English: This artist’s impression shows the final stages in the life of a supermassive star that fails to explode as a supernova but instead implodes under gravity to form a black hole. From left to right: the massive star has evolved to a red supergiant, the envelope of the star is ejected and expands, producing a cold, red transient source surrounding the newly formed black hole. Some residual material may fall onto the black hole, as illustrated by the stream and the disc, potentially powering some optical and infrared emissions years after the collapse.
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https://creativecommons.org/licenses/by/4.0CC BY 4.0 Creative Commons Attribution 4.0 truetrue
این پرونده حاوی اطلاعات اضافهای است که احتمالاً دوربین دیجیتال یا پویشگری که در ایجاد یا دیجیتالی کردن آن به کار رفته آن را افزوده است. اگر پرونده از وضعیت ابتداییاش تغییر داده شده باشد آنگاه ممکن است شرح و تفصیلات موجود اطلاعات تصویر را تماماً بازتاب ندهد.
صاحب امتیاز/ارائه کننده
NASA, ESA, and P. Jeffries (STScI)
منبع
ESA/Hubble
عنوان کوتاه
N6946-BH1 failed supernova (artist's impression)
عنوان تصویر
This artist’s impression shows the final stages in the life of a supermassive star that fails to explode as a supernova but instead implodes under gravity to form a black hole. From left to right: the massive star has evolved to a red supergiant, the envelope of the star is ejected and expands, producing a cold, red transient source surrounding the newly formed black hole. Some residual material may fall onto the black hole, as illustrated by the stream and the disc, potentially powering some optical and infrared emissions years after the collapse. Links: NASA press release N6946-BH1
شرایط استفاده
Creative Commons Attribution 4.0 International License
تاریخ و زمان تولید دادهها
۲۶ مهٔ ۲۰۱۷، ساعت ۱۳:۴۲
توضیحات پرونده JPEG
This illustration shows the final stages in the life of a supermassive star that fails to explode as a supernova but instead implodes under gravity to form a black hole. From left to right: the massive star has evolved to a red supergiant, the envelope of the star is ejected and expands, producing a cold, red transient source surrounding the newly formed black hole. Some residual material may fall onto the black hole, as illustrated by the stream and the disk, potentially powering some optical and infrared emissions years after the collapse.