XMM-Newton Space Telescope
XMM-Newton 太空望远镜
XMM-Newton Light Paths for X-rays
Image credit:ESA / AOES Medialab
 |
The XMM-Newton (X-ray Multimirror Misson-Newton) is an orbiting X-ray observatory launched by ESA in December 1999. It is in a highly elliptical orbit with apogee 114,000 km and perigee 7000 km. The intended observations for XMM Newton include the detection of X-ray emissions from Solar System objects and detailed studies of star-forming regions. One of the star-forming regions that has been observed is M-16, the Eagle Nebula. XMM-Newton（X射线多镜任务-牛顿）是欧洲航天局（ESA）于1999年12月发射的轨道X射线天文卫星。它处于一个高度椭圆轨道上，近地点7000公里，远地点114000公里。XMM-Newton的观测目标包括探测太阳系天体的X射线辐射以及对恒星形成区进行详细研究。其中已观测到的一个恒星形成区是M-16，即鹰星云。 |
References:
参考文献：
| Telescopes
望远镜 |
XMM-Newton光路径
XMM-牛顿光路径用于X射线图像。信用：ESA / AOES Medialab
Chandra X-ray Observatory
Solar System Concepts
索引钱德勒X射线望远镜太阳系概念
| HyperPhysics********** Astrophysics
HyperPhysics ********** 天体物理学 | R Nave |
返回