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[[es:Rho Capricorni]]
[[fa:رو بزغاله]]
[[fa:رو بزغاله]]
[[id:Rho Capricorni]]
[[id:Rho Capricorni]]

Revision as of 08:30, 28 September 2011

ρ Capricorni
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Capricornus
Right ascension 20h28m51.6s
Declination −17°48′49″
Apparent magnitude (V) +4.77
Distance98.7 ± 2.6 ly
(30.3 ± 0.8 pc)
Spectral typeF2IV
Other designations
11 Capricorni, HR 7822, HD 194943, Gl 791.1, BD−18°5689, HIP 101027, SAO 163614, GC 28481, ADS 13887, CCDM J20289-1750

Rho Capricorni (ρ Cap, ρ Capricorni) is a binary star in the constellation Capricornus. It is approximately 98.7 light years from Earth.

Sometimes, this star is called by the name Bos, meaning the cow in Latin[1].

In Chinese, 牛宿 (Niú Su), meaning Ox (asterism), refers to an asterism consisting of β Capricorni, α2 Capricorni, ξ2 Capricorni, π Capricorni, ο Capricorni and ρ Capricorni.[2] Consequently, β Capricorni itself is known as 牛宿六 (Niú Su liù, English: the Sixth Star of Ox.)[3]

The primary component, ρ Capricorni A, is a yellow-white F-type subgiant with an apparent magnitude of +4.77. Its companion, ρ Capricorni B is an eighth magnitude star located 1.013 arcseconds or at least 30 AU from the primary.

References