Fil:Accretion Disk Binary System.jpg

Page contents not supported in other languages.
Fra Wikipedia, den frie encyklopædi

Accretion_Disk_Binary_System.jpg(800 × 525 billedpunkter, filstørrelse: 24 KB, MIME-type: image/jpeg)


Denne fil er fra Wikimedia Commons

Beskrivelse

  • English: Accretion Disk Binary System. NASA's explanation:
Our Sun is unusual in that it is alone - most stars occur in multiple or binary systems. In a binary system, the higher mass star will evolve faster and will eventually become a compact object - either a white dwarf star, a neutron star, or black hole. When the lower mass star later evolves into an expansion phase, it may be so close to the compact star that its outer atmosphere actually falls onto the compact star. Such is the case diagrammed above (artwork). Here gas from a blue giant star is shown being stripped away into an accretion disk around its compact binary companion. Gas in the accretion disk swirls around, heats up, and eventually falls onto the compact star. Extreme conditions frequently occur on the surface of the compact star as gas falls in, many times causing detectable X-rays, gamma-rays, or even cataclysmic novae explosions. Studying the extreme conditions in these systems tells us about the inner properties of ordinary matter around us.

Source: http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/23/image/a
Credit: STScI

Licensering

Public domain Denne fil er i offentligt domæne i USA fordi den udelukkende er skabt af NASA. NASAs ophavsretspolitik erklærer at materiale udgivet af NASA ikke er omfattet af ophavsret medmindre andet er nævnt. (Se også Template:PD-USGov, NASAs ophavsretspolitik eller JPLs politik for brug af billeder.)
Advarsler:

Captions

Tilføj en kort forklaring på en enkelt linje om hvad filen viser
Accretion disk binary system

Elementer som er med i denne fil

afbilder

image/jpeg

c2b18215b87deac56d4a7904bce470282e070bff

24.805 Byte

525 pixel

800 pixel

Filhistorik

Klik på en dato/tid for at se filen som den så ud på det tidspunkt.

Dato/tidMiniaturebilledeDimensionerBrugerKommentar
nuværende25. jan. 2008, 01:58Miniature af versionen fra 25. jan. 2008, 01:58800 × 525 (24 KB)Ilmari Karonen*{{en|Accretion Disk Binary System. NASA's explanation: :Our Sun is unusual in that it is alone - most stars occur in multiple or binary systems. In a binary system, the higher mass star will evolve faster and will eventually become a compact object - eit

Den følgende side bruger denne fil:

Global filanvendelse

Metadata