HD 169830

HD 169830 is a star in the southern constellation of Sagittarius. It has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.90. The star is located at a distance of 120 light years from the Sun based on parallax. It is drifting closer with a radial velocity of −17.3 km/s, and is predicted to come as close as 20.7 ly (6.4 pc) in 2.08 million years. HD 169830 is known to be orbited by two large Jupiter-like exoplanets.

HD 169830
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 18h 27m 49.48500s
Declination –29° 49 00.7008
Apparent magnitude (V) +5.90
Characteristics
Spectral type F7V
B−V color index 0.517±0.004
Variable type “None”
Astrometry
Radial velocity (Rv)−17.271±0.0004 km/s
Proper motion (μ) RA: −0.341 mas/yr
Dec.: 16.103 mas/yr
Parallax (π)27.1461 ± 0.1469 mas
Distance120.1 ± 0.7 ly
(36.8 ± 0.2 pc)
Absolute magnitude (MV)+3.08
Details
Mass1.4 M
Radius1.84 R
Luminosity4.63 L
Surface gravity (log g)4.06 cgs
Temperature6,300±50 K
Metallicity [Fe/H]0.15 dex
Rotation8.3 d
Rotational velocity (v sin i)3.83 km/s
Age4.95 Gyr
Other designations
CD−29°14965, Gaia DR2 4048037707717866880, GC 25175, HD 169830, HIP 90485, HR 6907, SAO 186838, GSC 06869-01277, 2MASS J18274949-2949007
Database references
SIMBADdata
ARICNSdata

This is an F-type main-sequence star with a stellar classification of F7V. It is 3.83 billion years old and chromospherically inactive with a slow rotation rate, having a projected rotational velocity of 3.83 km/s. This star is 40% more massive and 84% larger than the Sun. Combining the mass and radius makes the surface gravity only 41% that of the Sun. It is radiating 4.6 times the luminosity of the Sun from its photosphere at an effective temperature of 6,300 K.

A candidate stellar companion, designated component B, lies at an angular separation of 11 along a position angle of 265°.

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