Langbahn Team – Weltmeisterschaft

File:Accretion Disk Binary System.jpg

Accretion_Disk_Binary_System.jpg (800 × 525 pixels, file size: 24 KB, MIME type: image/jpeg)

Summary

  • 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

Licensing

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:

Captions

Accretion disk binary system

Items portrayed in this file

depicts

copyright status

public domain

applies to jurisdiction: United States of America
determination method or standard: work of the federal government of the United States

media type

image/jpeg

checksum

c2b18215b87deac56d4a7904bce470282e070bff

determination method or standard: SHA-1

data size

24,805 byte

height

525 pixel

width

800 pixel

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current23:58, 24 January 2008Thumbnail for version as of 23:58, 24 January 2008800 × 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

Global file usage

The following other wikis use this file:

View more global usage of this file.

Metadata