HIP 14810
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aries |
| Right ascension | 03h 11m 14.23s[1] |
| Declination | +21° 05′ 50.5″[1] |
| Apparent magnitude (V) | 8.53 |
| Characteristics | |
| Spectral type | G5V |
| B−V color index | 0.777 |
| Astrometry | |
| Proper motion (μ) | RA: -3.66 ± 1.81[1] mas/yr Dec.: -53.44 ± 1.10[1] mas/yr |
| Parallax (π) | 18.71 ± 1.26[1] mas |
| Distance | 170 ± 10 ly (53 ± 4 pc) |
| Absolute magnitude (MV) | 4.91 |
| Details | |
| Mass | 0.98 ± 0.02[2] M☉ |
| Radius | 1.08 ± 0.03[2] R☉ |
| Luminosity | 0.99 ± 0.01[2] L☉ |
| Surface gravity (log g) | 4.35 ± 0.03[2] cgs |
| Temperature | 5535 ± 51[2] K |
| Metallicity | 0.23 ± 0.3 |
| Age | 8.7 ± 2.0[2] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
| Extrasolar Planets Encyclopaedia | data |
| Data sources: | |
| Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) | |
HIP 14810 is a G-type main-sequence star located approximately 170 light-years away[1] in the constellation of Aries.
Planetary system
Orbiting the star are three confirmed planets. The discovery paper for HIP 14810 b and HIP 14810 c was published in 2007,[3] while that for HIP 14810 d was published in 2009, together with a revision for the orbital parameters for planet c.[4]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥3.88 ± 0.32 MJ | 0.0692 ± 0.0040 | 6.673855 ± 0.000019 | 0.14270 ± 0.00094 | — | — |
| c | ≥1.28 ± 0.10 MJ | 0.545 ± 0.031 | 147.730 ± 0.065 | 0.164 ± 0.012 | — | — |
| d | ≥0.570 ± 0.052 MJ | 1.89 ± 0.11 | 952 ± 15 | 0.173 ± 0.037 | — | — |
See also
References
- 1 2 3 4 5 6 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752
. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry - 1 2 3 4 5 6 Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575. A18. arXiv:1411.4302. Bibcode:2015A&A...575A..18B. doi:10.1051/0004-6361/201424951.
- ↑ Wright, J. T.; et al. (2007). "Four New Exoplanets and Hints of Additional Substellar Companions to Exoplanet Host Stars". The Astrophysical Journal. 657 (1): 533–545. arXiv:astro-ph/0611658. Bibcode:2007ApJ...657..533W. doi:10.1086/510553.
- 1 2 Wright, J. T.; et al. (2009). "A Third Giant Planet Orbiting HIP 14810". The Astrophysical Journal Letters. 699 (2): L97–L101. arXiv:0906.0567. Bibcode:2009ApJ...699L..97W. doi:10.1088/0004-637X/699/2/L97.
External links
- Extrasolar Planet Interactions by Rory Barnes & Richard Greenberg, Lunar and Planetary Lab, University of Arizona
- Image HIP 14810
Coordinates: 
03h 11m 14.2304s, +21° 05′ 50.491″
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