HD 171028

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HD 171028
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ophiuchus
Right ascension 18h 32m 15.4933s[1]
Declination 06° 56′ 44.6858″[1]
Apparent magnitude (V) 8.301[2]
Characteristics
Spectral type G0[3]
B−V color index 0.61[3]
Distance
365 ± 2 ly
(112.0 ± 0.6 pc)
Details
Gyr
TYC 458-1450-1, 2MASS J18321548+0656446[5]
Database references
SIMBADdata

HD 171028 is a

light years from the Sun based on parallax, and is drifting further away with a radial velocity of +13.5 km/s.[1]

This is a yellow-hued

projected rotational velocity of 2.3 km/s.[3] It has the same mass as the Sun, but the radius is 2.4 times larger. The star is radiating 5.4[1] times the luminosity of the Sun from its photosphere at an effective temperature of 5,671 K.[2]

In the summer of 2007, a Jovian planetary companion was discovered by the

radial velocity method.[3] This object is orbiting at a distance of 1.32 AU from the host star with a period of 1.5 years and an eccentricity (ovalness) of 0.59. Since the inclination of the orbit is unknown, only a minimum mass can be determined. This planet has at least double the mass of Jupiter.[7]

The HD 171028 planetary system[7]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥1.98 MJ 1.32 550±3 0.59±0.01

See also

  • List of extrasolar planets

References