HIP 5158

HIP 5158 is a star with a pair of orbiting substellar companions, located in the equatorial constellation of Cetus, the whale. It has the older designation CD-23 395, which is derived from the Cordoba Durchmusterung catalogue of southern stars. Based on parallax measurements, it is located 169 light years from the Sun. It has an absolute magnitude of 7.11, but at that distance the star has an apparent visual magnitude of 10.16, which is too dim to be visible to the naked eye. The system is receding with a radial velocity of 15.3 km/s, and it has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.205·yr−1.

HIP 5158
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus
Right ascension 01h 06m 02.050s
Declination –22° 27 11.35
Apparent magnitude (V) 10.16
Characteristics
Spectral type K5V
Apparent magnitude (B) 11.238
B−V color index 1.078±0.001
Astrometry
Radial velocity (Rv)15.28±0.23 km/s
Proper motion (μ) RA: 203.818±0.025 mas/yr
Dec.: −106.926±0.032 mas/yr
Parallax (π)19.3199 ± 0.0198 mas
Distance168.8 ± 0.2 ly
(51.76 ± 0.05 pc)
Absolute magnitude (MV)7.11
Details
Mass0.75±0.01 M
Radius0.69±0.02 R
Luminosity0.19±0.01 L
Surface gravity (log g)4.63±0.02 cgs
Temperature4,571±14 K
Metallicity [Fe/H]0.10±0.07 dex
Rotation42.3 days
Age4.5±3.2 Gyr
Other designations
CD–23°395, HIP 5158, SAO 166798, PPM 243575, LTT 617, NLTT 3632, 2MASS J01060202-2227111
Database references
SIMBADdata
Exoplanet Archivedata

The spectrum of HIP 5158 matches an ordinary K-type main-sequence star, an orange dwarf, with a stellar classification of K5V. The age of this star is poorly constrained, but it appears to be comparable to the Sun. It is spinning slowly with a rotation period of around 42.3 days. Based on the abundance of iron, this star appears metal rich, having concentration of heavy elements equal to 125% of solar abundance. It has 75% of the mass of the Sun and 60% of the Sun's radius. The star is radiating just 19% of the luminosity of the Sun from its photosphere at an effective temperature of 4,571 K.

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