Gamma Capricorni
Gamma Capricorni or γ Capricorni, formally named Nashira (/ˈnæʃɪrə/), is a giant star in the constellation of Capricornus. Based on parallax measurements obtained during the Hipparcos mission, it is located at a distance of approximately 157 light-years from the Sun. The star is drifting closer with a radial velocity of −31 km/s. It is 2.56 degrees south of the ecliptic, so it can be occulted by the Moon, and (rarely) by planets.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Capricornus |
Right ascension | 21h 40m 05.45648s |
Declination | −16° 39′ 44.307184″ |
Apparent magnitude (V) | +3.67 |
Characteristics | |
Spectral type | kF0hF1VmF2 |
U−B color index | +0.22 |
B−V color index | +0.32 |
Variable type | α2 CVn |
Astrometry | |
Radial velocity (Rv) | −31.2±0.5 km/s |
Proper motion (μ) | RA: +187.56 mas/yr Dec.: −22.45 mas/yr |
Parallax (π) | 20.77 ± 0.72 mas |
Distance | 157 ± 5 ly (48 ± 2 pc) |
Absolute magnitude (MV) | +2.60 |
Details | |
Mass | 2.44 M☉ |
Radius | 2.35 R☉ |
Surface gravity (log g) | 3.69 cgs |
Temperature | 7,520 K |
Metallicity [Fe/H] | +0.5 dex |
Rotational velocity (v sin i) | 40 km/s |
Other designations | |
Nashira, Gamma Cap, Gam Cap, γ Cap, 40 Capricorni, BD−17°6340, FK5 812, GJ 4209, HD 206088, HIP 106985, HR 8278, SAO 164560 | |
Database references | |
SIMBAD | data |
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