Observation data Epoch J2000.0 Equinox (celestial coordinates) | |
---|---|
Constellation | Equuleus |
Right ascension | 21h 10m 31.31996s[1] |
Declination | 10° 02′ 56.1180″[1] |
Apparent magnitude (V) | 6.07[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | A2 Vs[3] (A1 Si Sr Cr)[4] |
U−B color index | +0.04[2] |
B−V color index | +0.02[2] |
Astrometry | |
Radial velocity (Rv) | +6.9[5] km/s |
Proper motion (μ) | RA: –2.696[1] mas/yr Dec.: +15.802[1] mas/yr |
Parallax (π) | 8.5862 ± 0.1086[1] mas |
Distance | 380 ± 5 ly (116 ± 1 pc) |
Absolute magnitude (MV) | +0.236[6] |
Details | |
Mass | 2.59±0.14[3] M☉ |
Radius | 1.7[7] R☉ |
Luminosity | 70.6+19.4 −15.2[3] L☉ |
Temperature | 9,078+169 −165[3] K |
Rotational velocity (v sin i) | 65[3] km/s |
Age | 970[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
6 Equulei is a probable (95% chance) astrometric binary[9] star system in the northern constellation of Equuleus, located 380 light years from the Sun. It is barely visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 6.07.[2] The system is moving further away from the Earth with a heliocentric radial velocity of +6.9 km/s.[5] It forms a wide optical double with γ Equulei, at an angular separation of 336 arcseconds in 2011.[10]
The visible component is an Ap star[3] with a stellar classification of A2Vs,[3] matching the evolutionary state of an A-type main sequence star while displaying "sharp" absorption lines. It is an estimated 970[6] million years old with a projected rotational velocity of 65 km/s.[3] The star has 2.6[3] times the mass of the Sun and around 1.7[7] times the Sun's radius. It is radiating 71[3] times the luminosity of the Sun from its photosphere at an effective temperature of 9,078 K.[3]
Original source: https://en.wikipedia.org/wiki/6 Equulei.
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