":{"id":2415293,"title":"Liberty Double Eagle Gold Coin","price":20.0,"description":"WEIGHT IN GOLD 18 K : 22.04 GR\nWEIGHT IN SILVER 925 : 16.55 GR \nThe $10 Liberty Eagle Gold Coin was struck by the United States Mint from 1838 through 1907. The Gold Liberty Eagle's obverse was designed by Christian Gobrecht and is also known as the \"Coronet head\" eagle due to the artist's left-facing portrait of Lady Liberty in a coronet cap inscribed with \"LIBERTY\". The $10 Gold Liberty Eagle's reverse side features a heraldic eagle with wings outstretched, a cluster of arrows in one claw and an olive branch in the other. Also inscribed on the reverse is, \"UNITED STATES OF AMERICA\" and \"TEN D.\". This design was used for nearly 70 years with only a slight change in the portrait in 1839, and the addition of the motto IN GOD WE TRUST banner on the reverse side in 1866. $10 Liberty Eagle Coins without the \"In God We Trust\" banner on the reverse side are referred to as \"No Motto\" coins, and the coins that were minted with the banner are known as \"With Motto\". The gold Liberty Head Eagle coins that were produced at the U.S. mints in Carson City (CC), Denver (D), New Orleans (O), and San Francisco (S) all have a mint mark that can be found on the reverse side just beneath the eagle. Gold $10 Liberty Head eagles that were minted at the U.S. Philadelphia mint do not contain a mint mark at all. ","imageAlt":"3D printable model Liberty Double Eagle Gold Coin","url":"https://www.cgtrader.com/3d-print-models/jewelry/pendant/liberty-double-eagle-gold-coin","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/scY8ZPjKdqoG36yHEyjAjcfL/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/3.jpg","gridUrl":"https://media.cgtrader.com/variants/scY8ZPjKdqoG36yHEyjAjcfL/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/3.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-print-models/jewelry/pendant/liberty-double-eagle-gold-coin","isCgtVerified":false,"types":{"printReady":true,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":51,"name":".stl","is_native":false},{"id":13,"name":".3dm","is_native":false}],"categorySlug":"jewelry","subcategorySlug":"pendant","categoryTitle":"Jewelry","subcategoryTitle":"Pendants","schemaImageUrl":"https://img-new.cgtrader.com/items/2415293/ef60d11266/liberty-double-eagle-gold-coin-3d-model-ef60d11266.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6453820","type":"listingItem","attributes":{"id":6453820,"title":"Henize 70","price":3.0,"description":"Description\nHenize 70 (N70) is a faint emission nebula and superbubble located in the Large Magellanic Cloud in the constellation of Dorado. Henize 70 was first observed in 1950 in a survey of bright planetary nebulae. Based on appearance it was proposed that it might be a supernova remnant. In 1956, it was added to a catalogue of Hα emission stars and nebulae by Karl Gordon Henize, where it was described as an emission nebula rather than a planetary nebula. A paper published in 1978 proposed that the formations of Henize 70 and other emission nebulae could be due to stellar winds. Later in 1981, a scientific article mentioned a higher likeliness of a supernova explosion forming the nebula instead of stellar winds. A 2014 study measured that Henize 70 featured high SII and Hα ratios, indicating that it is not a supernova remnant. Henize 70 has spectral line ratios relatively similar to that of supernova remnants due to having similar SII/Hα line ratios although most supernova remnants have higher NII/Hα line ratios.\n\nTexture Resolution: 2048 x 1615","imageAlt":"3D Henize 70","url":"https://www.cgtrader.com/3d-models/space/other/henize-70","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/tyb34z90wp37lkb5w2n9m3zounam/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/henize%2070.jpg","gridUrl":"https://media.cgtrader.com/variants/tyb34z90wp37lkb5w2n9m3zounam/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/henize%2070.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/henize-70","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/6453820/a059861812/henize-70-3d-model-a059861812.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6456310","type":"listingItem","attributes":{"id":6456310,"title":"Musica Star","price":3.0,"description":"Description\n18 Delphini, also named Musica is a single star in the constellation of Delphinus of the low northern hemisphere. It has a Sun-like golden hue and is faintly visible to the naked eye with an apparent visual magnitude of 5.506. The star is located at a distance of approximately 245 light-years from the Sun based on parallax, and it is drifting further away with a radial velocity of +4 km/s. An object believed to be an extrasolar planet (designated 18 Delphini b or Arion) orbits the star. 18 Delphini is the star's Flamsteed designation, abbreviated 18 Del. Following its discovery the planet was designated 18 Delphini b. As part of the NameExoWorlds program by the International Astronomical Union, in 2015 the name Musica, Latin for 'music', was selected for this star by Tokushima Prefectural Jonan High School Science Club of Japan. The planet was given the name Arion, after a genius of poetry and music in ancient Greece. According to legend, his life was saved at sea by dolphins after attracting their attention by the playing of his kithara. The constellation 'Delphinus' is Latin for 'dolphin'. The stellar classification of 18 Delphini is G6III, which means it is an evolved star that has cooled and expanded off the main sequence. It is a suspected red clump giant that is generating energy from core helium fusion. A moderate level of X-ray emission has been detected from this star, which suggests it has a mildly active chromosphere. The star is 650 million years old with more than double the mass of the Sun, and has expanded to seven times the Sun's radius. It is radiating 34 times the luminosity of the Sun from its photosphere at an effective temperature of 5,071 K. The Washington Double Star Catalogue lists a pair of visual companions for this star. Component B is magnitude 9.88 and lies at an angular separation of 197.5 arcseconds along a position angle (PA) of 162° from the brighter star as of 2003. Component C has a magnitude of 12.77 with a separation of 129.3 arcseconds as of 2000. The proper motion of both stars are diverging significantly from 18 Delphini, so they can be ruled out as physical companions. However, a faint star located 29.2″ away appears to be a co-moving companion. This has a projected separation of 2,199 AU and a mass estimated as 19% that of the Sun. It is a small red dwarf star with a class of M4–5.\n\nTexture Resolution: 800 x 800","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/musica-star","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/hiw1fkq4hycyoqdkgjoaezha986o/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/musica%20star.jpg","gridUrl":"https://media.cgtrader.com/variants/hiw1fkq4hycyoqdkgjoaezha986o/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/musica%20star.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/musica-star","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/6456310/de78d076b0/musica-star-3d-model-de78d076b0.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5823059","type":"listingItem","attributes":{"id":5823059,"title":"Centaurus Cluster","price":3.0,"description":"Description\n\nCentaurus Cluster. The Centaurus Cluster is like a flying fish or albatross bird. The Centaurus Cluster (A3526) is a cluster of hundreds of galaxies, located approximately 170 million light-years away in the Centaurus constellation. The brightest member galaxy is the elliptical galaxy NGC 4696 (~11m). The Centaurus cluster shares its supercluster, the Hydra–Centaurus Supercluster, with IC4329 Cluster and Hydra Cluster. The cluster consists of two different sub-groups of galaxies with different velocities. Cen 30 is the main subgroup containing NGC 4696. Cen 45 which is centered on NGC 4709, is moving at 1500 km/s relative to Cen 30, and is believed to be merging with the main cluster.\n\nTexture Resolution: 2808 x 2957","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/centaurus-cluster","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/Z83oYdLt5RRb7PdWgi5tuU6C/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/centaurus%20cluster.jpg","gridUrl":"https://media.cgtrader.com/variants/Z83oYdLt5RRb7PdWgi5tuU6C/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/centaurus%20cluster.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/centaurus-cluster","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5823059/b0cb425c6b/centaurus-cluster-3d-model-b0cb425c6b.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5806410","type":"listingItem","attributes":{"id":5806410,"title":"Giant Void","price":3.0,"description":"Description\nDescription\n\nGiant Void. Giant Void is like a circle or teleportation portal. The Giant Void (also known as the Giant Void in NGH, Canes Venatici Supervoid, and AR-Lp 36) is an extremely large region of space with an underdensity of galaxies and located in the constellation Canes Venatici. It is the second-largest-confirmed void to date, with an estimated diameter of 300 to 400 Mpc (1 to 1.3 billion light-years) and its centre is approximately 1.5 billion light-years away (z = 0.116). It was discovered in 1988 and was the largest void in the Northern Galactic Hemisphere, and possibly the second-largest ever detected. Even the hypothesized Eridanus Supervoid corresponding to the location of the WMAP cold spot is dwarfed by this void, although the Giant Void does not correspond to any significant cooling to the cosmic microwave background. Inside this vast void there are 17 galaxy clusters, concentrated in a spherically shaped region 50 Mpc in diameter. Studies of the motion of these clusters show that they have no interaction to each other, meaning the density of the clusters is very low resulting in weak gravitational interaction. The void's location in the sky is close to the Boötes Void. In a series of papers published between 2004 and 2006, cosmologist and theoretical physicist Laura Mersini-Houghton presented a theory that the universe arose from a multiverse, and made a series of testable predictions which included the existence of the Giant Void.\n\nTexture Resolution: 1200 x 680","imageAlt":"Giant Void 3D","url":"https://www.cgtrader.com/3d-models/space/other/giant-void-8e4fcb7e-8c38-4ee4-a990-ca62569a658d","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/sdEgB1oP2RnyzGPx13S1HPcc/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/giant%20void-2.jpg","gridUrl":"https://media.cgtrader.com/variants/sdEgB1oP2RnyzGPx13S1HPcc/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/giant%20void-2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/giant-void-8e4fcb7e-8c38-4ee4-a990-ca62569a658d","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":215,"name":".png","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5806410/94da924ab8/giant-void-3d-model-94da924ab8.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"4219564","type":"listingItem","attributes":{"id":4219564,"title":"Double Cupholder-Phoneholder for Citroen C5 X7","price":10.0,"description":"The Citroen C5 X7 generation, launched in 2008, was mercilessly mocked and criticized for having a rather silly cupholder located inside the centre cubbyhole, beneath the armrest.\n\nThis solution comprises of using the tray beneath the radio and inserting this 3D printed double cupholder. It can hold various types of coffee cups, a 33cl can and small water bottles up to 0.5l in size. \n\nAlternatively, it can also be used as a smartphone holder, though it cannot do so while holding drinks and vice versa. It can hold a smartphone up to 176mm in height and around 13mm in thickness (including a phone case). There are alternative springs included to keep the phone in place. Please check the images and the video for further info. \n\nPLEASE MAKE SURE YOU WATCH THE VIDEO, as this solution may not be compatible with your particular C5 X7.\n\nThis is also a 100% reversible solution, so if you like, you can remove this and replace it with the original mat and use it just as before. It is recommended you use some Blue-tac/Bostik or whatever it's called in the location illustrated in one of the pictures to prevent rattling.\n\nThis model does not need supports EXCEPT where indicated in the pictures. The pieces that need support are in shown red in the general image listing the parts. Also, please watch the video for any information that may not be obvious from the images.\n\nIt is highly recommended you use ABS or some other kind of filament that is resistant to heat, as materials such as PLA will lead to the printed model melting if the car is left in the hot sun.","imageAlt":"Double Cupholder-Phoneholder for Citroen C5 3D print model","url":"https://www.cgtrader.com/3d-print-models/gadgets/other/double-cupholder-phoneholder-for-citroen-c5-x7","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/kTq3txPrktyeT9nTESxpZkNG/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Double%20Cupholder.00_09_24_16.Still008.jpg","gridUrl":"https://media.cgtrader.com/variants/kTq3txPrktyeT9nTESxpZkNG/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Double%20Cupholder.00_09_24_16.Still008.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-print-models/gadgets/other/double-cupholder-phoneholder-for-citroen-c5-x7","isCgtVerified":true,"types":{"printReady":true,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":51,"name":".stl","is_native":false}],"categorySlug":"gadgets","subcategorySlug":"other","categoryTitle":"Gadgets","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/4219564/e8748269dd/double-cupholder-phoneholder-for-citroen-c5-x7-3d-model-e8748269dd.webp","saleOffDiscount":50,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":true}},{"id":"3306428","type":"listingItem","attributes":{"id":3306428,"title":"Cherries single double triple","price":19.0,"description":"Texture set:\n- PBR textures 4096x4096 .png / Base Color / Metallic / Normal / (DirectX) / Roughnes / Height\n- PBR textures 4096x4096 .png /Diffuse / Glossiness / Specular / Normal (DirectX)\n- textures made in Substance Painter\n- 3ds Max; obj; fbx files have standard mat: spec/gloss textures\n\nGeometry:\n- Units: Centimeters\n- Polygons: 19894\n- Vertex: 19912\n- Triangles: 0\n- Quads: 19894\n- Ngons: 0\n- Vertex with more than 5 edges: 0\n\nObject:\n- Dimension cm: 12.1cm x 3.9cm x 5.7cm\n- Dimension inches: 4.75\" x 1.53\" x 2.24\"\n- Model parts: 9\n- Material count: 1\n- XForm: Yes\n- BoxTrick: Yes\n","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/food/fruit/cherries-single-double-triple","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/RVGpxvAxZWneXWbyvHACy5uZ/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/002.jpg","gridUrl":"https://media.cgtrader.com/variants/RVGpxvAxZWneXWbyvHACy5uZ/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/002.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/food/fruit/cherries-single-double-triple","isCgtVerified":true,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":5,"name":".fbx","is_native":false},{"id":17,"name":".max","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":null,"name":null,"is_native":false}],"categorySlug":"food","subcategorySlug":"fruit","categoryTitle":"Food","subcategoryTitle":"Fruit","schemaImageUrl":"https://img-new.cgtrader.com/items/3306428/21be383ccb/cherries-single-double-triple-3d-model-21be383ccb.webp","saleOffDiscount":50,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5864026","type":"listingItem","attributes":{"id":5864026,"title":"Saraswati Supercluster","price":3.0,"description":"Description\nSaraswati Supercluster. This Saraswati Supercluster is like a lizard. The Saraswati Supercluster is a massive galaxy supercluster about 1.2 gigaparsecs (4 billion light years) away within the Stripe 82 region of SDSS, in the direction of the constellation Pisces. It is one of the largest structures found in the universe, with a major axis in diameter of about 200 Mpc (652 million light years). It consists of at least 43 galaxy clusters, and has the mass of 2 × 1016 MO, forming a galaxy filament. The Saraswati supercluster was discovered by a team of astrophysicists from the Inter-University Centre for Astronomy and Astrophysics and Indian Institute of Science Education and Research led by Joydeep Bagchi and colleagues in Pune, India in 2017. Analyzing the data of Stripe 82 of the comprehensive Sloan Digital Sky Survey, particularly the sets of LOWZ data from the Baryon Oscillation Spectroscopic Survey, part of the DR12 catalogue of the SDSS, the team discovered an overdensity of the sampled 625 galaxies from LOWZ and 3,016 from the LEGACY-BOSS-SOUTHERN, a survey of the southern sky that is also a part of SDSS DR12. It was named after the Hindu goddess of knowledge Saraswati, as well as the mythological Sarasvati river; since the Sanskrit name also means “ever flowing stream with many pools”, and the supercluster has many clusters and groups moving and merging together. The Saraswati Supercluster is one of the largest and most massive superclusters known, comparable to the massive Shapley Concentration in the nearby universe. The supercluster consists of 43 massive galaxy clusters, the most massive being Abell 2631 and ZwCL 2341.1+0000 respectively. It is surrounded by a network of galaxy filaments, clusters, and voids. The Saraswati supercluster and its environs reveal that some extreme large-scale, prominent matter density enhancements had formed in the past when dark energy had just started to dominate structure formation. This galactic concentration sheds light on the role of dark energy and cosmological initial conditions in supercluster formation.\n\nTexture Resolution: 1280 x 720","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/saraswati-superluster","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/Rdc36JRh6iH9vi1y9ccNHfsC/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/saraswati%20cluster.jpg","gridUrl":"https://media.cgtrader.com/variants/Rdc36JRh6iH9vi1y9ccNHfsC/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/saraswati%20cluster.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/saraswati-superluster","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":215,"name":".png","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5864026/7a8bba940d/saraswati-supercluster-3d-model-7a8bba940d.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5850766","type":"listingItem","attributes":{"id":5850766,"title":"Pandoras Cluster","price":3.0,"description":"Description\n\nPandora's Cluster(Abell 2744), nicknamed Pandora's Cluster, is a giant galaxy cluster resulting from the simultaneous pile-up of at least four separate, smaller galaxy clusters that took place over a span of 350 million years, and is located approximately 4 billion light years from Earth. The galaxies in the cluster make up less than five percent of its mass. The gas (around 20 percent) is so hot that it shines only in X-rays. Dark matter makes up around 75 percent of the cluster's mass. This cluster also shows a radio halo along with several other Abell clusters. It has a strong central halo, along with an extended tail, which could either be relic radiation, or an extension of the central halo. Renato Dupke, a member of the team that discovered the Cluster, explained the origin of the name in an interview: \"We nicknamed it ‘Pandora's Cluster’ because so many different and strange phenomena were unleashed by the collision.\" In February 2023, NASA's James Webb Space Telescope captured unprecedented details of Abell 2744, revealing previously unseen galaxies and offering insights into the early universe. This remarkable observation underscores the ongoing exploration of Pandora's Cluster and its significance in understanding cosmic evolution.\n\nTexture Resolution: 8068 x 8067","imageAlt":"3D model Pandoras Cluster","url":"https://www.cgtrader.com/3d-models/space/other/pandoras-cluster","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/tE5KRrVY5H4ckFW7JYd4USnM/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/pandoras%20cluster.jpg","gridUrl":"https://media.cgtrader.com/variants/tE5KRrVY5H4ckFW7JYd4USnM/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/pandoras%20cluster.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/pandoras-cluster","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5850766/59c16768b2/pandoras-cluster-3d-model-59c16768b2.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6455952","type":"listingItem","attributes":{"id":6455952,"title":"Alcor and Mizar Stars","price":3.0,"description":"Description\nMizar and Alcor are two stars forming a naked eye double in the handle of the Big Dipper (or Plough) asterism in the constellation of Ursa Major. Their magnitudes are 2.2 and 3.9, and the pair can easily be seen without the aid of a telescope. Mizar and its fainter companion Alcor are actually a four-star binary system consisting of two pairs of double stars that are gravitationally bound to each other. The traditional name Mizar derives from the Arabic المئزر or mi'zar, meaning 'apron; wrapper, cover'. Alcor was originally the Arabic سها or suhā/sohā, meaning either 'the forgotten' or 'neglected one'. The ancient Persians and the Bedouins used distinguishing Mizar and Alcor as a test of vision.\nMizar, also designated Zeta Ursae Majoris (ζ Ursae Majoris, abbreviated Zeta UMa, ζ UMa), is itself a quadruple system and Alcor, also designated 80 Ursae Majoris (80 UMa), is a binary star, the pair together forming a sextuple system. Mizar was the first known binary star system, claimed to be discovered by Italian astronomer Giovanni Battista Riccioli in 1650. The whole system lies about 83 light-years away from the Sun, as measured by the Hipparcos astrometry satellite.\nWith normal eyesight Alcor appears at about 12 arcminutes from Mizar. Alcor is of magnitude 3.99 and spectral class A5V. It has a faint red dwarf companion separated by 1 arcsecond. Mizar and Alcor's proper motions show they move together, along with most of the other stars of the Big Dipper except Alpha Ursae Majoris and Eta Ursae Majoris, as members of the Ursa Major moving group, a mostly dispersed group of stars sharing a common birth. However, it has yet to be demonstrated conclusively that they are gravitationally bound. Parallax measurements by Gaia indicate that Alcor and Mizar are somewhat closer together than previously thought: 0.36±0.19 pc. The uncertainty is due to not knowing exactly how far away the stars are. If they are exactly the same distance from us then the distance between them is only 17800 AU (0.281 ly). Between Mizar and Alcor, the 8th-magnitude star Sidus Ludoviciana is a distant background object.\nAlcor Star is located on lower left and Mizar Star is located on upper center.\n\nTexture Resolution: 1172 x 896","imageAlt":"Alcor and Mizar Stars 3D","url":"https://www.cgtrader.com/3d-models/space/other/alcor-and-mizar-stars","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/k2ioklp18bltei3yvmsvw0mxt3xq/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/alcor%20and%20mizar%20stars.jpg","gridUrl":"https://media.cgtrader.com/variants/k2ioklp18bltei3yvmsvw0mxt3xq/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/alcor%20and%20mizar%20stars.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/alcor-and-mizar-stars","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/6455952/23fdf693ee/alcor-and-mizar-stars-3d-model-23fdf693ee.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"3616935","type":"listingItem","attributes":{"id":3616935,"title":"3D Best Double Decker Bus","price":149.0,"description":"Single Cabin Double Decker Bus which belongs to BEST\n\nIt was first introduced in 1937,\nOnce Bombay had 242 buses, today there are only 122 commuters and due to electrical buses are introducing nowadays this Legendary bus is getting obsolete. So to preserve such beloved passenger vehicle, i created this in 3D format.\n\nThis model was created with the 3ds max and blender later textured with substance painter and rendered with marmoset toolbag.\n\nHighpoly PBR Model. This model is not rigged, but all the moveable parts are separated, so the model can be easily rigged and animated. The model has 2K textures set.\n\nThis Model Contains:\nPolygons - 2840879\nVertexs - 2568335\n\nModel formats:\n- *.Blender (2.93.5)\n- *.FBX (Multi Format)\n- *.OBJ (Multi Format)\n\nHope you guys like this and feel free to share the opinions in comments section.","imageAlt":"PBR 3D Best Double Decker Bus","url":"https://www.cgtrader.com/3d-models/vehicle/bus/3d-best-double-decker-bus","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/MWhDn7sGZWcvVAR5EBwmvna6/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Best_Double%20Decker%20Bus_View_7.jpg","gridUrl":"https://media.cgtrader.com/variants/MWhDn7sGZWcvVAR5EBwmvna6/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Best_Double%20Decker%20Bus_View_7.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/vehicle/bus/3d-best-double-decker-bus","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":21,"name":".blend","is_native":true},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":null,"name":null,"is_native":false}],"categorySlug":"vehicle","subcategorySlug":"bus","categoryTitle":"Vehicle","subcategoryTitle":"Bus","schemaImageUrl":"https://img-new.cgtrader.com/items/3616935/2592dc3976/3d-best-double-decker-bus-3d-model-2592dc3976.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"2962581","type":"listingItem","attributes":{"id":2962581,"title":"HeadScarf Double Tuck","price":19.99,"description":"**3D Photorealistic clothing item**\n\n- Multiple formats available: DAE, FBX, ZTL, OBJ, Maya\n- 3D scanned using photogrammetry\n- 4k Texture Map \u0026 Normal Map included (find them in the zip folder ending with _OBJ)\n- Polycount is suited for renders / film application or for realtime use in high-end gaming PC's.\n\nEnjoy!","imageAlt":"3D model HeadScarf Double Tuck","url":"https://www.cgtrader.com/3d-models/character/clothing/headscarf-double-tuck","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/S6SKkDq1BfnUg76z1C7nbZR2/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/headscarf-double-tuck-3d-model.jpg","gridUrl":"https://media.cgtrader.com/variants/S6SKkDq1BfnUg76z1C7nbZR2/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/headscarf-double-tuck-3d-model.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/character/clothing/headscarf-double-tuck","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":55,"name":".ztl","is_native":false},{"id":11,"name":".ma","is_native":false},{"id":25,"name":".dae","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":5,"name":".fbx","is_native":false}],"categorySlug":"character","subcategorySlug":"clothing","categoryTitle":"Character","subcategoryTitle":"Clothing","schemaImageUrl":"https://img-new.cgtrader.com/items/2962581/001a0de382/headscarf-double-tuck-3d-model-001a0de382.webp","saleOffDiscount":50,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5817834","type":"listingItem","attributes":{"id":5817834,"title":"Vega Star","price":3.0,"description":"Description\n\nStar Vega redirects here. For the psychologist, see Star Vega (psychologist). For other uses, see Vega (disambiguation). Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years (7.7 parsecs) from the Sun, and one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed arguably the next most important star in the sky after the Sun. Vega was the northern pole star around 12,000 BCE and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system. Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their main sequence lifetimes. Compared with the Sun, Vega has a lower abundance of elements heavier than helium. Vega is also a variable star—that is, a star whose brightness fluctuates. It is rotating rapidly with a speed of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles. Based on observations of more infrared radiation than expected, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars. Observations by the James Webb Space Telescope show that the disk is exceptionally smooth, with no evidence of shaping by massive planets, though there is some evidence that there may be one or more Neptune-mass planets closer to the star.\n\nTexture Resolution: 1600 x 1037","imageAlt":"3D model Vega Star","url":"https://www.cgtrader.com/3d-models/space/other/vega-cluster-b52926aa-4751-4a23-b87a-de5478345d50","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/jYMhxpz7mQMqzvHEZrSf4YxG/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/vega%20star2.jpg","gridUrl":"https://media.cgtrader.com/variants/jYMhxpz7mQMqzvHEZrSf4YxG/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/vega%20star2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/vega-cluster-b52926aa-4751-4a23-b87a-de5478345d50","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5817834/3426dacb56/vega-star-3d-model-3426dacb56.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"2735351","type":"listingItem","attributes":{"id":2735351,"title":"Double cab Truck Sprinter","price":35.0,"description":"The second generation Sprinter was introduced in Europe in 2006. It was voted Van of the Year 2007 and again in 2008 by Professional Van and Light Truck Magazine. \nMercedes-Benz Sprinter 2006 -2015. Freightliner Sprinter Dodge Sprinter (2007–2010) JAC Sunray (China)\n\nDimensions: 6,820mm (Length) x 2,380 mm (Height) x 2150mm\n\nPolys:141614 Verts:148619\nFormats: .max .fbx .obj \nRender: Corona, VRay. \nSuccessful renderings! See other models in my profile.","imageAlt":"Double cab Truck Sprinter 3D model","url":"https://www.cgtrader.com/3d-models/vehicle/truck/double-cab-truck-sprinter","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/zBLJznHB4NeNQEdir3oeFofv/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/01.jpg","gridUrl":"https://media.cgtrader.com/variants/zBLJznHB4NeNQEdir3oeFofv/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/01.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/vehicle/truck/double-cab-truck-sprinter","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false}],"categorySlug":"vehicle","subcategorySlug":"truck","categoryTitle":"Vehicle","subcategoryTitle":"Truck","schemaImageUrl":"https://img-new.cgtrader.com/items/2735351/5cda5f588f/double-cab-truck-sprinter-3d-model-5cda5f588f.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"3749017","type":"listingItem","attributes":{"id":3749017,"title":"Double Mouthpiece","price":14.0,"description":"3D model created in 3ds max 2021.\n\nDouble Mouthpiece features:\n\nmaterials, texture.\nall objects are named and grouped\ninclude file format: max 2021, max 2018, DAE, OBJ, FBX, 3ds, ASS, DWF, DWG, ABC","imageAlt":"Double Mouthpiece 3D","url":"https://www.cgtrader.com/3d-models/sports/game/double-mouthpiece","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/rtx1fPYbNwMV81ofQy5e3tnM/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/1.jpg","gridUrl":"https://media.cgtrader.com/variants/rtx1fPYbNwMV81ofQy5e3tnM/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/1.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/sports/game/double-mouthpiece","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":false},{"id":25,"name":".dae","is_native":false},{"id":104,"name":".abc","is_native":false},{"id":4,"name":".dwg","is_native":false},{"id":2,"name":".3ds","is_native":false},{"id":7,"name":".dxf","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false}],"categorySlug":"sports","subcategorySlug":"game","categoryTitle":"Sports","subcategoryTitle":"Game","schemaImageUrl":"https://img-new.cgtrader.com/items/3749017/45695779d2/double-mouthpiece-3d-model-45695779d2.webp","saleOffDiscount":50,"eligibleForSubscription":false,"subscriptionSubscribed":true,"subscriptionPotential":false}},{"id":"5863393","type":"listingItem","attributes":{"id":5863393,"title":"Coma Wall","price":3.0,"description":"Description\nComa Wall also known CfA2 Great Wall. This Coma Wall is like a firework. The Great Wall (also called Coma Wall), sometimes specifically referred to as the CfA2 Great Wall, is an immense galaxy filament. It is one of the largest known superstructures in the observable universe.\n\nThis structure was discovered c. 1989 by a team of American astronomers led by Margaret J. Geller and John Huchra while analyzing data gathered by the second CfA Redshift Survey of the Center for Astrophysics | Harvard \u0026 Smithsonian (CfA). The term \"Great\" has been added to distinguish it as an even larger type compared to standard galaxy walls.\n\nThe CfA2 Great Wall has the maximum dimensions of either 500 million or 750 million light years depending on the figure and the reference used.[citation needed] It is 200 million light years in width and about 16 million light years in thickness. Its nearest point is about 300 million light years from Earth, while its furthest point is 550 million light years away. It consists of three massive galaxy superclusters: Hercules, Coma, and Leo.\n\nThe CfA2 Great Wall includes the Coma Filament.\n\nTexture Resolution: 1150 x 1132","imageAlt":"Coma Wall 3D model","url":"https://www.cgtrader.com/3d-models/space/other/coma-wall","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/xwwqVLCsypeedkAi3wpjJMnc/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/coma%20wall.jpg","gridUrl":"https://media.cgtrader.com/variants/xwwqVLCsypeedkAi3wpjJMnc/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/coma%20wall.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/coma-wall","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":215,"name":".png","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5863393/4ca884b75b/coma-wall-3d-model-4ca884b75b.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6015323","type":"listingItem","attributes":{"id":6015323,"title":"Cosmic Walls and Clusters Collection","price":15.0,"description":"Description\nThis is a collection of 49 Cosmic Walls and Clusters Models. Each asset is a high end, photorealistic 3D model, that is created to help you add the realism to your project. Each model is suitable for any visual production - broadcast, high-res film close-ups, advertising, games, design visualization, forensic presentation, etc.\n\nEach model was originally created in 3Ds Max 2022, then fully textured and rendered using V-Ray.\n\nAll geometry and visual aspects of the model are optimized to give you highest possible quality for up to 2k renders. There is no post-production used on any of the renders you see.\n\nThis collection contains:\n\n1 El Gordo Cluster(1st) - $3 2 El Gordo Cluster(2nd)- $3 3 El Gordo Cluster(3rd) - $3 4 Pavo Indus Supercluster - $3 5 Boss Great Wall(1st) - $3 6 Boss Great Wall(2nd) - $3 7 GRB 090423(1st) - $3 8 GRB 090423(2nd) - $3 9 Cosmic Web(1st) - $3 10 Cosmic Web(2nd) - $3 11 Cosmic Web(3rd) - $3 12 Shapley Supercluster(1st) - $3 Shapley Supercluster(2nd) - $3 14 Shapley Supercluster(3rd) - $3 15 Shapley Supercluster(4th) - $3 16 Shapley Supercluster(5th) - $3 17 Bullet Cluster - $3 18 Giant Void(1st) - $3 19 Giant Void(2nd) - $3 20 Clowes Campusano LQG - $3 21 U1 11 LQG - $3 22 Saraswati Supercluster - $3 23 Bok Globules - $3 24 Bootes Void - $3 25 Horologium Supercluster(1st) - $3 26 Horologium Supercluster(2nd) - $3 27Horologium Supercluster(3rd) - $3 28 Pandoras Cluster(1st) - $3 29 Pandoras Cluster(2nd) - $3 30 Centaurus Cluster - $3 31 Finger of God Globule - $3 32 KBC Void - $3 33 Hercules Corona Borealis Great Wall(1st) - $3 34 Hercules Corona Borealis Great Wall(2nd) - $3 35 Hercules Corona Borealis Great Wall(3rd) - $3 36 ASASSN 15lh - $3 37 Cosmic Filament - $3 38 Corona Borealis(1st) - $3 39 Corona Borealis(2nd) - $3 40 Southern Local Supervoid - $3 41 Giant GRB Ring - $3 42 Virgo Cluster - $3 43 Tonantzintla 618(1st) - $3 44 Tonantzintla 618(2nd) - $3 45 Ulas J1342 - $3 46 Leo Supercluster - $3 47 Coma Wall - $3 You save - $147 Features: -Each model is accurately sized to match the real object. -Clean and optimized topology is used for maximum polygon efficiency. -Each model is fully sub-dividable to allow Turbosmooth Iterations to increase mesh smoothness if needed. -All textures and materials are tailored and applied for high quality render results. -All objects have fully unwrapped UVs. -No extra plugins are needed for this model. -Lights and cameras are included in the scenes.\n\nSpecifications:\n\n-Each model is included in 1 file format. -3ds Max V-Ray\n\n-Units in all formats: #generic -All Textures are JPG and PNG format with the following resolutions: - 1089 x 580 px, 1679 x 1679 px, 400 x 400 px, 1200 x 686 px, 1600 x 1600 px, 500 x 500 px, 1446 x 1446 px, 800 x 800 px, 1200 x 720 px, 512 x 386 px, 512 x 386 px, 1280 x 720 px, 1023 x 685 px, 1150 x 1132 px, 736 x 915 px, 1530 x 1182 px, 768 x 768 px, 512 x 414 px, 1000 x 532 px, 1354 x 768 px, 3997 x 3861 px, 1156 x 1156 px, 1526 x 1526 px\n\nAdditional Notes:\n\nThis collection was created for 1 day form our Leading 3D artists to ensure you get the best quality model and save precious production time.\n\nIf you have any questions, you can contact us trough support. Just send a support ticket!","imageAlt":"3D Cosmic Walls and Clusters Collection","url":"https://www.cgtrader.com/3d-models/space/other/cosmic-walls-and-clusters-collection","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/2t4vsi6id4ebe3uq6ordm1ryf5d4/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/cosmic%20walls%20and%20clusters%20collection%20thumbnail.jpg","gridUrl":"https://media.cgtrader.com/variants/2t4vsi6id4ebe3uq6ordm1ryf5d4/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/cosmic%20walls%20and%20clusters%20collection%20thumbnail.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/cosmic-walls-and-clusters-collection","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":215,"name":".png","is_native":false},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/6015323/ac4ad33ccf/cosmic-walls-and-clusters-collection-3d-model-ac4ad33ccf.webp","saleOffDiscount":0,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5861132","type":"listingItem","attributes":{"id":5861132,"title":"Shapley Supercluster","price":3.0,"description":"Description\nDescriptionShapley Supercluster. This Shapley Supercluster is like a gas cloud or nebula. The Shapley Supercluster or Shapley Concentration (SCl 124) is the largest concentration of galaxies in our nearby universe that forms a gravitationally interacting unit, thereby pulling itself together instead of expanding with the universe. It appears as a striking overdensity in the distribution of galaxies in the constellation of Centaurus. It is 650 million light-years away (z=0.046). In 1930, Harlow Shapley and his colleagues at the Harvard College Observatory started a survey of galaxies in the southern sky, using photographic plates obtained at the 24-inch Bruce telescope at Bloemfontein, South Africa. By 1932, Shapley reported the discovery of 76,000 galaxies brighter than 18th apparent magnitude in a third of the southern sky, based on galaxy counts from his plates. Some of this data was later published as part of the Harvard galaxy counts, intended to map galactic obscuration and to find the space density of galaxies. In this catalog, Shapley could see most of the 'Coma-Virgo cloud' (now known to be a superposition of the Coma Supercluster and the Virgo Supercluster), but found a 'cloud' in the constellation of Centaurus to be the most striking concentration of galaxies. He found it particularly interesting because of its great linear dimension, the numerous population and distinctly elongated form. This can be identified with what we now know as the core of the Shapley Supercluster. Shapley estimated the distance to this cloud to be 14 times that to the Virgo Cluster, from the average diameters of the galaxies. This would place the Shapley Supercluster at a distance of 231 Mpc, based on the current estimate of the distance to Virgo. In recent times, the Shapley Supercluster was named by Somak Raychaudhury, from a survey of galaxies from UK Schmidt Telescope Sky survey plates, using the Automated Plate Measuring Facility (APM) at the University of Cambridge in England. In this paper, the supercluster was named after Harlow Shapley, in recognition of his pioneering survey of galaxies in which this concentration of galaxies was first seen. 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For the psychologist, see Star Vega (psychologist). For other uses, see Vega (disambiguation). Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years (7.7 parsecs) from the Sun, and one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed arguably the next most important star in the sky after the Sun. Vega was the northern pole star around 12,000 BCE and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to have its image and spectrum photographed. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system. Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their main sequence lifetimes. Compared with the Sun, Vega has a lower abundance of elements heavier than helium. Vega is also a variable star—that is, a star whose brightness fluctuates. It is rotating rapidly with a speed of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles. Based on observations of more infrared radiation than expected, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars. Observations by the James Webb Space Telescope show that the disk is exceptionally smooth, with no evidence of shaping by massive planets, though there is some evidence that there may be one or more Neptune-mass planets closer to the star.\n\nTexture Resolution: 750 x 420","imageAlt":"Vega Cluster 3D","url":"https://www.cgtrader.com/3d-models/space/other/vega-cluster-d94c9331-0dc5-4231-bb71-4c6184d490a4","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/68Wh6G5M3dSQajMADMoDmtRh/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/vega%20cluster--2.jpg","gridUrl":"https://media.cgtrader.com/variants/68Wh6G5M3dSQajMADMoDmtRh/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/vega%20cluster--2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/vega-cluster-d94c9331-0dc5-4231-bb71-4c6184d490a4","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5813566/64ae914794/vega-cluster-3d-model-64ae914794.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5861088","type":"listingItem","attributes":{"id":5861088,"title":"Shapley Supercluster","price":3.0,"description":"Description\nShapley Supercluster. This Shapley Supercluster is like a bacteria. The Shapley Supercluster or Shapley Concentration (SCl 124) is the largest concentration of galaxies in our nearby universe that forms a gravitationally interacting unit, thereby pulling itself together instead of expanding with the universe. It appears as a striking overdensity in the distribution of galaxies in the constellation of Centaurus. It is 650 million light-years away (z=0.046). In 1930, Harlow Shapley and his colleagues at the Harvard College Observatory started a survey of galaxies in the southern sky, using photographic plates obtained at the 24-inch Bruce telescope at Bloemfontein, South Africa. By 1932, Shapley reported the discovery of 76,000 galaxies brighter than 18th apparent magnitude in a third of the southern sky, based on galaxy counts from his plates. Some of this data was later published as part of the Harvard galaxy counts, intended to map galactic obscuration and to find the space density of galaxies. In this catalog, Shapley could see most of the 'Coma-Virgo cloud' (now known to be a superposition of the Coma Supercluster and the Virgo Supercluster), but found a 'cloud' in the constellation of Centaurus to be the most striking concentration of galaxies. He found it particularly interesting because of its great linear dimension, the numerous population and distinctly elongated form. This can be identified with what we now know as the core of the Shapley Supercluster. Shapley estimated the distance to this cloud to be 14 times that to the Virgo Cluster, from the average diameters of the galaxies. This would place the Shapley Supercluster at a distance of 231 Mpc, based on the current estimate of the distance to Virgo. In recent times, the Shapley Supercluster was named by Somak Raychaudhury, from a survey of galaxies from UK Schmidt Telescope Sky survey plates, using the Automated Plate Measuring Facility (APM) at the University of Cambridge in England. In this paper, the supercluster was named after Harlow Shapley, in recognition of his pioneering survey of galaxies in which this concentration of galaxies was first seen. 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Sirius is the brightest star in the night sky. Its name is derived from the Greek word Σείριος (Latin script: Seirios), meaning lit. 'glowing' or 'scorching'. The star is designated α Canis Majoris, Latinized to Alpha Canis Majoris, and abbreviated α CMa or Alpha CMa. With a visual apparent magnitude of −1.46, Sirius is almost twice as bright as Canopus, the next brightest star. Sirius is a binary star consisting of a main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, termed Sirius B. The distance between the two varies between 8.2 and 31.5 astronomical units as they orbit every 50 years. Sirius appears bright because of its intrinsic luminosity and its proximity to the Solar System. At a distance of 2.64 parsecs (8.6 ly), the Sirius system is one of Earth's nearest neighbours. Sirius is gradually moving closer to the Solar System and it is expected to increase in brightness slightly over the next 60,000 years to reach a peak magnitude of −1.68. Coincidentally, at about the same time, Sirius will take its turn as the southern Pole Star, around the year 66,270 AD. In that year, Sirius will come to within 1.6 degrees of the south celestial pole. This is due to axial precession and proper motion of Sirius itself which moves slowly in the SSW direction, so it will be visible from the southern hemisphere only. After that time, its distance will begin to increase, and it will become fainter, but it will continue to be the brightest star in the Earth's night sky for approximately the next 210,000 years, at which point Vega, another A-type star that is intrinsically more luminous than Sirius, becomes the brightest star. Sirius A is about twice as massive as the Sun (MO) and has an absolute visual magnitude of +1.43. It is 25 times as luminous as the Sun, but has a significantly lower luminosity than other bright stars such as Canopus, Betelgeuse, or Rigel. The system is between 200 and 300 million years old. It was originally composed of two bright bluish stars. The initially more massive of these, Sirius B, consumed its hydrogen fuel and became a red giant before shedding its outer layers and collapsing into its current state as a white dwarf around 120 million years ago. Sirius is colloquially known as the \"Dog Star\", reflecting its prominence in its constellation, Canis Major (the Greater Dog). The heliacal rising of Sirius marked the flooding of the Nile in Ancient Egypt and the \"dog days\" of summer for the ancient Greeks, while to the Polynesians, mostly in the Southern Hemisphere, the star marked winter and was an important reference for their navigation around the Pacific Ocean.\n\nTexture Resolution: 1010 x 1112","imageAlt":"Sirius Star 3D model","url":"https://www.cgtrader.com/3d-models/space/other/sirius-star-70a04588-38a7-4a6e-94f9-a33febaaa443","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/ypvpcmjuoqfkj7dkq37c7yduu4ia/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/sirius%20star.jpg","gridUrl":"https://media.cgtrader.com/variants/ypvpcmjuoqfkj7dkq37c7yduu4ia/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/sirius%20star.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/sirius-star-70a04588-38a7-4a6e-94f9-a33febaaa443","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/6016850/dd9ce08af4/sirius-star-3d-model-dd9ce08af4.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5806991","type":"listingItem","attributes":{"id":5806991,"title":"Hercules Corona Borealis Great Wall","price":3.0,"description":"Description\nDescription\n\nHercules Corona Borealis Great Wall. The Hercules Corona Borealis Great Wall is like a dragon. The Hercules–Corona Borealis Great Wall (HCB) or simply the Great Wall is a galaxy filament that is the largest known structure in the observable universe, measuring approximately 10 billion light-years in length (the observable universe is about 93 billion light-years in diameter). This massive superstructure is a region of the sky seen in the data set mapping of gamma-ray bursts (GRBs) that has been found to have a concentration of similarly distanced GRBs that is unusually higher than the expected average distribution. It was discovered in early November 2013 by a team of American and Hungarian astronomers led by István Horváth, Jon Hakkila and Zsolt Bagoly while analyzing data from the Swift Gamma-Ray Burst Mission, together with other data from ground-based telescopes. It is the largest known formation in the universe, exceeding the size of the Huge-LQG by about a factor of two. The overdensity lies at the Second, Third and Fourth Galactic Quadrants (NGQ2, NGQ3 and NGQ4) of the sky. Thus, it lies in the Northern Hemisphere, centered on the border of the constellations Draco and Hercules. The entire clustering consists of around 19 GRBs with the redshift ranges between 1.6 and 2.1. Typically, the distribution of GRBs in the universe appears in the sets of less than the 2σ distribution, or with less than two GRBs in the average data of the point-radius system.[clarification needed] One possible explanation of this concentration is the Hercules–Corona Borealis Great Wall. The wall has a mean size in excess of 2 billion to 3 billion parsecs (6 to 10 billion light-years). Such a supercluster can explain the significant distribution of GRBs because of its tie to star formation. Doubt has been placed on the existence of the structure in other studies, positing that the structure was found through biases in certain statistical tests, without considering the full effects of extinction. A 2020 paper (by the original group of discoverers and others) says that their analysis of the most reliable current dataset supports the structure's existence, but that the THESEUS satellite will be needed to decide the question conclusively.\n\nTexture Resolution: 720 x 720","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/hercules-corona-borealis-great-wall-354543cd-6331-45bc-a6d5-fd5b2ed894fe","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/zH4f8FfXqEygaeMmduRHJ39k/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/hercules%20corona%20borealis-2.jpg","gridUrl":"https://media.cgtrader.com/variants/zH4f8FfXqEygaeMmduRHJ39k/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/hercules%20corona%20borealis-2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/hercules-corona-borealis-great-wall-354543cd-6331-45bc-a6d5-fd5b2ed894fe","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5806991/7c410be474/hercules-corona-borealis-great-wall-3d-model-7c410be474.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"1977306","type":"listingItem","attributes":{"id":1977306,"title":"Mitsubishi L200 Triton 2020 Double Cab","price":119.0,"description":"- detailed exterior, simple interior.\n- every object has material's name, you can easily change or apply materials\n.\n.\n.\n.max format:\nRar archive contains:\n1. 3ds max 2011 with vray materials, which you can see in preview images studio renders. Carpaint colour can be slightly different. Lighting and render setup included but render results can be different because photoshop was used to correct contrast, brightness, saturation etc.. but Photoshop CS6 macro file (.atn) for post production is also included.\n2. 3ds max 2011 with mental ray materials, which you can see in preview images on outdoor renders. Carpaint colour can be different. Enviroment not included.\n3. 3ds max 2011 with simple standard materials scanline\nJust put into your scene and render!\nIn each scene model is provided with mesh smooth modifier on stack on objects that need it. Mesh smooth is set 1 or 2 for renders. Exterior and wheels are in different layers. \n.\n.obj format:\nRar archive contains two versions of model:\n1. Exported without collapsing after mesh smooth. Low or med poly mesh which you can see in preview images, good if you need to edit model.\n2. Exported after appllying mesh smooth. Just import, apply materials and render\nSimple materials, textures may have to be added manually.\n.\n.lwo, .c4d format:\nRar archive contains model exported without collapsing after mesh smooth. Low or med poly mesh which you can see in preview images, good if you need to edit model.\nSimple materials, textures may have to be added manually. In Cinema 4D some elements may have to be optimized.\n.\n.fbx and .3ds format:\nRar archive contains model exported after appllying mesh smooth. Just import, apply materials and render.\nSimple materials, textures may have to be added manually.\n.\n.stl format:\nRar archive contains model in two resolutions. Geometry only.\n.\n.\n.\nPolycount:\nwithout meshsmooth max,obj,lwo,c4d, stl: 350 000 polygons\ncollapsed fbx,3ds,obj,stl: 3 300 000 faces/ 1 900 000 polygons","imageAlt":"3D model Mitsubishi L200 Triton 2020 Double Cab","url":"https://www.cgtrader.com/3d-models/car/suv/mitsubishi-l200-triton-2020-double-cab","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/1x9Nd1NPM4HA6JCQRheagBn9/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Mitsubishi_L200_2020_01.jpg","gridUrl":"https://media.cgtrader.com/variants/1x9Nd1NPM4HA6JCQRheagBn9/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Mitsubishi_L200_2020_01.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/car/suv/mitsubishi-l200-triton-2020-double-cab","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":2,"name":".3ds","is_native":false},{"id":6,"name":".c4d","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":8,"name":".lwo","is_native":false},{"id":17,"name":".max","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":51,"name":".stl","is_native":false},{"id":null,"name":null,"is_native":false}],"categorySlug":"car","subcategorySlug":"suv","categoryTitle":"Car","subcategoryTitle":"SUV","schemaImageUrl":"https://img-new.cgtrader.com/items/1977306/e7c9a649ae/mitsubishi-l200-triton-2020-double-cab-3d-model-e7c9a649ae.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"2995035","type":"listingItem","attributes":{"id":2995035,"title":"Birkenstock Women Arizona Suede Double Buckle Sandals","price":8.0,"description":"Model:\n\n-Birkenstock Women's Arizona Suede Double Buckle: https://www.overstock.com/Clothing-Shoes/Sandals/1948/subcat.html?featuredproduct=31693168\n\nGeometry:\n\n-Birkenstock Women's Arizona Suede Double Buckle: polys: 107,584; verts: 113,196\n\nDimensions:\n\n-Birkenstock Women's Arizona Suede Double Buckle: Lenght: 10,5cm; Width: 25cm; Height: 7,5cm \n\nMaterials:\n\n-Birkenstock Women's Arizona Suede Double Buckle: Leather, Cork\n\nThe materials are available in the Max file format with V-Ray. No plugins were used.\n\nFORMATS: -3ds max 2016, 2017 or higher *.max V-RayNext - with materials for V-ray 3.0 or higher *.obj - with mapping with materials..obj file, ready to import to any software. *.fbx - with mapping without materials- Autodesk FBX files\n\nRENDERINGS *previews rendered with V-Ray, the lighting setup is not included\n\nIf you like this product, please rate it. Thank you! 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It can be used in cinematics or can be simplified for mobile use. \n\n**Features:**\n- This model is designed for the next-gen real time engines (i.e. Unreal Engine, Unity), however it may be used with other renderers (i.e. mental ray, v-ray, Arnold, etc)\n- Default hair color is blonde, so it can be tinted to other colors or be made darker. \n- Textures are Color/Albedo, Alpha, Normal, Specular, AO. 4K resolution (4096x4096 px). \n- Hair geometry is organized in layers for easy isolations and adjustment.\n- Includes two levels of details (Lower Poly 23K tris, Higher Poly 54K tris). \n- Real world scale. Upon importing the model will appear at 180 cm or about 5 feet 11 inches.\n- Includes head placeholder (untextured).\n- All objects are named and organized.\n- Previews are rendered in Marmoset Toolbag 3.\n\n**Package includes:**\n- FBX (lower resolution @ 23K, higher resolution @ 54K), plus head placeholder.\n- OBJ (lower resolution @ 23K, higher resolution @ 54K), plus head placeholder.\n- Marmoset Toolbag 3 scene (as seen in the preview images)\n\n//Textures\n- COLOR (ALBEDO) – TGA 32bit – 4096 (Blonde, Red, Dark)\n- NORMAL – PNG - 4096\n- SPECULAR – PNG - 4096\n- AO – PNG – 4096\n- ALPHA – PNG - 4096\n\n**Triangle Count:**\n\n- 23209 tris (lower) \n- 53962 tris (higher)\n\n**Note:** _*textured face is NOT included in the package_\n\n**Recomended:**\nThis hair style is compatible with “Female Custom Basemesh.” It will fit perfectly on the head even after facial and body adjustments. \n\nhttps://www.cgtrader.com/3d-models/character/woman/female-custom-basemesh\n\n_*If you have any questions about this model, please send me a message and I will be happy to assist. \nThanks for looking!_\n\n\n","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/character/woman/hair-double-braid-gen2","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/UicSSBi7SQvCgjT28NEjQ62E/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Hair_DoubleBraid_by_AlexLashko_00_CGT.jpg","gridUrl":"https://media.cgtrader.com/variants/UicSSBi7SQvCgjT28NEjQ62E/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Hair_DoubleBraid_by_AlexLashko_00_CGT.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/character/woman/hair-double-braid-gen2","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":true}},"metaverseFormatsList":[{"id":5,"name":".fbx","is_native":false},{"id":137,"name":".tbscene","is_native":false},{"id":12,"name":".obj","is_native":false}],"categorySlug":"character","subcategorySlug":"woman","categoryTitle":"Character","subcategoryTitle":"Woman","schemaImageUrl":"https://img-new.cgtrader.com/items/4975965/dfdcce4968/hair-double-braid-gen2-3d-model-dfdcce4968.webp","saleOffDiscount":30,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5862315","type":"listingItem","attributes":{"id":5862315,"title":"El Gordo Cluster","price":3.0,"description":"Description\nEl Gordo Cluster. This El Gordo Cluster is like a starfield with comets. El Gordo (lit. The Fat One) (ACT-CL J0102-4915 or SPT-CL J0102-4915) is the largest distant galaxy cluster observed at its distance or beyond, as of 2011. As of 2014, it held the record for being the largest distant galaxy cluster to have been discovered with a mass of slightly less than three quadrillion solar masses although later its mass was reduced to about 2.1×1015 (2.1 quadrillion) solar masses with a 10% uncertainty. It was found by NASA's Chandra X-ray Observatory, the Atacama Cosmology Telescope (funded by the National Science Foundation) and the European Southern Observatory's Very Large Telescope. This galaxy cluster, officially named as, 'ACT-CL J0102-4915', has been given a 'nickname' by the researchers as 'El Gordo', which stands for the Fat One or the Big One in Spanish. It is located more than 7 billion light-years from Earth. Findings and results on 'El Gordo' were announced at the 219th meeting of American Astronomical Society in Austin, Texas.\n\nTexture Resolution: 2000 x 2000","imageAlt":"3D model ray El Gordo Cluster","url":"https://www.cgtrader.com/3d-models/space/other/el-gordo-cluster-e13f4f78-e8cf-47b4-9f2d-d392b8d1aa90","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/C2EaNpu2mpntHLpgzBTuKftZ/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/el%20gordo%20cluster-2.jpg","gridUrl":"https://media.cgtrader.com/variants/C2EaNpu2mpntHLpgzBTuKftZ/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/el%20gordo%20cluster-2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/el-gordo-cluster-e13f4f78-e8cf-47b4-9f2d-d392b8d1aa90","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":215,"name":".png","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5862315/98fa6f1bc2/el-gordo-cluster-3d-model-98fa6f1bc2.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5864705","type":"listingItem","attributes":{"id":5864705,"title":"Bullet Cluster","price":3.0,"description":"Description\nBullet Cluster. This Bullet Cluster is like a gas cloud with blue and pink colors. The Bullet Cluster (1E 0657-56) consists of two colliding clusters of galaxies. Strictly speaking, the name Bullet Cluster refers to the smaller subcluster, moving away from the larger one. It is at a comoving radial distance of 1.141 Gpc (3.72 billion light-years). The object is of a particular note for astrophysicists, because gravitational lensing studies of the Bullet Cluster are claimed to provide strong evidence for the existence of dark matter. Observations of other galaxy cluster collisions, such as MACS J0025.4-1222, similarly support the existence of dark matter. The major components of the cluster pair—stars, gas and the putative dark matter—behave differently during collision, allowing them to be studied separately. The stars of the galaxies, observable in visible light, were not greatly affected by the collision, and most passed right through, gravitationally slowed but not otherwise altered. The hot gas of the two colliding components, seen in X-rays, represents most of the baryonic, or \"ordinary\", matter in the cluster pair. The gases of the intracluster medium interact electromagnetically, causing the gases of both clusters to slow much more than the stars.\n\nThe third component, the dark matter, was detected indirectly by the gravitational lensing of background objects. In theories without dark matter, such as modified Newtonian dynamics (MOND), the lensing would be expected to follow the baryonic matter; i.e. the X-ray gas. However, the lensing is strongest in two separated regions near (possibly coincident with) the visible galaxies. This provides support for the idea that most of the gravitation in the cluster pair is in the form of two regions of dark matter, which bypassed the gas regions during the collision. This accords with predictions of dark matter as only gravitationally interacting, other than weakly interacting.\n\nTexture Resolution: 3000 x 2168","imageAlt":"Bullet Cluster 3D model","url":"https://www.cgtrader.com/3d-models/space/other/bullet-cluster","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/7VLXMgvVAF6CeUdB8GiddF2e/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/bullet%20cluster.jpg","gridUrl":"https://media.cgtrader.com/variants/7VLXMgvVAF6CeUdB8GiddF2e/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/bullet%20cluster.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/bullet-cluster","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5864705/8ad6886585/bullet-cluster-3d-model-8ad6886585.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6298024","type":"listingItem","attributes":{"id":6298024,"title":"Wool Double Breasted Coat","price":4.99,"description":"**Realistic 3D Model of Wool Double Breasted Coat Created by Paradoox Studio.**\n\nThis product is perfect for use in any project.\nThis model is excellent for photorealistic visualization, promotional shots, video production, and real-time visualizations or game engines.\nIt can be used wherever you might need it.\n\n.\n.\n.\n\n  Info about this product:\n\n- The model has a clean quad-based topology\n- All the formats you need\n- Low-Poly\n- Unwrapped\n- PBR Materials\n- 4K Texture Resolution\n- The model is built for real\n- World scale\n- Units used: cm\n- It doesn’t have a third-party renderer or plug-ins\n- It doesn’t have a missing DLL\n- It doesn’t have NGons\n- It doesn’t have Overlapping Vertices\n- It doesn’t have Overlapping Faces\n- It doesn’t have missing textures\n- It doesn’t have Poles\n- All objects, textures, and materials have their names  \n- You can also use the model directly in programs supporting the formats we provided.\n\n.\n.\n.\n\n**Join our Discord community:**\n\nhttps://discord.gg/VM5PN6euyh \n\n.\n.\n.\n\n**Please leave me a comment if you like it and rate the product.**","imageAlt":"3D asset Wool Double Breasted Coat","url":"https://www.cgtrader.com/3d-models/character/clothing/wool-double-breasted-coat","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/qztptor2lnc371puu61w6mexvsrc/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/Wool_double_breasted_coat_R_001.jpg","gridUrl":"https://media.cgtrader.com/variants/qztptor2lnc371puu61w6mexvsrc/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/Wool_double_breasted_coat_R_001.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/character/clothing/wool-double-breasted-coat","isCgtVerified":true,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":true}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":21,"name":".blend","is_native":false},{"id":null,"name":null,"is_native":false},{"id":11,"name":".ma","is_native":false},{"id":51,"name":".stl","is_native":false},{"id":25,"name":".dae","is_native":false},{"id":104,"name":".abc","is_native":false},{"id":55,"name":".ztl","is_native":false},{"id":6,"name":".c4d","is_native":false},{"id":117,"name":".gltf","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":207,"name":".usd","is_native":false},{"id":null,"name":null,"is_native":false}],"categorySlug":"character","subcategorySlug":"clothing","categoryTitle":"Character","subcategoryTitle":"Clothing","schemaImageUrl":"https://img-new.cgtrader.com/items/6298024/43e73e5d1e/wool-double-breasted-coat-3d-model-43e73e5d1e.webp","saleOffDiscount":50,"eligibleForSubscription":true,"subscriptionSubscribed":true,"subscriptionPotential":false}},{"id":"5842771","type":"listingItem","attributes":{"id":5842771,"title":"Phoenix Cluser","price":3.0,"description":"Description\nPhoenix Cluster. The Phoenix Cluster is like an ant. The Phoenix Cluster (SPT-CL J2344-4243) is a massive, Abell class type I galaxy cluster located at its namesake, southern constellation of Phoenix. It was initially detected in 2010 during a 2,500 square degree survey of the southern sky using the Sunyaev–Zeldovich effect by the South Pole Telescope collaboration. It is one of the most massive galaxy clusters known, with the mass on the order of 2×1015 MO, and is the most luminous X-ray cluster discovered, producing more X-rays than any other known massive cluster. It is located at a comoving distance of 8.61 billion light-years (2.64 gigaparsecs) from Earth. About 42 member galaxies were identified and currently listed in the SIMBAD Astronomical Database, though the real number may be as high as 1,000 galaxies. The Phoenix Cluster was first reported in a paper by R. Williamson and colleagues during a survey by the South Pole Telescope in Antarctica, being one of the 26 galaxy clusters identified by the survey. The detection has been conducted at frequencies between 95, 150, and 220 GHz, with 14 of the galaxy clusters detected have been previously identified, while 12 – including Phoenix Cluster, being new discoveries. The would-be named Phoenix Cluster (still identified by its numerical catalogue entry SPT-CL J2344–4243) has been remarked to be having the largest X-ray luminosity of any cluster described by the survey. A bright, type-2 Seyfert galaxy has also been pronounced lying 19 arcseconds from the apparent center of the cluster that has been identified as 2MASX J23444387-4243124, which would later be named Phoenix A, the cluster's central galaxy.\n\nTexture Resolution: 864 x 864","imageAlt":"Phoenix Cluser 3D","url":"https://www.cgtrader.com/3d-models/space/other/phoenix-cluser","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/Pho23N1BJVhLKw5XH9Wk6nBA/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/phoenix%20cluster--2.jpg","gridUrl":"https://media.cgtrader.com/variants/Pho23N1BJVhLKw5XH9Wk6nBA/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/phoenix%20cluster--2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/phoenix-cluser","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5842771/ca4c824ce9/phoenix-cluser-3d-model-ca4c824ce9.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6455408","type":"listingItem","attributes":{"id":6455408,"title":"Henize 2-10","price":3.0,"description":"Description\nHen 2-10, also known as He 2-10 and Henize 2-10, is a dwarf starburst galaxy located 34 million light years away in the constellation of Pyxis. The galaxy is believed to be an early stage starburst galaxy. A black hole was later discovered near the center of the dwarf galaxy, suggesting that the black holes found at the center of most large galaxies may have formed before the galaxies themselves. Recent estimates have placed the mass of this black hole around 3×106 MO, and the mass of the entire dwarf galaxy at about 1×1010 MO. Henize 2-10 draws its name from a catalog of planetary nebulae assembled by astronomer Karl Henize. Henize additionally noted that the object was identified in an unpublished paper by Rudolph Minkowski. The object was likely misidentified as a planetary nebula due to the galaxy's strong emission lines, a feature common of planetary nebulas. It was not until the 1970s when observations of Hen 2-10 indicated that the center of the object was a strong source of radio waves that it was shown that Hen 2-10 was a dwarf galaxy rather than a planetary nebula. Supporting evidence for the reclassification came in the form of excess infrared emission and a higher than usual density of neutral hydrogen. Hen 2-10 is a starburst galaxy featuring at least two star-forming regions near the center of the galaxy. These regions feature a variety of different substances, and multiple super star clusters. A study of some of these SSCs estimates their age to be between 4 and 5 megayears. The galaxy also features emission typical of that in a Wolf–Rayet star, further providing evidence for the starburst region of the galaxy. It was one of the first galaxies found to feature this emission. The strong prevalence of this emission has led to its classification as a Wolf–Rayet galaxy, a special subclass of starburst galaxy that features a higher than normal number of Wolf–Rayet stars. Furthermore, observations have shown irregularities in the southeast portion of the galaxy which could be interpreted as a tidal tail. This tidal tail suggests that Hen 2-10 may have had past interactions with other galaxies, possibly even a merger event. In 2011, a team of researchers studied the non-thermal emission of the galaxy center and indicated that the source strengths of radio waves are too strong to come from x-ray binaries while the source strengths of x-rays are too strong to be supernova remnants. However, these sources do align with known data for black holes. This original paper postulated the mass of the black hole to be ~1×106 MO, but a newer study has refined the estimate to 3×106 MO. The presence of SSCs near the center of the galaxy, and not a singular nuclear star cluster (NSC) has led some to believe that Hen 2-10 is a galaxy in its early years. The presence of the black hole is seen to be evidence of the dissipationless model of NSC formation. In this model, the SSCs will move to the center and form a singular NSC. Due to the black hole's relatively small mass, it is not believed to have a major effect on the timescale of this motion, although it is not yet understood how the black hole will affect the NSC formation. 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In cosmology, galaxy filaments are the largest known structures in the universe, consisting of walls of galactic superclusters. These massive, thread-like formations can commonly reach 50 to 80 megaparsecs (160 to 260 megalight-years)—with the largest found to date being the Hercules-Corona Borealis Great Wall at around 3 gigaparsecs (9.8 Gly) in length—and form the boundaries between voids. Due to the accelerating expansion of the universe, the individual clusters of gravitationally bound galaxies that make up galaxy filaments are moving away from each other at an accelerated rate; in the far future they will dissolve. 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This Shapley Supercluster is like a steam logo. The Shapley Supercluster or Shapley Concentration (SCl 124) is the largest concentration of galaxies in our nearby universe that forms a gravitationally interacting unit, thereby pulling itself together instead of expanding with the universe. It appears as a striking overdensity in the distribution of galaxies in the constellation of Centaurus. It is 650 million light-years away (z=0.046). In 1930, Harlow Shapley and his colleagues at the Harvard College Observatory started a survey of galaxies in the southern sky, using photographic plates obtained at the 24-inch Bruce telescope at Bloemfontein, South Africa. By 1932, Shapley reported the discovery of 76,000 galaxies brighter than 18th apparent magnitude in a third of the southern sky, based on galaxy counts from his plates. Some of this data was later published as part of the Harvard galaxy counts, intended to map galactic obscuration and to find the space density of galaxies. In this catalog, Shapley could see most of the 'Coma-Virgo cloud' (now known to be a superposition of the Coma Supercluster and the Virgo Supercluster), but found a 'cloud' in the constellation of Centaurus to be the most striking concentration of galaxies. He found it particularly interesting because of its great linear dimension, the numerous population and distinctly elongated form. This can be identified with what we now know as the core of the Shapley Supercluster. Shapley estimated the distance to this cloud to be 14 times that to the Virgo Cluster, from the average diameters of the galaxies. This would place the Shapley Supercluster at a distance of 231 Mpc, based on the current estimate of the distance to Virgo. In recent times, the Shapley Supercluster was named by Somak Raychaudhury, from a survey of galaxies from UK Schmidt Telescope Sky survey plates, using the Automated Plate Measuring Facility (APM) at the University of Cambridge in England. In this paper, the supercluster was named after Harlow Shapley, in recognition of his pioneering survey of galaxies in which this concentration of galaxies was first seen. 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Williamson and colleagues during a survey by the South Pole Telescope in Antarctica, being one of the 26 galaxy clusters identified by the survey. The detection has been conducted at frequencies between 95, 150, and 220 GHz, with 14 of the galaxy clusters detected have been previously identified, while 12 – including Phoenix Cluster, being new discoveries. The would-be named Phoenix Cluster (still identified by its numerical catalogue entry SPT-CL J2344–4243) has been remarked to be having the largest X-ray luminosity of any cluster described by the survey. 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This Virgo Cluster is like a stars in space. The Virgo Cluster is a cluster of galaxies whose center is 53.8 ± 0.3 Mly (16.5 ± 0.1 Mpc) away in the constellation Virgo. Comprising approximately 1,300 (and possibly up to 2,000) member galaxies, the cluster forms the heart of the larger Virgo Supercluster, of which the Local Group (containing the Milky Way galaxy) is a member. The Local Group actually experiences the mass of the Virgo Supercluster as the Virgocentric flow. It is estimated that the Virgo Cluster's mass is 1.2×1015 MO out to 8 degrees of the cluster's center or a radius of about 2.2 Mpc.\n\nMany of the brighter galaxies in this cluster, including the giant elliptical galaxy Messier 87, were discovered in the late 1770s and early 1780s and subsequently included in Charles Messier's catalogue of non-cometary fuzzy objects. Described by Messier as nebulae without stars, their true nature was not recognized until the 1920s.\n\nThe cluster extends across approximately 8 degrees centered in the constellation Virgo. Some of its most prominent members can be seen with binoculars and small telescopes, while a 6-inch telescope will reveal about 160 of the cluster's galaxies on a clear night. 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LL Pegasi (AFGL 3068) is a Mira variable star surrounded by a pinwheel-shaped nebula, IRAS 23166+1655, thought to be a preplanetary nebula. It is a binary system that includes an extreme carbon star. 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The Fornax Cluster is a cluster of galaxies lying at a distance of 19 megaparsecs (62 million light-years). It has an estimated mass of (7±2)×1013 solar masses, making it the second richest galaxy cluster within 100 million light-years, after the considerably larger Virgo Cluster. It may be associated with the nearby Eridanus Group. It lies primarily in the constellation Fornax, with its southern boundaries partially crossing into the constellation of Eridanus, and covers an area of sky about 6° across or about 28 sq degrees. The Fornax Cluster is a particularly valuable source of information about the evolution of such clusters due to its relatively close proximity to the Sun. It also shows the gravitational effects of a merger of a galaxy subgroup with the main galaxy group, which in turn lends clues about the associated galactic superstructure. At the centre of the cluster lies NGC 1399. Other cluster members include NGC 1316 (the group's brightest galaxy), NGC 1365, NGC 1427A, NGC 1427 and NGC 1404. 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This El Gordo Cluster is like a latin N letter. El Gordo (lit. The Fat One) (ACT-CL J0102-4915 or SPT-CL J0102-4915) is the largest distant galaxy cluster observed at its distance or beyond, as of 2011. As of 2014, it held the record for being the largest distant galaxy cluster to have been discovered with a mass of slightly less than three quadrillion solar masses although later its mass was reduced to about 2.1×1015 (2.1 quadrillion) solar masses with a 10% uncertainty. It was found by NASA's Chandra X-ray Observatory, the Atacama Cosmology Telescope (funded by the National Science Foundation) and the European Southern Observatory's Very Large Telescope. This galaxy cluster, officially named as, 'ACT-CL J0102-4915', has been given a 'nickname' by the researchers as 'El Gordo', which stands for the Fat One or the Big One in Spanish. It is located more than 7 billion light-years from Earth. 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This GRB 090423 is like a comet that's passing through the supernova explosion. GRB 090423 was a gamma-ray burst (GRB) detected by the Swift Gamma-Ray Burst Mission on April 23, 2009, at 07:55:19 UTC whose afterglow was detected in the infrared and enabled astronomers to determine that its redshift is z = 8.2, making it one of the most distant objects detected at that time with a spectroscopic redshift (GN-z11, discovered in 2016, has a redshift of 11). A gamma-ray burst is an extremely luminous event flash of gamma rays that occurs as the result of an explosion, and is thought to be associated with the formation of a black hole. The burst itself typically only lasts for a few seconds, but gamma-ray bursts frequently produce an afterglow at longer wavelengths that can be observed for many hours or even days after the burst. Measurements at these wavelengths, which include X-ray, ultraviolet, optical, infrared, and radio, enable follow-up study of the event. The finite speed of light means that GRB 090423 is also one of the earliest objects ever detected for which a spectroscopic redshift has been measured. The universe was only 630 million years old when the GRB occurred, and its detection confirms that massive stars were born and dying even very early on in the life of the universe. GRB 090423 and similar events provide a unique means of studying the early universe, as few other objects of that era are bright enough to be seen with today's telescopes. On April 23, 2009, at 07:55:19 UTC the Swift satellite detected a burst that lasted about 10 seconds and was located in the direction of the constellation Leo. Swift localized the field in which GRB 090423 occurred, and 77 seconds after the burst, the Swift UVOT Photometric System took a 150-second exposure of the field, but was unable to detect an optical or ultraviolet afterglow. A few minutes after its discovery, ground-based telescopes began observing the field. Within 20 minutes of the burst, Nial Tanvir and his team found an infrared source at the Swift position using the United Kingdom Infrared Telescope (UKIRT) on Mauna Kea, Hawaii. The initial observations taken by UKIRT were triggered autonomously via the eSTAR Project. They observed a drop off in flux beyond 1.13 micrometres with the VLT. Attributing this drop off to Lyman alpha absorption by neutral hydrogen in the intergalactic medium, they calculated a redshift of 8.2 for GRB 090423. The team of C.C. Thöne and Paolo D'Avanzo observed the afterglow of GRB 090423 using the Italian TNG 3.6m telescope located in the Canary Islands, Spain. They obtained two hours of spectra, which when combined, suggested a very weak signal at the position of the afterglow. They too saw a drop off in flux near 1.1 micrometres, and reported a redshift of 8.1 for GRB 090423, which is consistent, within error, of the redshift reported by Tanvir et al. The redshift of 8.1 suggest the burst may have lasted approximately 1.2 seconds in the local frame of the emitter, its duration being redshifted accordingly to the observed 10 seconds. The intergovernmental astronomy organisation, European Southern Observatory (ESO) operates the Very Large Telescope that obtained the spectrum reported by Tanvir et al. The GRB was not visible in Chile when Swift first detected the burst at 07:55 UTC, but was the following day at 03:00 UTC, which enabled the Gamma-Ray Burst Optical/Near-Infrared Detector (GROND) at La Silla Observatory to make observations of the burst, and find a photometric redshift consistent with the value reported elsewhere. The last observers to gather data during the event was the Combined Array for Research in Millimeter-wave Astronomy (CARMA) observatory. The observation of GRB 090423 by CARMA was taken at a frequency of 92.5 GHz. 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The Fornax Cluster is a cluster of galaxies lying at a distance of 19 megaparsecs (62 million light-years). It has an estimated mass of (7±2)×1013 solar masses, making it the second richest galaxy cluster within 100 million light-years, after the considerably larger Virgo Cluster. It may be associated with the nearby Eridanus Group. It lies primarily in the constellation Fornax, with its southern boundaries partially crossing into the constellation of Eridanus, and covers an area of sky about 6° across or about 28 sq degrees. The Fornax Cluster is a particularly valuable source of information about the evolution of such clusters due to its relatively close proximity to the Sun. It also shows the gravitational effects of a merger of a galaxy subgroup with the main galaxy group, which in turn lends clues about the associated galactic superstructure. At the centre of the cluster lies NGC 1399. Other cluster members include NGC 1316 (the group's brightest galaxy), NGC 1365, NGC 1427A, NGC 1427 and NGC 1404. Fornax can be divided into two subclusters: the main cluster, centered on NGC 1399, and a subgroup 3 degrees to the southwest centered on the lenticular galaxy NGC 1316 that is currently in the process of infalling with the largest subcluster to merge with it, and whose galaxies are experiencing relatively strong star formation activity.\n\nTexture Resolution: 1280 x 640","imageAlt":null,"url":"https://www.cgtrader.com/3d-models/space/other/fornax-cluster-a19b2b76-6055-4d17-ac35-975c66b3cd26","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/B2RZdnBnFRfhCDK61P2DZQWw/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/fornax%20cluster-2.jpg","gridUrl":"https://media.cgtrader.com/variants/B2RZdnBnFRfhCDK61P2DZQWw/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/fornax%20cluster-2.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/fornax-cluster-a19b2b76-6055-4d17-ac35-975c66b3cd26","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5862880/65bb7919f4/fornax-cluster-3d-model-65bb7919f4.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"6953184","type":"listingItem","attributes":{"id":6953184,"title":"Rail Double M02","price":18.89,"description":"**Rail Double M02**\n.\n\n- For **Embed Fbx file** please contact us after purchasing.\n\n- Low-Poly version Total  Polys:1107 Tris:1898 Edges: 2056 Verts: 951\n\n\n.\n\n**Dimensions - cm**\n- **Pivot Point is centered the object and setted at 0.0.0. **\n- Units centimeters,real-world scale.\n- no hidden polygons, non-overlapping uv maps \u0026 no-ngons.\n\n.\n\n- *.max (3ds Max 2021)\n- *.fbx (Multi Format)\n- *.obj (Multi Format)\n- *.3ds (Multi Format)\n- *.dwg (Multi Format)\n\n- rendered in substance painter. (substance file is not included.)\n- 3ds, fbx, dwg, dae and dwg exported files from max 2021 with pbr textures.\n\n.\n\n**4K pbr textures** \n- pbr metallic roughness texture set; 4K BaseColor, Height, Metallic, Normal, Roughness.\n\n\n\nThanks. \n","imageAlt":"Rail Double M02 3D asset","url":"https://www.cgtrader.com/3d-models/military/gun/rail-double-m02","isCLDApplicable":false,"isSaleOffApplicable":true,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/rae3yehxes7c8nsajjdwawgyxhoa/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/01.jpg","gridUrl":"https://media.cgtrader.com/variants/rae3yehxes7c8nsajjdwawgyxhoa/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/01.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/military/gun/rail-double-m02","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":true,"rigged":false,"lowPoly":true}},"metaverseFormatsList":[{"id":2,"name":".3ds","is_native":false},{"id":25,"name":".dae","is_native":false},{"id":4,"name":".dwg","is_native":false},{"id":5,"name":".fbx","is_native":false},{"id":17,"name":".max","is_native":false},{"id":12,"name":".obj","is_native":false},{"id":215,"name":".png","is_native":false},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"military","subcategorySlug":"gun","categoryTitle":"Military","subcategoryTitle":"Gun","schemaImageUrl":"https://img-new.cgtrader.com/items/6953184/52ff629e4f/rail-double-m02-3d-model-52ff629e4f.webp","saleOffDiscount":50,"eligibleForSubscription":false,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5862136","type":"listingItem","attributes":{"id":5862136,"title":"El Gordo Cluster","price":3.0,"description":"Description\nEl Gordo Cluster. This El Gordo Cluster is like a comet. El Gordo (lit. The Fat One) (ACT-CL J0102-4915 or SPT-CL J0102-4915) is the largest distant galaxy cluster observed at its distance or beyond, as of 2011. As of 2014, it held the record for being the largest distant galaxy cluster to have been discovered with a mass of slightly less than three quadrillion solar masses although later its mass was reduced to about 2.1×1015 (2.1 quadrillion) solar masses with a 10% uncertainty. It was found by NASA's Chandra X-ray Observatory, the Atacama Cosmology Telescope (funded by the National Science Foundation) and the European Southern Observatory's Very Large Telescope. This galaxy cluster, officially named as, 'ACT-CL J0102-4915', has been given a 'nickname' by the researchers as 'El Gordo', which stands for \"the Fat One\" or \"the Big One\" in Spanish. It is located more than 7 billion light-years from Earth. Findings and results on 'El Gordo' were announced at the 219th meeting of American Astronomical Society in Austin, Texas.\n\nTexture Resolution: 1530 x 1182","imageAlt":"3D El Gordo Cluster","url":"https://www.cgtrader.com/3d-models/space/other/el-gordo-cluster","isCLDApplicable":false,"isSaleOffApplicable":false,"gaAttributes":{},"primaryImage":{"gridFallbackUrl":"https://media.cgtrader.com/variants/VPoWQapD2Khrna8yo6jLj7hW/a26e47dab5f2d22c43d6c5ce4b4b46ecc30c70918878397cba1a10c1e35d7bfc/el%20gordo%20cluster.jpg","gridUrl":"https://media.cgtrader.com/variants/VPoWQapD2Khrna8yo6jLj7hW/78add9c2f02fbd73a43ffb3970be38683c5f15eff6ca849dc78c644f4ff9ce1b/el%20gordo%20cluster.webp","isAdultContent":false},"modelInfo":{"modelUrl":"https://www.cgtrader.com/3d-models/space/other/el-gordo-cluster","isCgtVerified":false,"types":{"printReady":false,"animated":false,"pbr":false,"rigged":false,"lowPoly":false}},"metaverseFormatsList":[{"id":17,"name":".max","is_native":true},{"id":216,"name":".jpg","is_native":false}],"categorySlug":"space","subcategorySlug":"other","categoryTitle":"Space","subcategoryTitle":"Other","schemaImageUrl":"https://img-new.cgtrader.com/items/5862136/b16122d3db/el-gordo-cluster-3d-model-b16122d3db.webp","saleOffDiscount":0,"eligibleForSubscription":true,"subscriptionSubscribed":false,"subscriptionPotential":false}},{"id":"5861027","type":"listingItem","attributes":{"id":5861027,"title":"Shapley Supercluster","price":3.0,"description":"Description\nShapley Supercluster. This Shapley Supercluster is like a space with stars in black and white background. The Shapley Supercluster or Shapley Concentration (SCl 124) is the largest concentration of galaxies in our nearby universe that forms a gravitationally interacting unit, thereby pulling itself together instead of expanding with the universe. It appears as a striking overdensity in the distribution of galaxies in the constellation of Centaurus. It is 650 million light-years away (z=0.046). In 1930, Harlow Shapley and his colleagues at the Harvard College Observatory started a survey of galaxies in the southern sky, using photographic plates obtained at the 24-inch Bruce telescope at Bloemfontein, South Africa. By 1932, Shapley reported the discovery of 76,000 galaxies brighter than 18th apparent magnitude in a third of the southern sky, based on galaxy counts from his plates. Some of this data was later published as part of the Harvard galaxy counts, intended to map galactic obscuration and to find the space density of galaxies. In this catalog, Shapley could see most of the 'Coma-Virgo cloud' (now known to be a superposition of the Coma Supercluster and the Virgo Supercluster), but found a 'cloud' in the constellation of Centaurus to be the most striking concentration of galaxies. He found it particularly interesting because of its \"great linear dimension, the numerous population and distinctly elongated form\". This can be identified with what we now know as the core of the Shapley Supercluster. Shapley estimated the distance to this cloud to be 14 times that to the Virgo Cluster, from the average diameters of the galaxies. This would place the Shapley Supercluster at a distance of 231 Mpc, based on the current estimate of the distance to Virgo. In recent times, the Shapley Supercluster was named by Somak Raychaudhury, from a survey of galaxies from UK Schmidt Telescope Sky survey plates, using the Automated Plate Measuring Facility (APM) at the University of Cambridge in England. In this paper, the supercluster was named after Harlow Shapley, in recognition of his pioneering survey of galaxies in which this concentration of galaxies was first seen. 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The galaxies in the cluster make up less than five percent of its mass. The gas (around 20 percent) is so hot that it shines only in X-rays. Dark matter makes up around 75 percent of the cluster's mass. This cluster also shows a radio halo along with several other Abell clusters. It has a strong central halo, along with an extended tail, which could either be relic radiation, or an extension of the central halo. Renato Dupke, a member of the team that discovered the Cluster, explained the origin of the name in an interview: We nicknamed it ‘Pandora's Cluster’ because so many different and strange phenomena were unleashed by the collision. In February 2023, NASA's James Webb Space Telescope captured unprecedented details of Abell 2744, revealing previously unseen galaxies and offering insights into the early universe. 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The Fornax Cluster is a cluster of galaxies lying at a distance of 19 megaparsecs (62 million light-years). It has an estimated mass of (7±2)×1013 solar masses, making it the second richest galaxy cluster within 100 million light-years, after the considerably larger Virgo Cluster. It may be associated with the nearby Eridanus Group. It lies primarily in the constellation Fornax, with its southern boundaries partially crossing into the constellation of Eridanus, and covers an area of sky about 6° across or about 28 sq degrees. The Fornax Cluster is a particularly valuable source of information about the evolution of such clusters due to its relatively close proximity to the Sun. It also shows the gravitational effects of a merger of a galaxy subgroup with the main galaxy group, which in turn lends clues about the associated galactic superstructure. At the centre of the cluster lies NGC 1399. Other cluster members include NGC 1316 (the group's brightest galaxy), NGC 1365, NGC 1427A, NGC 1427 and NGC 1404. 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This Shapley Supercluster is like a space with stars. The Shapley Supercluster or Shapley Concentration (SCl 124) is the largest concentration of galaxies in our nearby universe that forms a gravitationally interacting unit, thereby pulling itself together instead of expanding with the universe. It appears as a striking overdensity in the distribution of galaxies in the constellation of Centaurus. It is 650 million light-years away (z=0.046). In 1930, Harlow Shapley and his colleagues at the Harvard College Observatory started a survey of galaxies in the southern sky, using photographic plates obtained at the 24-inch Bruce telescope at Bloemfontein, South Africa. By 1932, Shapley reported the discovery of 76,000 galaxies brighter than 18th apparent magnitude in a third of the southern sky, based on galaxy counts from his plates. Some of this data was later published as part of the Harvard galaxy counts, intended to map galactic obscuration and to find the space density of galaxies. In this catalog, Shapley could see most of the 'Coma-Virgo cloud' (now known to be a superposition of the Coma Supercluster and the Virgo Supercluster), but found a 'cloud' in the constellation of Centaurus to be the most striking concentration of galaxies. He found it particularly interesting because of its great linear dimension, the numerous population and distinctly elongated form. This can be identified with what we now know as the core of the Shapley Supercluster. Shapley estimated the distance to this cloud to be 14 times that to the Virgo Cluster, from the average diameters of the galaxies. This would place the Shapley Supercluster at a distance of 231 Mpc, based on the current estimate of the distance to Virgo. In recent times, the Shapley Supercluster was named by Somak Raychaudhury, from a survey of galaxies from UK Schmidt Telescope Sky survey plates, using the Automated Plate Measuring Facility (APM) at the University of Cambridge in England. In this paper, the supercluster was named after Harlow Shapley, in recognition of his pioneering survey of galaxies in which this concentration of galaxies was first seen. 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The Boss Great Wall is like a bird. The BOSS Great Wall is a supercluster complex that was identified, using the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey (SDSS), in early 2016. It was discovered by a research team from several institutions, consisting of: Heidi Lietzen, Elmo Tempel, Lauri Juhan Liivamägi, Antonio Montero-Dorta, Maret Einasto, Alina Streblyanska, Claudia Maraston, Jose Alberto Rubiño-Martín and Enn Saar. The BOSS Great Wall is one of the largest superstructures in the observable universe, though there are even larger structures known. The large complex has a mean redshift of z ~ 0.47 (z times Hubble length ≈ 6.8 billion light years). It consists of two elongated superclusters, two large superclusters, and several smaller superclusters as well. The elongated superclusters form galaxy walls, with the larger of the two having a diameter of 186/h Mpc (supercluster A in the figure); the second wall's being 173/h Mpc (supercluster B). The other two main superclusters are moderately large, having diameters of 91/h Mpc and 64/h Mpc (superclusters D and C, respectively). The superstructure is roughly 1 billion light years in diameter, and has a total mass approximately 10,000 times the Milky Way galaxy. It contains at least 830 visible galaxies (represented in the figure within their respective superclusters), as well as many others that are not visible (dark galaxies). The researchers used Minkowski functionals to verify the structure's overall shape and size; the first three quantifying the thickness, width, and length followed by the fourth determining the structure's overall curvature. The research team compared the luminosities and stellar masses within the superstructure to known high stellar mass galaxies within the SDSS's 7th data release, DR7. This allowed the team to scale the data using known values, from local superclusters, to determine the overall morphology of the BOSS Great Wall. It is currently debated amongst astronomers if the BOSS Great Wall may be considered a structure, due to the intricacies of its shape and overall size. The question of whether the supercluster complex is moving together or being slowly separated by the expanding universe is a key factor to this discussion. Nevertheless, when compared to several other chain structures, such as the Sloan Great Wall, the BOSS Great Wall's superclusters are far richer, containing more dense, high stellar mass galaxies. 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The perforated surface allows the candlelight to softly diffuse, producing a cozy and calming glow ideal for home décor. Designed specifically for 3D printing, the model prints as a single solid piece and works perfectly with LED or standard tealights. 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This model contains the Curved Double Cleaver itself \n \nAll modeled in Maya, textured with Substance Painter.\n\nThe model was built to scale and is UV unwrapped properly. Contains one 4K texture set\n\n\n \n⦁    36592 tris. \n\n⦁    Contains: .FBX .OBJ and .DAE\n\n⦁    Model has clean topology. No Ngons.\n\n⦁    Built to scale\n\n⦁    Unwrapped UV Map\n\n⦁    4K Texture set\n\n⦁    High quality details\n\n⦁    Based on real life references\n\n⦁    Renders done in Marmoset Toolbag\n\n\n\nPolycount: \n\nVerts 18604\n\nEdges 37118\n\nFaces 18564\n\nTris 36592\n\n\nNOTE: These 3D items are licensed for use in personal and commercial projects. 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For this just send a message to me.\n- If you need other preview pictures from different places can contact me and ask for more preview pictures;\n- If the price is not suitable for you can contact me and discuss the price.\n- Contact me if you have any question about the products that are displayed on my profile and am ready to provide full answer and support.\n- When you purchase this product or other product you enjoy full and continuous support.\n- Want to order a model? 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