Holmberg IX V1

Holmberg IX V1
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ursa Major
Right ascension 09h 57m 37.14s
Declination +69° 02′ 11.0″
Apparent magnitude (V) 20.7
Characteristics
A
Evolutionary stage Yellow supergiant
Spectral type G
B
Evolutionary stage Yellow supergiant
Spectral type G
Astrometry
Distance13 million ly
Absolute magnitude (MV)-7.1
Orbit
PrimaryHolmberg IX V1 A
NameHolmberg IX V1 B
Period (P)270.7 days
Semi-major axis (a)547 R
Eccentricity (e)0
Inclination (i)55.7°
Details
A
Mass15-20 M
Radius337 R
Luminosity54,450 L
Temperature4,800 K
Metallicity [Fe/H]-0.328 dex
Age10-15 Myr
B
Mass15-20 M
Radius306 R
Luminosity54,450 L
Temperature5,040 K
Metallicity [Fe/H]-0.328 dex
Age10-15 Myr
Other designations
EQ J095737+690211
Database references
SIMBADdata

Holmberg IX V1, also known as EQ J095737+690211 is a W Ursae Majoris type eclipsing contact binary star system in the constellation of Ursa Major. The binary system is located in the dwarf galaxy Holmberg IX, roughly 13 million light years (or 4 million parsecs) away. The binary system has a maximum visual magnitude of 20.7, and is one of most extreme and rarest systems discovered.