File:Grand star-forming region R136 in NGC 2070 (captured by the Hubble Space Telescope).jpg
![File:Grand star-forming region R136 in NGC 2070 (captured by the Hubble Space Telescope).jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/2/25/Grand_star-forming_region_R136_in_NGC_2070_%28captured_by_the_Hubble_Space_Telescope%29.jpg/587px-Grand_star-forming_region_R136_in_NGC_2070_%28captured_by_the_Hubble_Space_Telescope%29.jpg?20091224000755)
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[edit]DescriptionGrand star-forming region R136 in NGC 2070 (captured by the Hubble Space Telescope).jpg |
العربية: تظهر صورة تلكسوب هبل هذه مئات النجوم الحديثة الولادة داخل حضانة نجمية في سحابة ماجلان الكبرى وتسمى سديم "دورادوس 30"، وهذه هي أكثر الحضانات النجمية المعروفة خصوبة وحجما في جميع المجرات المجاورة لدرب التبانة، وهذه المجموعة الكبيرة من النجوم الحديثة التكوين الظاهرة في الصورة تسمى "آر136" وعمرها يبلغ بضعة ملايين من السنين فقط، والعديد من هذه النجوم الزرقاء هي من بعض أكبر الأحجام المعروف للنجوم فأحجام الكثير منها تصل إلى أكثر من 100 ضعف حجم الشمس، ويتوقع العلماء أن هذه النجوم بعد بضعة ملايين من السنين فقط سوف تنفجر في سلسلة من "المستعرات العظيمة" (السوبرنوفا) مثل المفرقعات النارية، وهذه الصورة التقطها تلسكوب هبل بالأشعة فوق البنفسجية لمساحة يبلغ عرضها 100 سنة ضوئية.
وهذا السديم قريب من الأرض كفاية حتى يستطيع هبل إظهار النجوم منفردة (أي لا تبدو كسحابة غبشاء مثل المجرات البعيدة بل يبدو كل نجم وحده بوضوح) مما أعطى الفلكيين معلومات هامة عن ولادة النجوم ونموها، وربما تكون درب التبانة وسحابة ماجلان الصغرى قد زادتا ولادة النجوم في السديم بسبب جاذبيتهما التي تتسبب بضغط الغاز داخل سحابة ماجلان الكبرى، ومن الممكن أن دورانها حول درب التبانة يساهم أيضا في ضغط الغاز. الألوان في الصورة: الأجسام الزرقاء هي بعض أكثر النجوم المعروفة حرارة وحجما، والأخضر هو لون الأكسجين والأحمر هو الهيدروجين.Deutsch: Der Supersternhaufen R136 nahe dem Zentrum des Emissionsnebels 30 Doradus (auch als Tarantelnebel oder NGC 2070 bekannt) vom Hubble-Weltraumteleskop aufgenommen. (Dieses JPG-Bild wurde aus einer TIFF-Datei erzeugt)
English: A Hubble Space Telescope image of the R136 super star cluster, near the center of the 30 Doradus Nebula, also known as the Tarantula Nebula or NGC 2070. (Converted to JPG from the source TIFF file)
Esperanto: Kosmoteleskopo Hubble bildo de la R136 súper stelo peniko, proksime de la centro de la 30 Doradus Nebulozo, ankaŭ sciata kiel la Tarántula Nebulozo aŭ NGC 2070. (Konvertiĝis al JPG el la fonta TIFF-dosiero)
Français : Image du superamas d'étoiles R136, près du centre de la Nébuleuse de la Tarentule (NGC 2070), obtenue avec le télescope spatial Hubble.
Македонски: Ѕвезденото јато R136 близу средиштето на маглината „30 Златна Рипка“ (наречена и „Тарантула“, NGC 2070). Сликата е направена со вселенскиот телескоп „Хабл“.
Русский: R136 — компактное звёздное скопление, которое находится в центре туманности «Тарантул» (галактика NGC 2070). Фото сделано с помощью телескопа «Хаббл». |
Date | Between 20 October 2009 and 27 October 2009 |
Source | http://hubblesite.org/newscenter/archive/releases/2009/32/image/a/ (direct link) |
Author | NASA, ESA, F. Paresce (INAF-IASF, Bologna, Italy), R. O'Connell (University of Virginia, Charlottesville), and the Wide Field Camera 3 Science Oversight Committee |
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Assessment
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This image was selected as picture of the day on Wikimedia Commons for 16 July 2012. It was captioned as follows: English: A Hubble Space Telescope image of the R136 super star cluster, near the center of the 30 Doradus Nebula, also known as the Tarantula Nebula or NGC 2070. Other languages:
Deutsch: Der Supersternhaufen R136 nahe dem Zentrum des Emissionsnebels 30 Doradus (auch als Tarantelnebel oder NGC 2070 bekannt) vom Hubble-Weltraumteleskop aufgenommen. English: A Hubble Space Telescope image of the R136 super star cluster, near the center of the 30 Doradus Nebula, also known as the Tarantula Nebula or NGC 2070. Español: Una imagen del Telescopio Espacial Hubble del supercúmulo estelar R136, cerca del centro de la nebulosa 30 Doradus, también conocida como Nebulosa de la Tarántula o NGC 2070. Italiano: Foto scattata dal telescopio spaziale Hubble dell'ammasso aperto R136, vicino al centro della Nebulosa Tarantola. Nederlands: Een afbeelding gemaakt door ruimtetelescoop Hubble van het supersterrencluster R136, nabij het centrum van de Tarantulanevel of NGC 2070. Македонски: Ѕвезденото јато R136 близу средиштето на маглината „30 Златна Рипка“ (наречена и „Тарантула“, NGC 2070). Сликата е направена со вселенскиот телескоп „Хабл“. Русский: Галактика NGC 2070. Снимок сделан космическим телескопом Хаббла. |
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Deutsch: Dieses Bild wurde als Bild der Woche auf der tschechischen Wikipedia für die 50. Woche 2016 ausgewählt. English: This image was selected as a picture of the week on the Czech Wikipedia for 50th week, 2016. Français : Cette image est sélectionnée en tant qu’image de la semaine sur la Wikipédia Tchèque pour la 50e semaine de 2016. Italiano: Questa immagine è stata selezionata come Immagine della settimana su Wikipedia in ceco per la L settimana del 2016. Македонски: Сликава е избрана за слика на неделата на чешката Википедија за L недела од 2016 година. Русский: Эта иллюстрация была выбрана изображением недели в чешском разделе «Википедии» для недели номер 50 2016 года. Українська: Ця ілюстрація була вибрана зображенням тижня в чеському розділі «Вікіпедії» для тижня номер 50, 2016 року. |
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Licensing
[edit]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. |
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Annotations InfoField | This image is annotated: View the annotations at Commons |
R136
Melnick 34
Melnick 42
R134
Melnick 39
R145
File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 00:07, 24 December 2009 | ![]() | 3,939 × 4,024 (11.15 MB) | Tryphon (talk | contribs) | Higher resolution, from http://imgsrc.hubblesite.org/hu/db/images/hs-2009-32-a-full_jpg.jpg. |
23:49, 23 December 2009 | ![]() | 2,981 × 2,981 (6.12 MB) | Tryphon (talk | contribs) | {{Information |Description=This is the most detailed view of the largest stellar nursery in our local galactic neighborhood. The massive, young stellar grouping, called R136, is only a few million years old and resides in the 30 Doradus Nebula, a turbulen |
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File change date and time | 15:25, 10 December 2009 |
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