Epsilon Corvi
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Epsilon Corvi (ε Crv, ε Corvi) is a star in the southern constellation of Corvus. It has the traditional name Minkar Template:IPAc-en, from Arabic منقار minqar meaning "beak [of the crow]"[9] The apparent visual magnitude is +3.0[2] and it is located at a distance of Template:Convert from Earth.[1]
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Chariot (asterism), refers to an asterism consisting of ε Corvi, γ Corvi, δ Corvi and β Corvi.[10] Consequently, ε Corvi itself is known as Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.).[11]
Epsilon Corvi is a red giant with a stellar classification of K2 III, having consumed the hydrogen at its core and evolved away from the main sequence. It has about three times the Sun's mass, while having expanded to 57 times the Sun's radius. The photosphere irradiates 930 times more energy than the Sun and has an effective temperature of Template:Val,[6] giving it an orange hue that is characteristic of a K-type star.[12] It spent much of its life as a main sequence star of spectral type B5V.[13]
References
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- ↑ Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
- ↑ Template:In lang 香港太空館 - 研究資源 - 亮星中英對照表 Template:Webarchive, Hong Kong Space Museum. Accessed on line November 23, 2010.
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