LHS 1678

LHS 1678
Observation data
Epoch J2000      Equinox J2000
Constellation Caelum
Right ascension 04h 32m 42.635s
Declination −39° 47 12.15
Apparent magnitude (V) 12.482
Characteristics
A
Evolutionary stage Red dwarf
Spectral type M2V
Apparent magnitude (B) 13.5
Apparent magnitude (R) 11.533
Apparent magnitude (G) 9.02
Apparent magnitude (H) 8.501
Apparent magnitude (K) 8.264
B−V color index 1.018
B
Evolutionary stage Possible brown dwarf, maybe a jovian planet
Astrometry
Radial velocity (Rv)10.94±0.28 km/s
Total velocity94.6±0.4 km/s
Proper motion (μ) RA: +239.368 mas/yr
Dec.: −967.597 mas/yr
Parallax (π)50.34±0.02 mas
Distance64.79 ± 0.03 ly
(19.865 ± 0.008 pc)
Orbit
PrimaryA
CompanionB
Period (P)42 or 100 years
Semi-major axis (a)17 or 100 mas
(36 or 210 AU)
Details
A
Mass0.345±0.014 M
Radius0.329±0.01 R
Luminosity0.0145±0.0003 L
Temperature3490±50 K
Metallicity [Fe/H]−0.36±0.06 dex
Rotation66±22 d
Age4.22±0.87 or 4–9 Gyr
Other designations
TOI-696, Gaia DR2 4864160624337973248, Gaia DR3 4864160624337973248, LHS 1678, LTT 2022, TIC 77156829, 2MASS J04324261-3947112, WISEA J043242.84-394722.1
Database references
SIMBADdata

LHS 1678 (TOI-696) is an astrometric binary star system, located about 65 light-years from the Earth in the constellation Caelum. It is made up of a red dwarf and a companion star whose nature is still uncertain, but is likely to be a brown dwarf. The red dwarf star is known to host three small, close-in exoplanets. The apparent magnitude of LHS 1678 is 12.5, which is too dim to be seen with the naked eye or a small telescope.