HD 27894

HD 27894 is a single star with a system of orbiting exoplanets, located in the southern constellation of Reticulum. It is too faint to be seen with the naked eye at an apparent visual magnitude of 9.36. This system lies at a distance of 142.5 light years from the Sun, as determined via parallax measurements, and is drifting further away with a radial velocity of 83 km/s.

HD 27894
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Reticulum
Right ascension 04h 20m 47.046s
Declination −59° 24 39.02
Apparent magnitude (V) 9.36
Characteristics
Spectral type K2 V
U−B color index +0.90
B−V color index +1.003±0.002
Astrometry
Radial velocity (Rv)82.785±0.0008 km/s
Proper motion (μ) RA: 182.473±0.012 mas/yr
Dec.: 270.012±0.017 mas/yr
Parallax (π)22.8888 ± 0.0121 mas
Distance142.50 ± 0.08 ly
(43.69 ± 0.02 pc)
Absolute magnitude (MV)6.225
Details
Mass0.83±0.03 M
Radius0.79±0.02 R
Luminosity0.33±0.01 L
Surface gravity (log g)4.56±0.03 cgs
Temperature4,923±32 K
Metallicity [Fe/H]+0.30±0.07 dex
Rotation44 days
Rotational velocity (v sin i) 1.5 km/s
Age7.7±2.3 Gyr
Other designations
CD−59° 829, HD 27894, HIP 20277, LTT 1953
Database references
SIMBADdata

The spectrum of HD 27894 presents as a K-type main-sequence star, an orange dwarf, with a stellar classification of K2 V. This is a quiescent solar-type star that displays no significant magnetic activity in its chromosphere and is spinning slowly with a rotation period of roughly 44 days. The abundance of iron in the star is much higher than in the Sun, an indicator that it is metal-rich. It has 83% of the mass of the Sun and 79% of the Sun's radius. The star is radiating 33% of the luminosity of the Sun from its photosphere at an effective temperature of 4,923 K.

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