TOI-2267

TOI-2267
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus
Right ascension 04h 20m 12.64355s
Declination +84° 54′ 06.2765″
Apparent magnitude (V) 15.41
Characteristics
Evolutionary stage main sequence + main sequence
Spectral type M5V+M6V
Astrometry
Radial velocity (Rv)−19.0±0.3 km/s
Proper motion (μ) RA: +182.388 mas/yr
Dec.: −213.503 mas/yr
Parallax (π)44.3496±0.3556 mas
Distance73.5 ± 0.6 ly
(22.5 ± 0.2 pc)
Position (relative to A)
ComponentB
Epoch of observation9 December 2021
Angular distance0.384
Position angle279.7°
Projected separation8 AU
Details
A
Mass0.1710±0.0079 M
Radius0.2075±0.0225 R
Luminosity0.0033±0.0003 L
Surface gravity (log g)4.99±0.05 cgs
Temperature3030±100 K
Metallicity [Fe/H]0.164±0.11 dex
Rotation0.6958 days
Age≳1 Gyr
B
Mass0.0989±0.0130 M
Radius0.130±0.030 R
Luminosity0.0011±0.0003 L
Surface gravity (log g)5.28±0.18 cgs
Temperature2930±160 K
Metallicity [Fe/H]0.164±0.11 dex
Rotation0.4936 days
Age≳1 Gyr
Other designations
G 222-3, LP 4-80, LSPM J0420+8454, NLTT 12645, TOI-2267, TIC 459837008
Database references
SIMBADdata
Exoplanet Archivedata

TOI-2267 is a binary star located 73.5 light-years (22.5 parsecs) away from the Sun. The system has a visual apparent magnitude of 15.4, too faint to be seen with the naked eye. It consists of two red dwarfs that are separated by only 8 AU.