HD 16175
Star HD 16175 |
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AladinLite | |||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | Andromeda | ||||||||||
Right ascension | 02 h 37 m 1.91 s | ||||||||||
declination | + 42 ° 03 ′ 45.5 ″ | ||||||||||
Apparent brightness | 7.28 likes | ||||||||||
Typing | |||||||||||
Known exoplanets | 1 | ||||||||||
Spectral class | G0 | ||||||||||
Astrometry | |||||||||||
Radial velocity | (21.5 ± 0.4) km / s | ||||||||||
parallax | (17.28 ± 0.67) mas | ||||||||||
distance | (189 ± 7) ly (58 ± 2) pc |
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Visual absolute brightness M vis | +3.47 mag | ||||||||||
Proper movement | |||||||||||
Rec. Share: | (−38.90 ± 0.63) mas / a | ||||||||||
Dec. portion: | (−40.37 ± 0.53) mas / a | ||||||||||
Physical Properties | |||||||||||
Other names and catalog entries |
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HD 16175 is a sub-giant of the spectral class G0 in the constellation Andromeda, about 200 light years away . It has an apparent visual magnitude of 7.3 mag and is a foreground star to the open star cluster Messier 34 .
The star has a spectroscopic companion with the systematic name HD 16175 b and an orbital period of about 2.7 years. With a minimum mass of approx. 4.4 Jupiter masses, the companion could be an exoplanet or a brown dwarf . The eccentricity of the orbit is estimated to be 0.59 ± 0.11; with an estimated mass of 1.3 solar masses for the central star, the object has a major semi-axis of approx. 2.1 astronomical units .
Web links and individual references
- The exoplanet in the "Encyclopedia of Extrasolar Planets"