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参宿六

File:Orion_constellation_map.svg · Wikimedia Commons · See Wikimedia Commons

EntityQ14028· pop 40· linked from 167 articles

Also known as Kappa Orionis, κ Orionis, κ Ori, ROT 929, WH 507, SAO 132542, PPM 188455, PLX 1330

Saiph , designation Kappa Orionis (κ Orionis, abbreviated Kappa Ori, κ Ori) and 53 Orionis (53 Ori), is a blue supergiant star and the sixth-brightest star in the constellation of Orion. Of the four bright stars that compose Orion's main quadrangle, it is the star at the south-eastern corner. A northern-hemisphere observer facing south would see it at the lower left of Orion, and a southern-hemisphere observer facing north would see it at the upper right. Parallax measurements yield an estimated distance of from the Sun. It is smaller, less luminous but hotter at its surface than Rigel with an

Wikidata facts

Instance of
variable star
Constellation
Orion
Distance from Earth
245
Radius
22.2
Image
Orion constellation map.png
Show 15 more facts
catalog code
ALS 14795
spectral class
B0
stellar rotational velocity
53
apparent magnitude
2.077826
right ascension
86.93912016833
declination
-9.66960491861
effective temperature
23170
right ascension component of proper motion
1
parallax
4.52
radial velocity
20.5
epoch
J2000.0
surface gravity
1000
luminosity
56.881
absolute magnitude
-6.1
declination component of proper motion
-2
Sources (4)

via Wikidata · CC0

Article · 中文

参宿六(κ Ori / 猎户座κ )是猎户座的第六亮星,俗名Saiph,其名称来源于阿拉伯语saif al jabbar,字面意思是巨人之剑。参宿六组成猎户座四边形的西南角。北半球的观测者可以在南方看到它位于猎户座的左下角;而南半球的观测者则可以在北方看到它位于猎户座的右上角。 参宿六距离太阳720光年,这跟参宿七与太阳的距离差不多,略近一些,二者的质量也接近,但是参宿六并未膨胀到参宿七般庞大,它的半径仅仅是太阳的14倍,与参宿七相比仅有1/5的大小。它的星等(+2.06)比参宿七更暗,因为表面温度高达26,500K,其辐射的能量大部分集中在人类肉眼无法看到的紫外波段,所以看起来更暗,由其质量推算其本真光度大约为太阳的8万3千倍,比参宿七略低一些。类似于参宿六的大恒星最终会自我崩塌并爆炸成为超新星。

Abstract from DBpedia / Wikipedia · CC BY-SA