跳至內容

File:Accretion Disk Binary System.jpg

頁面內容不支援其他語言。
這個檔案來自維基共享資源
維基百科,自由的百科全書

Accretion_Disk_Binary_System.jpg (800 × 525 像素,檔案大小:24 KB,MIME 類型: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

授權條款

Public domain 本作品由NASA創作,屬於公有領域。根據NASA的版權政策:“NASA的創作除非另有聲明否則不受版權保護。”(參見:Template:PD-USGov/zhNASA版權政策JPL圖像使用政策
警告:

說明

添加單行說明來描述出檔案所代表的內容
Accretion disk binary system

在此檔案描寫的項目

描繪內容

image/jpeg

c2b18215b87deac56d4a7904bce470282e070bff

斷定方法:​SHA-1 中文 (已轉換拼寫)

24,805 位元組

525 像素

800 像素

檔案歷史

點選日期/時間以檢視該時間的檔案版本。

日期/時間縮⁠圖尺寸使用者備⁠註
目前2008年1月24日 (四) 23:58於 2008年1月24日 (四) 23:58 版本的縮圖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

全域檔案使用狀況

詮釋資料