跳转到内容

File:Gamma-ray-burst-Mechanism.jpg

页面内容不支持其他语言。
这个文件来自维基共享资源
维基百科,自由的百科全书

原始文件 (3,840 × 2,160像素,文件大小:633 KB,MIME类型:image/jpeg


摘要

描述
English: MECHANISM OF GAMMA-RAY BURSTS

https://earthsky.org/space/jan-14-2019-gamma-ray-burst-brightest-so-far

What are gamma ray bursts? They are cosmic explosions, with radiation up to a trillion times the energy of visible light. This illustration shows the set-up for the most common type of gamma ray burst. The core of a massive star (left) has collapsed and formed a black hole. This “engine” drives a jet of particles that moves through the collapsing star and out into space at nearly the speed of light. The prompt emission, which typically lasts a minute or less, may arise from the jet’s interaction with gas near the newborn black hole and from collisions between shells of fast-moving gas within the jet (internal shock waves). The afterglow emission occurs as the leading edge of the jet sweeps up its surroundings (creating an external shock wave) and emits radiation across the spectrum for some time — months to years, in the case of radio and visible light, and many hours at the highest gamma-ray energies yet observed. These far exceed 100 billion electron volts (GeV) for two recent GRBs.
日期
来源 https://en.es-static.us/upl/2019/11/gamma-ray-burst-mechanism-lg.jpg
作者 NASA/Goddard Space Flight Center/ICRAR.

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/zhNASA版权方针页面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
Gamma-ray-burst Mechanism - November 24, 2019

此文件中描述的项目

描绘内容

image/jpeg

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2019年11月25日 (一) 16:532019年11月25日 (一) 16:53版本的缩略图3,840 × 2,160(633 KB)DrbogdanUser created page with UploadWizard

以下页面使用本文件:

全域文件用途

以下其他wiki使用此文件:

元数据