Eta Capricorni

Eta Capricorni
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Capricornus
Right ascension 21h 04m 24.30132s
Declination −19° 51 17.9711
Apparent magnitude (V) +4.84 (5.02 + 7.39)
Characteristics
Spectral type A4 V + F2 V
U−B color index +0.09
B−V color index +0.17
Astrometry
Proper motion (μ) RA: −37.62±0.90 mas/yr
Dec.: −24.95±0.88 mas/yr
Parallax (π)20.20±0.82 mas
Distance161 ± 7 ly
(50 ± 2 pc)
Absolute magnitude (MV)+1.35
Orbit
Period (P)27.85±0.15 yr
Semi-major axis (a)0.265±0.003
Eccentricity (e)0.410±0.005
Inclination (i)162.6±0.5°
Longitude of the node (Ω)171.1±15.0°
Periastron epoch (T)2002.46±0.09
Argument of periastron (ω)
(secondary)
238.2±15.0°
Details
η Cap A
Mass2.03±0.12 M
Luminosity24 L
Metallicity [Fe/H]−0.01 dex
η Cap B
Mass1.21±0.07 M
Other designations
η Cap, 22 Cap, BD−20°6115, HD 200499, HIP 104019, HR 8060, SAO 189986, WDS J21044-1951AB
Database references
SIMBADdata

Eta Capricorni, Latinized from η Capricorni, is a binary star system in the southern constellation of Capricornus. It can be seen with the naked eye, having a combined apparent visual magnitude of +4.84. Based upon an annual parallax shift of 20.20 mas as seen from the Earth, the star is located about 161 light years from the Sun.

The pair orbit each other with a period of 27.85 years, a semimajor axis of 0.265 arc seconds, an eccentricity of 0.410. The primary member, component A, is a white-hued A-type main sequence star with an apparent magnitude of +5.02. Its companion, component B, has an apparent magnitude of +7.39.