BX Trianguli

BX Trianguli

Artist's impression of BX Trianguli. The planet is not represented here.
Observation data
Epoch J2000      Equinox J2000
Constellation Triangulum
Right ascension 02h 20m 50.85419s
Declination +33° 20 47.4683
Apparent magnitude (V) 13.366±0.006
Characteristics
Evolutionary stage Red dwarf
Spectral type M2
Variable type Eclipsing binary + Flare star
Astrometry
Proper motion (μ) RA: +144.250 mas/yr
Dec.: –111.210 mas/yr
Parallax (π)18.9896±0.0259 mas
Distance171.8 ± 0.2 ly
(52.66 ± 0.07 pc)
Orbit
PrimaryA
CompanionB
Period (P)0.1926 days (4.62 hours)
Semi-major axis (a)1.33±0.03 R
Inclination (i)66.89±0.45°
Details
A
Mass0.578±0.04 M
Radius0.59±0.01 R
Luminosity0.053 L
Temperature3,735 K
B
Mass0.28±0.02 M
Radius0.27±0.01 R
Luminosity0.007 L
Temperature3,359±28 K
Other designations
BX Tri, LSPM J0220+3320, GSC 02314-00530, 2MASS J02205082+3320479, NSVS 6550671
Database references
SIMBADdata

BX Trianguli is a binary system made up of two red dwarfs, in the constellation Triangulum. Both stars eclipse each other and have an orbital period of four hours and 40 minutes. They are located at around 170 light-years from Earth based upon parallax measurements.