附近星空(赤道坐标,上北下南),在星图里打开

恒星 › 武仙座

中山增一

武仙座 ξ
视星等
3.70肉眼可见
绝对星等
0.59
距离
137 光年41.9 秒差距
光谱型
K0IIIK 型(橙)
色指数 B−V
0.94
光度
50.7太阳 = 1
赤经(J2000)
17h 57m 45.9s
赤纬(J2000)
+29° 14′ 52″
所在星座
武仙座
视向速度
-2.0 km/s
自行
赤经 +82.3、赤纬 -18.7 毫角秒 / 年
中国古星名
中山增一
拜耳 / 弗兰斯蒂德名
武仙座 ξ
编号
HIP 87933 · HD 163993 · HR 6703

百科

武仙座ξ,又名BD+29 3156,HD 163993、SAO 85590、HR 6703,是武仙座的一颗恒星,视星等为3.7,位于银经54.91,银纬23.77,其B1900.0坐标为赤经17h 53m 52.7s,赤纬+29° 23.77′ 31″。

摘自中文维基百科「中山增一」,按 CC BY-SA 4.0 使用。

英文维基百科

中文条目比较短,这里附上内容更多的英文维基百科条目原文(未翻译)。

Xi Herculis is a solitary star located within the northern constellation of Hercules. The star is visible to the naked eye with an apparent visual magnitude of 3.70. Based upon an annual parallax shift of 23.85 mas as seen from Earth, it is located 137 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.05 due to interstellar dust. It is a suspected member of the Sirius stream of co-moving stars.

This is an evolved G-type giant star with a stellar classification of G8 III. It is a red clump star, which means it is on the horizontal branch and generating energy through the thermonuclear fusion of hydrogen at its core. The star is emitting X-rays with a luminosity of 3.03×10³⁰ erg s⁻¹ in the 0.3–10 keV band. It has twice the mass of the Sun but, at the age of two and a half billion years, it has expanded to 10 times the Sun's radius. The star is radiating 57 times the solar luminosity from its photosphere at an effective temperature of 5,032 K.

Xi Herculis was discovered to be a variable star when the Hipparcos data was analyzed. It is a semiregular variable star, oscillating in brightness by 3 hundredths of a magnitude, over a period of 120.8 days.

Chinese name

In R. H. Allen's book Star Names: Their Lore and Meaning, this star, together with ν Her and 99 Her (b Herculis) represent the state of Zhongshan (or Chung Shan, "the Middle Mountain"), but in Chinese literature, that name is applied to ο Her.

Markov 1, the mini teapot

One third of a degree to the north-northwest of Xi Herculis is the location of a telescopic asterism in the shape of a teapot. This teapot (Markov 1) could be seen as a somewhat twisted small equivalent of the large and easy to recognize teapot asterism in the constellation Sagittarius.

以上取自英文维基百科「Xi Herculis」(英文原文,未翻译),按 CC BY-SA 4.0 使用。

资料卡

类型
恒星、后发座FK型变星、near-infrared source、ultraviolet source
质量
2.01太阳 = 1
半径
10太阳 = 1
年龄
24.8 亿年

数据来自 Wikidata(CC0),数值已换算成常用单位。

武仙座里的其他亮星

整个星座 ›
名称星座星等距离光谱
天市右垣一武仙座 β武仙座2.78139 光年G8III
帝座武仙座 α¹武仙座2.78360 光年M5IIvar
天纪二武仙座 ζ武仙座2.8135 光年F9IV
天市左垣一武仙座 δ武仙座3.1275.1 光年A3IVv SB
女床一武仙座 π武仙座3.16377 光年K3IIvar
天市左垣三武仙座 μ武仙座3.4227.1 光年G5IV
天纪增一武仙座 η武仙座3.48109 光年G8III-IV
天市右垣二武仙座 γ武仙座3.74193 光年A9III
天棓五武仙座 ι武仙座3.82455 光年B3V SB
天市左垣四武仙座 ο武仙座3.84338 光年B9.5V
屠肆一武仙座 109武仙座3.85119 光年K2III
天纪九武仙座 θ武仙座3.86753 光年K1IIvar