集信:Hubble ultra deep field high rez edit1.jpg
交面
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戟𡱩形䀡𠓀:600×600點影。 度分解恪:240×240點影 | 480×480點影 | 768×768點影 | 1.024×1.024點影 | 2.048×2.048點影 | 6.200×6.200點影。
集信㭲 (6.200×6.200點影、戟𡱩集信:18,19 MB、矯MIME:image/jpeg)
集信尼得留於威其迷𠫾阿・古門吧伮固体得使用於各預案恪。 𠳒描寫𧵑集信在張模寫得顯示𨑜低。
Summary
DescriptionHubble ultra deep field high rez edit1.jpg |
Afrikaans: Hierdie foto van 'n afgeleë segment van die heelal is saamgestel uit data wat vanaf 3 September 2003 tot 16 Januarie 2004 deur die Hubble-ruimteteleskoop verkry is. Dit bevat sterrestelsels van verskeie ouderdomme, vorme, groottes en kleure. Die kleinstes en rooistes hiervan is sommige van die verste sterrestelsels wat ooit met 'n optiese teleskoop waargeneem is, en het kort na die oerknal reeds bestaan. Die gekose gebied bevat min sterre op die voorgrond, en is suidwestelik van Orion in die sterrebeeld Fornax geleë.
Deutsch: Das Hubble Ultra Deep Field ist ein Bild einer kleinen Himmelsregion aufgenommen vom Hubble-Weltraumteleskop über einen Zeitraum vom 3. September 2003 bis 16. Januar 2004. Dabei wurde eine Himmelsregion ausgewählt, die kaum störende helle Sterne im Vordergrund enthält. Man entschied sich für ein Zielgebiet südwestlich von Orion im Sternbild Chemischer Ofen.
English: The Hubble Ultra Deep Field, is an image of a small region of space in the constellation Fornax, composited from Hubble Space Telescope data accumulated over a period from September 3, 2003 through January 16, 2004. The patch of sky in which the galaxies reside was chosen because it had a low density of bright stars in the near-field.
Español: El Campo Ultra Profundo del Hubble, es una imagen de una pequeña región del espacio en la constelación Fornax, compuesta de datos obtenidos por el telescopio espacial Hubble durante el período entre el 3 de Septiembre de 2003 y el 16 de Enero de 2004. Esta parte del cielo fue escogida por su baja densidad de estrellas brillantes en sus proximidades.
Français : Le champ ultra profond de Hubble, une image d'une petite portion du ciel dans la constellation du Fourneau, prise par le télescope spatial Hubble du 3 septembre 2003 au 16 juillet 2004. La portion de ciel a été choisie car elle possède peu d'étoiles brillantes proches. |
Date |
between 3 September 2003 and 16 January 2004 date QS:P,+2003-00-00T00:00:00Z/8,P1319,+2003-09-03T00:00:00Z/11,P1326,+2004-01-16T00:00:00Z/11 |
Source | https://hubblesite.org/contents/news-releases/2004/news-2004-07.html |
Author | NASA and the European Space Agency. Edited by Noodle snacks |
Other versions | Image:Hubble ultra deep field.jpg |
This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: Black point adjustment.
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Licensing
Public domainPublic domainfalsefalse |
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This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag. |
Assessment
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Captions
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Hubble Ultra Deep Field, an image of a small segment of space in constellation Fornax
الكون الكائن من الانفجار العظيم الذي داخله يتكون كل شيء.
Items portrayed in this file
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media type English
image/jpeg
歷史集信
扨𠓨𣈜/𣇞抵䀡內容集信在時點妬。
𣈜/𣇞 | 形䀡𠓀 | 戟櫸 | 成員 | 描寫 | |
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現在 | 15:39、𣈜25𣎃11𢆥2008 | ![]() | 6.200×6.200 (18,19 MB) | wikimediacommons>JJ Harrison | ==Summary== {{Information |Description = {{de|Das Hubble Ultra Deep Field ist ein Bild einer kleinen Himmelsregion aufgenommen vom Hubble-Weltraumteleskop über einen Zeitraum vom 3. September 2003 bis 16. Januar 2004. |
張使用集信
張𢖖󠄁使用集信尼:
特性形
集信尼貯通信補充、固体得添自𣛠影技術數或𣛠𢭯得使用抵造或數化集信。
裊集信㐌得𢯢𢷮𬧺貝狀態班頭、𠬠數枝節固体空反暎𣹓𨁥集信㐌𢯢𢷮。
標題𧵑形 |
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向 | 常 |
分解蹺朝卬 | 600點/印初 |
分解蹺朝高 | 600點/印初 |
份繌使用 | Adobe Photoshop CS3 Windows |
𣈜𣇞𢯢集信 | 19:19、𣈜25𣎃11𢆥2008 |
空間𦭷 | 𣗓校整 |
朝卬形 | 6.200 點影 |
朝高形 | 6.200 點影 |
𣈜𣇞數化 | 06:56、𣈜2𣎃3𢆥2004 |
𣈜𢯢超與料吝𡳳 | 06:19、𣈜26𣎃11𢆥2008 |
番版IIM | 2 |