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单词 Quasar 3C273
释义

Quasar 3C273

中文百科

3C 273 3C 273

(重定向自Quasar 3C273)
使用哈伯太空望远镜的先进巡天照相机拍摄的3C 273。创建者:NASA/ESA。
使用哈伯太空望远镜的摄影图
Position de 3C 273 dans la constellation de la Vierge.

3C 273是位于室女座的一个类星体。它在可见光波段上是最明亮的一个类星体,在天空中的视星等大约是12.9等,是最靠近地球的类星体之一,红移 z只有0.158。它的光度距离,D L = 24.4亿光年(749 Mpc)是经由z值换算的。它也是最明亮的类星体之一,绝对星等为-26.7等。通过对它宽广的发射谱线的回荡映射 reverberation mapping测量,它的质量是太阳质量的8.86 ± 1.87 亿倍。

英语百科

3C 273 3C 273

(重定向自Quasar 3C273)
3C 273 as imaged by the Hubble Space Telescope's Advanced Camera for Surveys. Credit: NASA/ESA.
Quasar 3C 273, with its jet. Image by Chandra X-ray Observatory
Position de 3C 273 dans la constellation de la Vierge.

3C 273 is a quasar located in the constellation Virgo. It was the first quasar ever to be identified.

It is the optically brightest quasar in our sky (m ~12.9), and one of the closest with a redshift, z, of 0.158. A luminosity distance of DL = 749 megaparsecs (2.4 Gly) may be calculated from z. It is also one of the most luminous quasars known, with an absolute magnitude of −26.7, meaning that if it were only as distant as Pollux (~10 parsecs) it would appear nearly as bright in the sky as the Sun. Since the sun's absolute magnitude is 4.83, it means that the quasar is over 4 trillion times brighter than the sun. Its mass has been measured to be 886 ± 187 million solar masses through broad emission-line reverberation mapping.

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更新时间:2025/6/24 1:03:20