HD 29587
Stern HD 29587 |
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AladinLite | |||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | Perseus | ||||||||||||
Right ascension | 04 h 41 m 36.32 s | ||||||||||||
declination | + 42 ° 07 ′ 6.5 ″ | ||||||||||||
Apparent brightness | 7.29 likes | ||||||||||||
Typing | |||||||||||||
Spectral class | G2 V | ||||||||||||
Astrometry | |||||||||||||
Radial velocity | (112.4 ± 0.1) km / s | ||||||||||||
parallax | (36.27 ± 0.87) mas | ||||||||||||
distance | (90 ± 2) ly (27.6 ± 0.7) pc |
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Visual absolute brightness M vis | +5.09 mag | ||||||||||||
Proper movement | |||||||||||||
Rec. Share: | (533.56 ± 0.99) mas / a | ||||||||||||
Dec. portion: | (−415.53 ± 0.91) mas / a | ||||||||||||
Physical Properties | |||||||||||||
radius | 0.9 R ☉ | ||||||||||||
Effective temperature | 5860 K | ||||||||||||
Other names and catalog entries |
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HD 29587 is a main sequence star of the spectral class G2 in the constellation Perseus, about 90 light years away from Earth . With an apparent magnitude of 7.29 mag, it can no longer be seen with the naked eye, even under optimal observation conditions. The central star is orbited by a spectroscopic companion with the systematic designation HD 29587 B , which could be a cool star or a brown dwarf.
Spectroscopic companion
The companion HD 29587 B , discovered through fluctuations in the radial speed of the central star, has an orbital period of about 1500 days; the eccentricity of the orbit is estimated to be 0.36 ± 0.10. The mass of the object was determined to be about 0.039 solar masses .
Sources and individual references
- ↑ a b c Hipparcos catalog (ESA 1997)
- ↑ Pulkovo radial velocities for 35493 HIP stars
- ↑ a b c Hipparcos, the New Reduction (van Leeuwen, 2007)
- ↑ Halbwachs et al .: Exploring the brown dwarf desert with Hipparcos ; in: Astronomy and Astrophysics, Vol. 355, pp. 581ff. (2000), bibcode : 2000A & A ... 355..581H