پەڕگە:Gamma ray burst.jpg

پەڕگەی سەرەکی(٢٬٠٠٠ × ١٬٣٩٦ پیکسڵ، قەبارەی پەڕگە: ١٫٢٣ مێگابایت، جۆری ئێم ئای ئێم ئی: image/jpeg)

ئەم پەڕگە لە Wikimedia Commonsەوەیە و لەوانەیە لە پڕۆژەکانی دیکەش بەکار ھاتبێت. پێناسەکەی لەسەر پەڕەی وەسفی پەڕگەکە لە خوارەوە نیشان دراوە.

وەسف
English: Drawing of a massive star collapsing to form a black hole. Energy released as jets along the axis of rotation forms a gamma ray burst that lasts from a few milliseconds to minutes. Such an event within several thousand light years of Earth could disrupt the biosphere by wiping out half of the ozone layer, creating nitrogen dioxide and potentially cause a mass extinction. Stars shine by burning hydrogen. The process is called nuclear fusion. Hydrogen burning produces helium "ash." As the star runs out of hydrogen (and nears the end of its life), it begins burning helium. The ashes of helium burning, such as carbon and oxygen, also get burned. The end result of this fusion is iron. Iron cannot be used for nuclear fuel. Without fuel, the star no longer has the energy to support its weight. The core collapses. If the star is massive enough, the core will collapse into a black hole. The black hole quickly forms jets; and shock waves reverberating through the star ultimately blow apart the outer shells. Gamma-ray bursts are the beacons of star death and black hole birth.
ڕێکەوت
سەرچاوە National Science Foundation Press Release 05-156: Gamma-Ray Burst Smashes a Record
بەرھەمھێنەر Nicolle Rager Fuller of the NSF
ڕێپێدان
(بەکارھێنانەوەی ئەم پەڕگەیە)
© The copyright holder of this file, National Science Foundation, allows anyone to use it for any purpose, provided that the copyright holder is properly attributed. Redistribution, derivative work, commercial use, and all other use is permitted.
دانەپاڵ:
National Science Foundation

VRT Wikimedia

This work is free and may be used by anyone for any purpose. If you wish to use this content, you do not need to request permission as long as you follow any licensing requirements mentioned on this page.

The Wikimedia Foundation has received an e-mail confirming that the copyright holder has approved publication under the terms mentioned on this page. This correspondence has been reviewed by a Volunteer Response Team (VRT) member and stored in our permission archive. The correspondence is available to trusted volunteers as ticket #2010051310027124.

If you have questions about the archived correspondence, please use the VRT noticeboard. Ticket link: https://ticket.wikimedia.org/otrs/index.pl?Action=AgentTicketZoom&TicketNumber=2010051310027124
Find other files from the same ticket: SDC query (SPARQL)

لێدوانەکان

Add a one-line explanation of what this file represents
lee pa

بەندەکانی لەم پەڕگەیەدا دەردەکەون

depicts ئینگلیزی

١٢ ئەیلوولی 2005

MIME type ئینگلیزی

image/jpeg

مێژووی پەڕگە

کرتە بکە لەسەر یەکێک لە ڕێکەوت/کاتەکان بۆ بینینی پەڕگەکە بەو شێوەی لەو کاتەدا بووە.

ڕێکەوت/کاتھێمائەندازەبەکارھێنەرتێبینی
هەنووکە‏١٣:٤٦، ١٧ی ئەیلوولی ٢٠٠٧ھێما بۆ وەشانی  ‏١٣:٤٦، ١٧ی ئەیلوولی ٢٠٠٧٢٬٠٠٠ لە ١٬٣٩٦ (١٫٢٣ مێگابایت)JehochmanThis image was created by the National Science Foundation and is in the public domain. Credit: Nicolle Rager Fuller/NSF http://www.nsf.gov/news/news_images.jsp?cntn_id=104440&org=NSF

ئەم پەڕەی 2ە ئەم پەڕگەیە بەکار دەھێنێت:

بەکارھێنانی سەرانسەریی پەڕگە

ئەم ویکیانەی دیکەی خوارەوەش ئەم پەڕگە بەکاردێنن:

بینینی بەکارھێنانی گشتی زیاتری ئەم پەڕگەیە.

دراوی مێتا