Lêer:Gamma_ray_burst.jpg
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Oorspronklike lêer (2 000 × 1 396 piksels, lêergrootte: 1,23 MG, MIME-tipe: image/jpeg)
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BeskrywingGamma 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. |
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Datum | ||||||
Bron | National Science Foundation Press Release 05-156: Gamma-Ray Burst Smashes a Record | |||||
Outeur | Nicolle Rager Fuller of the NSF | |||||
Toestemming (Hergebruik van die lêer) |
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Items portrayed in this file
uitbeelding
12 September 2005
media type Engels
image/jpeg
Lêergeskiedenis
Klik op die datum/tyd om te sien hoe die lêer destyds gelyk het.
Datum/Tyd | Duimnael | Dimensies | Gebruiker | Opmerking | |
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huidig | 13:46, 17 September 2007 | 2 000 × 1 396 (1,23 MG) | Jehochman | 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 |
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- Gamma-ray burst
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