HD 106515

HD 106515 is a binary star (and currently visual triple system) in the constellation of Virgo.

HD 106515
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Virgo
HD 106515 A
Right ascension 12h 15m 06.5667s
Declination –07° 15 26.353
Apparent magnitude (V) +7.99
HD 106515 B
Right ascension 12h 15m 06.1003s
Declination –07° 15 26.587
Apparent magnitude (V) +8.25
Characteristics
HD 106515 A
Spectral type K0 V
HD 106515 B
Spectral type K1 V
Astrometry
HD 106515 A
Radial velocity (Rv)20.66±0.11 km/s
Proper motion (μ) RA: −251.469 mas/yr
Dec.: −51.330 mas/yr
Parallax (π)29.3148 ± 0.0297 mas
Distance111.3 ± 0.1 ly
(34.11 ± 0.03 pc)
HD 106515 B
Radial velocity (Rv)19.94±0.11 km/s
Proper motion (μ) RA: −244.603 mas/yr
Dec.: −67.744 mas/yr
Parallax (π)29.3908 ± 0.0294 mas
Distance111.0 ± 0.1 ly
(34.02 ± 0.03 pc)
Absolute magnitude (MV)4.62
Orbit
PrimaryHD 106515 A
CompanionHD 106515 B
Period (P)4802.1+2397
−1141
yr
Semi-major axis (a)9.822+2.688
−1.329
"
(345+95
−47
 AU
)
Eccentricity (e)0.420+0.106
−0.104
Inclination (i)164.45+3.5
−11.3
°
Longitude of the node (Ω)92.06+45.08
−2.67
°
Periastron epoch (T)2376.4+44.4
−78.9
Argument of periastron (ω)
(secondary)
250.50+38.22
−14.07
°
Details
HD 106515 A
Mass0.888±0.018 M
Radius0.910±0.009 R
Luminosity0.68±0.05 L
Surface gravity (log g)4.39±0.18 cgs
Temperature5364±57 K
Metallicity [Fe/H]+0.016±0.009 dex
Rotational velocity (v sin i)1.7 km/s
Age9.233±2.133 Gyr
HD 106515 B
Mass0.861±0.015 M
Radius0.865±0.015 R
Luminosity0.55±0.05 L
Surface gravity (log g)4.30±0.20 cgs
Temperature5190±58 K
Metallicity [Fe/H]+0.022±0.010 dex
Rotational velocity (v sin i)1.8 km/s
Age9.155±2.199 Gyr
Other designations
BD−06°3532, HIP 59743, ADS 8477 AB, WDS J12151-0715AB
HD 106515 A: Gaia DR2 3584074380866605440, SAO 138673, LTT 4599, 2MASS J12150658-0715263
HD 106515 B: Gaia DR2 3584074376569429248, SAO 138674, LTT 4598, 2MASS J12150611-0715265
Database references
SIMBADdata
Exoplanet Archivedata

The A and B stars are both K-type main-sequence stars, both somewhat smaller and cooler than the Sun. The two are gravitationally bound and separated at 310 AU. The binary semimajor axis is 390 AU.

The third star in the visual triple, BD−06°3533, is a physically unrelated background star.

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