2 Equulei

2 Equulei
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Equuleus
A
Right ascension 21h 02m 12.50262s
Declination +07° 10 47.1545
Apparent magnitude (V) 7.41
B
Right ascension 21h 02m 12.39375s
Declination +07° 10 44.7957
Apparent magnitude (V) 7.64
Characteristics
A
Evolutionary stage subgiant
Spectral type F6V
B
Evolutionary stage subgiant
Spectral type F3V
Astrometry
Radial velocity (Rv)−4.8±1.6 km/s
Absolute magnitude (MV)2.16±0.18
A
Proper motion (μ) RA: −9.184 mas/yr
Dec.: −12.915 mas/yr
Parallax (π)8.8125±0.2481 mas
Distance370 ± 10 ly
(113 ± 3 pc)
B
Proper motion (μ) RA: −4.238 mas/yr
Dec.: −17.934 mas/yr
Parallax (π)8.5577 ± 0.0298 mas
Distance381 ± 1 ly
(116.9 ± 0.4 pc)
Details
2 Equ A
Mass1.73 M
Radius2.6 R
Luminosity12.9 L
Surface gravity (log g)3.84 cgs
Temperature6,127 K
Metallicity [Fe/H]0.17 dex
Age1.9 Gyr
2 Equ B
Mass1.61 M
Radius2.8 R
Luminosity10.9 L
Surface gravity (log g)3.72 cgs
Temperature6,420 K
Age2.2 Gyr
Other designations
λ Equ, 2 Equulei, BD+06°4731, HD 200256, HIP 103813, LTT 16227, SAO 126482
Database references
SIMBADdata

2 Equulei is a double star system in the constellation of Equuleus.

The primary component of the 2 Equulei pair is an F-type star. As of 2015, the secondary had an angular separation of 2.90 arc seconds along a position angle of 213° from the primary. They form a common proper motion pair, two stars at approximately the same distance and moving in the same direction. Gaia DR3 gives them parallaxes of 8.8125±0.2471 mas and 8.5577±0.0298 mas respectively, although they are flagged as potentially unreliable. These parallaxes correspond to a distance of around 380 ly, in contrast to the Hipparcos distance of 260±20 ly for the two stars as a pair.

2 Equulei has been referred to in some sources as λ (Lambda) Equulei, although it was not given that designation by Bayer.