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Diagrams of three possible geometries of the universe: closed, open and flat from top to bottom, corresponding to a density parameter which is greater than, less than or equal to 1. The closed universe is of finite size and, due to its curvature, traveling far enough in one direction will lead back to one's starting point. The open and flat universes are infinite and traveling in a constant direction will never lead to the same point.
La bildo estas kopiita de wikipedia:en. La originala priskribo estas: == Summary == Permission of NASA Official: Gary Hinshaw == Licensing == {{PD-USGov}} {| border="1" ! date/time || username || edit summary |---- | 04:52, 6 January 2006 || [[:en:User:
Bu faylda fotoaparat və ya skanerlə əlavə olunmuş məlumatlar var. Əgər fayl sonradan redaktə olunubsa, bəzi parametrlər bu şəkildə göstərilənlərdən fərqli ola bilər.
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Aprel 04, 2023
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Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarDaha yuksek versiyasi yoxdur End of universe jpg 8206 557 501 piksel fayl hecmi 52 KB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get This image was uploaded in the JPEG format even though it consists of non photographic data This information could be stored more efficiently or accurately in the PNG or SVG format If possible please upload a PNG or SVG version of this image without compression artifacts derived from a non JPEG source or with existing artifacts removed After doing so please tag the JPEG version with Superseded NewImage ext and remove this tag This tag should not be applied to photographs or scans For more information see BadJPEG This file was copied from the English Language Wikipedia The original description was Xulase Diagrams of three possible geometries of the universe closed open and flat from top to bottom corresponding to a density parameter W 0 displaystyle Omega 0 which is greater than less than or equal to 1 The closed universe is of finite size and due to its curvature traveling far enough in one direction will lead back to one s starting point The open and flat universes are infinite and traveling in a constant direction will never lead to the same point Source https wmap gsfc nasa gov universe uni shape html Author NASA WMAP Science Team Lisenziya Public domain Public domain false false This file is in the public domain in the United States because it was solely created by NASA NASA copyright policy states that NASA material is not protected by copyright unless noted See Template PD USGov NASA copyright policy page or JPL Image Use Policy Warnings Use of NASA logos insignia and emblems is restricted per U S law 14 CFR 1221 The NASA website hosts a large number of images from the Soviet Russian space agency and other non American space agencies These are not necessarily in the public domain Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI 1 See also PD Hubble and Cc Hubble The SOHO ESA amp NASA joint project implies that all materials created by its probe are copyrighted and require permission for commercial non educational use 2 Images featured on the Astronomy Picture of the Day APOD web site may be copyrighted 3 The National Space Science Data Center NSSDC site has been known to host copyrighted content Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain Unless otherwise noted date time username edit summary 04 52 6 January 2006 en User Voyajer Permission of NASA Official Gary Hinshaw Orijinal yukleme gundeliyi Legend cur this is the current file del delete this old version rev revert to this old version Click on date to download the file or see the image uploaded on that date del cur 04 52 6 January 2006 en User Voyajer Voyajer en User talk Voyajer Talk 557x501 52771 bytes Permission of NASA Official Gary Hinshaw CaptionsazerbaycancaAdd a one line explanation of what this file representsnkothe shape of Universealmandrei unterschiedliche Moglichkeiten der Krummung des Raums und damit der Beschaffenheit und dem Ende des UniversumsItems portrayed in this filetesvir edirMIME type nbsp ingilisimage jpeg Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki17 21 20 mart 2006557 501 52 KB MaksimLa bildo estas kopiita de wikipedia en La originala priskribo estas Summary Permission of NASA Official Gary Hinshaw Licensing PD USGov border 1 date time username edit summary 04 52 6 January 2006 en User Fayl kecidleri Bu sekile olan kecidler Boyuk partlayis Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur ar wikipedia org layihesinde istifadesi الانفجار العظيم بوابة رياضيات صورة مختارة أرشيف بوابة رياضيات صورة مختارة 16 شكل الكون مسألة التسطيح bn wikipedia org layihesinde istifadesi মহ ব স ফ রণ তত ত ব মহ ব শ ব র আক ত ca wikipedia org layihesinde istifadesi Big Bang Forma de l Univers cs wikipedia org layihesinde istifadesi Neeukleidovska geometrie de wikipedia org layihesinde istifadesi Dichteparameter Benutzer Schneffe himself Liste ungeloster Probleme der Physik Flachheitsproblem el wikipedia org layihesinde istifadesi Sympan en wikipedia org layihesinde istifadesi Big Bang Universe Geodesic Shape of the universe Flatness problem Portal Mathematics Featured picture archive Hadamard space User SteveChervitzTrutane Inhomogeneous cosmology Portal Mathematics Featured picture 2007 09 CAT k space Wikipedia Recent additions 2008 September User WritingMan Timescape cosmology es wikipedia org layihesinde istifadesi Destino final del universo Forma del universo Problema de planitud et wikipedia org layihesinde istifadesi Suur Pauk eu wikipedia org layihesinde istifadesi Big Bang Unibertsoa Lankide Aitor Larranaga Jaio Proba orria Inflazio kosmiko fa wikipedia org layihesinde istifadesi مه بانگ گیتی مسئله تخت بودن fi wikipedia org layihesinde istifadesi Maailmankaikkeus Alkurajahdys Maailmankaikkeuden muoto fr wikipedia org layihesinde istifadesi Forme de l Univers Courbure spatiale Geometrie riemannienne Big Bang Utilisateur Schnaggli Wikipedia Projets pedagogiques Cegep de Chicoutimi astro fr wikibooks org layihesinde istifadesi Cosmologie Les equations de Friedmann relativistes Cosmologie Version imprimable Bu faylin qlobal istifadesine baxin Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler error0 Menbe https az wikipedia org wiki Fayl End of universe jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,
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