LHS 1478

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LHS 1478
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia[1]
Right ascension 02h 57m 18.25955s[2]
Declination +76° 33 11.2535[2]
Apparent magnitude (V) 13.3[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type M3V[5]
Astrometry
Radial velocity (Rv)+69.79±0.27[2] km/s
Proper motion (μ) RA: +690.920 mas/yr[2]
Dec.: −399.894 mas/yr[2]
Parallax (π)54.9036±0.0177 mas[2]
Distance59.41 ± 0.02 ly
(18.214 ± 0.006 pc)
Absolute magnitude (MV)+12.1[4]
Details[5]
Mass0.236±0.012 M
Radius0.246±0.008 R
Luminosity0.00715±0.00012 L
Surface gravity (log g)4.87±0.06 cgs
Temperature3381±54 K
Metallicity [Fe/H]−0.13±0.19 dex
Rotation~6.4 d
Rotational velocity (v sin i)<2 km/s
Other designations
G 245-61, LHS 1478, LP 14-53, NLTT 9256, TOI-1640, TIC 396562848[6]
Database references
SIMBADdata
Exoplanet Archivedata

LHS 1478 (also known as TOI-1640) is a M3V-type main sequence star located 59.4 light-years from Earth in the constellation of Cassiopeia.[7] It has a mass of 0.24 solar masses and a radius of 0.25 solar radii. It has an effective temperature of 3381 Kelvin. The star is fairly inactive with no major flaring activity.[5][8]

References

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