跳去內容

File:Gamma ray burst.jpg

頁面內容唔支援其他語言。
出自維基百科,自由嘅百科全書

原本檔案 (2,000 × 1,396 像素,檔案大細:1.23 MB ,MIME類型:image/jpeg

描述
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.
日期
來源 National Science Foundation Press Release 05-156: Gamma-Ray Burst Smashes a Record
作者 Nicolle Rager Fuller of the NSF
許可
(重用呢個檔案)
© 我,National Science Foundation,呢個檔案嘅版權持有者,歡迎任何人係任何目的之下用呢幅圖。你可以改作、甚至用係商業用途都可以。
姓名標示:
National Science Foundation

VRT Wikimedia

呢個作品經已獲得授權使用,授權證明已經過確認同存檔喺維基媒體嘅VRT系統入邊。
有VRT帳號嘅用戶可以喺ticket #2010051310027124搵到。若果需要確認授權資訊,請聯絡有VRTS帳號嘅用戶或者喺VRT通告板留低訊息。

Ticket連結: https://ticket.wikimedia.org/otrs/index.pl?Action=AgentTicketZoom&TicketNumber=2010051310027124
Find other files from the same ticket: SDC query (SPARQL)

Captions

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

Items portrayed in this file

圖中顯示嘅係

12 9 2005

image/jpeg

檔案歷史

撳個日期/時間去睇響嗰個時間出現過嘅檔案。

日期/時間縮圖尺寸用戶註解
現時2007年9月17號 (一) 13:46響2007年9月17號 (一) 13:46嘅縮圖版本2,000 × 1,396(1.23 MB)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

以下嘅1版用到呢個檔:

全域檔案使用情況

下面嘅維基都用緊呢個檔案:

睇呢個檔案嘅更多全域使用情況

Metadata