跳转到内容

File:Accretion Disk Binary System.jpg

页面内容不支持其他语言。
這個文件來自維基共享資源
维基百科,自由的百科全书
    原始文件 (800 × 525像素,文件大小:24 KB,MIME类型:image/jpeg)


    摘要

    • 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

    许可协议

    Public domain 本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zh、NASA版权方针页面或JPL图片使用方针。)
    警告:

    说明

    添加一行文字以描述该文件所表现的内容
    Accretion disk binary system

    此文件中描述的项目

    描繪內容

    image/jpeg

    c2b18215b87deac56d4a7904bce470282e070bff

    24,805 字节

    525 像素

    800 像素

    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2008年1月24日 (四) 23:582008年1月24日 (四) 23:58版本的缩略图800 × 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

    全域文件用途

    元数据