File:Gamma ray burst.jpg
来自Wikimedia Commons
跳转到导航
跳转到搜索
本预览的尺寸:800 × 558像素。 其他分辨率:320 × 223像素 | 640 × 447像素 | 1,024 × 715像素 | 1,280 × 893像素 | 2,000 × 1,396像素。
原始文件 (2,000 × 1,396像素,文件大小:1.23 MB,MIME类型:image/jpeg)
文件信息
结构化数据
说明
描述Gamma ray burst.jpg |
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 | ||||||
来源 | National Science Foundation Press Release 05-156: Gamma-Ray Burst Smashes a Record | |||||
作者 | Nicolle Rager Fuller of the NSF | |||||
授权 (二次使用本文件) |
|
文件历史
点击某个日期/时间查看对应时刻的文件。
日期/时间 | 缩略图 | 大小 | 用户 | 备注 | |
---|---|---|---|---|---|
当前 | 2007年9月17日 (一) 13:46 | 2,000 × 1,396(1.23 MB) | Jehochman(留言 | 贡献) | This 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 |
您不可以覆盖此文件。
文件用途
以下7个页面使用本文件:
全域文件用途
以下其他wiki使用此文件:
- af.wikipedia.org上的用途
- ar.wikipedia.org上的用途
- ast.wikipedia.org上的用途
- bn.wikipedia.org上的用途
- ca.wikipedia.org上的用途
- ckb.wikipedia.org上的用途
- cs.wikipedia.org上的用途
- de.wikipedia.org上的用途
- el.wikipedia.org上的用途
- en.wikipedia.org上的用途
- Gamma-ray burst
- Eta Carinae
- GRB 970228
- User talk:Daniel Perley
- Wikipedia:Featured picture candidates/Gamma ray burst
- Wikipedia:Featured picture candidates/December-2007
- Gamma ray
- Portal:Astronomy/Featured/July 2009
- User talk:Cryptic C62/Archive 2
- User talk:Jehochman/Archive 21
- Wikipedia:Today's featured article/June 2011
- Wikipedia:Today's featured article/June 18, 2011
- Wikipedia:Main Page history/2011 June 18
- Wikipedia:WikiProject WikiFundi Content/Eta Carinae
- en.wikiquote.org上的用途
- eo.wikipedia.org上的用途
- es.wikipedia.org上的用途
- eu.wikipedia.org上的用途
- fa.wikipedia.org上的用途
- fi.wikipedia.org上的用途
- fr.wikipedia.org上的用途
- he.wikipedia.org上的用途
- hr.wikipedia.org上的用途
- ig.wikipedia.org上的用途
- it.wikipedia.org上的用途
- ja.wikipedia.org上的用途
查看此文件的更多全域用途。
元数据
此文件含有额外信息,这些信息可能是创建或数字化该文件时使用的数码相机或扫描仪所添加的。如果文件已从其原始状态修改,某些详细信息可能无法完全反映修改后的文件。
_error | 0 |
---|