HD 29587
![]() An artistic concept of brown dwarf HD 29587 B.  | |
|  Observation data Epoch J2000.0 Equinox J2000.0  | |
|---|---|
| Constellation | Perseus | 
| Right ascension | 04h 41m 36.3177s | 
| Declination | +42° 07′ 06.493″ | 
| Apparent magnitude (V) | 7.29 | 
| Characteristics | |
| Spectral type | G0V | 
| Variable type | none | 
| Details | |
| Mass | 1.09 M☉ | 
| Radius | 0.88 R☉ | 
| Luminosity | 0.811 L☉ | 
| Temperature | 5840 K | 
| Other designations | |
 HIP 21832, TYC 2901-00064-1, HD 29587, BD+41 931, SAO 39690, 2MASS J04413631+4207065   | |
| Database references | |
| SIMBAD | data | 
| Exoplanet Archive | data | 
| Extrasolar Planets Encyclopaedia  | data | 
HD 29587 is a Sun-like star located approximately 93 light-years away in the constellation of Perseus. The star is known to host a brown dwarf companion.[1]
|  Companion (in order from star)  | 
Mass |  Semimajor axis (AU)  | 
 Orbital period (days)  | 
Eccentricity | Inclination | Radius[1] | 
|---|---|---|---|---|---|---|
| b | ≥55 MJ | 2.54 | 1481 | 0.33 | — | — | 
References
- 1 2 Mazeh; Latham, David W.; Stefanik, Robert P. (1996). "Spectroscopic Orbits for Three Binaries with Low-Mass Companions and the Distribution of Secondary Masses near the Substellar Limit". Astrophysical Journal 466: 415–427. Bibcode:1996ApJ...466..415M. doi:10.1086/177521.
 
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