ملف:Starburst galaxy NGC 1569 (opo0838a).jpg
المزيد من الإجراءات
الملف الأصلي (3٬258 × 1٬960 بكسل حجم الملف: 3٫05 ميجابايت، نوع MIME: image/jpeg)
| هذا ملف من ويكيميديا كومنز. معلومات من صفحة وصفه مبينة في الأسفل. كومنز مستودع ملفات ميديا ذو رخصة حرة. |
ملخص
| الوصفStarburst galaxy NGC 1569 (opo0838a).jpg |
English: This image taken by NASA/ESA Hubble Space Telescope showcases the brilliant core of one of the most active galaxies in our local neighbourhood. The entire core is 5000 light-years wide.The galaxy, called NGC 1569, sparkles with the light from millions of newly formed young stars. NGC 1569 is pumping out stars at a rate that is 100 times faster than the rate observed in our Milky Way Galaxy. This frenzied pace has been almost continuous for the past 100 million years.The core's centrepiece is a grouping of three giant star clusters, each containing more than a million stars. (Two of the clusters are so close they appear as one grouping.) The clusters reside in a large, central cavity. The gas in the cavity has been blown out by the multitude of massive, young stars that already exploded as supernovae. These explosions also triggered a violent flow of gas and particles that is sculpting giant gaseous structures. The sculpted structure at lower right is about 3700 light-years long.Huge bubbles of gas, such as the two at left, appear like floating islands. The largest bubble is about 378 light-years wide and the smallest 119 light-years wide. They are being illuminated by the radiation from the bright, young stars within them. Some of those stars are peaking through their gaseous cocoons.The biggest and brightest objects surrounding the core are stars scattered throughout our Milky Way Galaxy. In contrast, the thousands of tiny white dots in the image are stars in the halo of NGC 1569. The galaxy is 11 million light-years from Earth.A new analysis of NGC 1569 shows that it is one and a half times farther from Earth than astronomers previously thought. The extra distance places the galaxy in the middle of a group of about 10 galaxies centered on the spiral galaxy IC 342. Gravitational interactions among the group's galaxies may be compressing gas in NGC 1569 and igniting the star-birthing frenzy.Hubble's Wide Field Planetary Camera 2 and Advanced Camera for Surveys made the observations of NGC 1569 in September 1999, November 2006, and January 2007. |
| التاريخ | ٢٠ نوفمبر ٢٠٠٨ (تاريخ الرفع) |
| المصدر | Starburst galaxy NGC 1569 |
| المؤلف | Credit for Advanced Camera Data: NASA, ESA, A. Aloisi (STScI/ESA), J. Mack and A. Grocholski (STScI), M. Sirianni (STScI/ESA), R. van der Marel (STScI), L. Angeretti, D. Romano, and M. Tosi (INAF-OAB), and F. Annibali, L. Greggio, and E. Held (INAF-OAP) Credit for Wide Field Planetary Camera 2 Data: NASA, ESA, P. Shopbell (California Institute of Technology), R. Dufour (Rice University), D. Walter (South Carolina State University, Orangeburg), and A. Wilson (University of Maryland, College Park) |
| إصدارات أخرى |
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ترخيص
| Public domainPublic domainfalsefalse |
يقع هذا الملفُّ في ملكية عامة لأنَّه أُنشِئ بواسطة ناسا (ناسا) ووكالة الفضاء الأوروبيَّة. ليس هناك حقوق تأليفٍ ونشرٍ على المواد التي تنتجها وكالة الفضاء الأمريكية بواسطة مَرصَد هابِل (وكذا الأمر للمواد التي أنتجتها وكالة الفضاء الأوروبية قبل العام 2008م) ويمكن بالتالي استعمالها بحرية دون أي كلفة مادية. لا تنطبق هذه الرُّخصة على المواد الَّتي أنتجتها وكالة الفضاء الأوروبيَّة بعد العام 2008.
مِن أجل المواد الَّتي أَنشأتها ناسا عبر مَعهد مَراصد علوم الفضاء حسب العقد NAS5-26555 ومِن أجل المواد التي أنشأتها وكالة الفضاء الأوروبيَّة عبر مركز معلومات هابل انظر تصريح حقوق التَّأليف والنَّشر على موقع مرصد هابل ووتصريح حقوق التَّأليف والنَّشر الخاصّ بالوكالة الأوروبيَّة في عام 2008. مِن أَجل المواد التي أنشأتها وكالة الفضاء الأوروبيَّة spacetelescope.org ونشرتها على موقع منذ العام 2009، استعمل قالب {{ESA-Hubble}}. |
الشروحات
العناصر المصورة في هذا الملف
يُصوِّر
image/jpeg
١٬٩٦٠ بكسل
٣٬٢٥٨ بكسل
4bc650810106c5ab66745a91b814f1c52a75bbb6
٢٠ نوفمبر 2008
pHash checksum الإنجليزية
4v4wrn6r3rgowaw9hg5k7pwyfz8al4coj80p4kjfevah91l7u9
تاريخ الملف
اضغط على زمن/تاريخ لرؤية الملف كما بدا في هذا الزمن.
| زمن/تاريخ | صورة مصغرة | الأبعاد | مستخدم | تعليق | |
|---|---|---|---|---|---|
| حالي | 22:27، 21 فبراير 2026 | 3٬258 × 1٬960 (3٫05 ميجابايت) | wikimediacommons>OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esahubble.org/archives/images/large/opo0838a.jpg via Commons:Spacemedia |
استخدام الملف
الصفحتان التاليتان تستخدمان هذا الملف:
بيانات وصفية
هذا الملف يحتوي على معلومات إضافية، غالبا ما تكون أضيفت من قبل الكاميرا الرقمية أو الماسح الضوئي المستخدم في إنشاء الملف.
إذا كان الملف قد عدل عن حالته الأصلية، فبعض التفاصيل قد لا تعبر عن الملف المعدل.
| عنوان الصورة |
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|---|---|
| الرصيد/المزود | Credit for Advanced Camera Data: NASA, ESA, A. Aloisi (STScI/ESA), J. Mack and A. Grocholski (STScI), M. Sirianni (STScI/ESA), R. van der Marel (STScI), L. Angeretti, D. Romano, and M. Tosi (INAF-OAB), and F. Annibali, L. Greggio, and E. Held (INAF-OAP)Credit for Wide Field Planetary Camera 2 Data: NASA, ESA, P. Shopbell (California Institute of Technology), R. Dufour (Rice University), D. Walter (South Carolina State University, Orangeburg), and A. Wilson (University of Maryland, College Park) |
| المصدر | ESA/Hubble |
| عنوان قصير |
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| شروط الاستخدام |
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| تاريخ ووقت توليد البيانات | 15:00، 20 نوفمبر 2008 |
| تعليق ملف JPEG | This image taken by NASA/ESA Hubble Space Telescope showcases the brilliant core of one of the most active galaxies in our local neighbourhood. The entire core is 5000 light-years wide. The galaxy, called NGC 1569, sparkles with the light from millions of newly formed young stars. NGC 1569 is pumping out stars at a rate that is 100 times faster than the rate observed in our Milky Way Galaxy. This frenzied pace has been almost continuous for the past 100 million years. The core's centrepiece is a grouping of three giant star clusters, each containing more than a million stars. (Two of the clusters are so close they appear as one grouping.) The clusters reside in a large, central cavity. The gas in the cavity has been blown out by the multitude of massive, young stars that already exploded as supernovae. These explosions also triggered a violent flow of gas and particles that is sculpting giant gaseous structures. The sculpted structure at lower right is about 3700 light-years long. Huge bubbles of gas, such as the two at left, appear like floating islands. The largest bubble is about 378 light-years wide and the smallest 119 light-years wide. They are being illuminated by the radiation from the bright, young stars within them. Some of those stars are peaking through their gaseous cocoons. The biggest and brightest objects surrounding the core are stars scattered throughout our Milky Way Galaxy. In contrast, the thousands of tiny white dots in the image are stars in the halo of NGC 1569. The galaxy is 11 million light-years from Earth. A new analysis of NGC 1569 shows that it is one and a half times farther from Earth than astronomers previously thought. The extra distance places the galaxy in the middle of a group of about 10 galaxies centered on the spiral galaxy IC 342. Gravitational interactions among the group's galaxies may be compressing gas in NGC 1569 and igniting the star-birthing frenzy. Hubble's Wide Field Planetary Camera 2 and Advanced Camera for Surveys made the observations of NGC 1569 in September 1999, November 2006, and January 2007. |
| الكلمات المفتاحية | NGC 1569 |
| معلومات الاتصال |
http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
| نسخة IIM | 4 |