HD 210702
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pegasus | 
| Right ascension | 22h 11m 51.33s[1] | 
| Declination | +16° 02′ 26.0″[1] | 
| Apparent magnitude (V) | 5.939 | 
| Characteristics | |
| Spectral type | K1IV | 
| U−B color index | 0.73 | 
| B−V color index | 0.951[2] | 
| R−I color index | 0.49 | 
| Astrometry | |
| Radial velocity (Rv) | 10.9 ± 2 km/s | 
| Proper motion (μ) | RA: -3.15 ± 0.34[1] mas/yr Dec.: -18.02 ± 0.33[1] mas/yr | 
| Parallax (π) | 18.20 ± 0.39[1] mas | 
| Distance | 179 ± 4 ly (55 ± 1 pc) | 
| Absolute magnitude (MV) | 2.201 | 
| Details | |
| Mass | 1.68 (1.50–1.84)[2] M☉ | 
| Radius | 5.1 (4.8–5.5)[2] R☉ | 
| Luminosity | 14.1[2] L☉ | 
| Surface gravity (log g) | 3.19 ± 0.08[2] cgs | 
| Temperature | 4967 ± 25[2] K | 
| Metallicity | 12 ± 4 % | 
| Age | 1.4 ± 1 G years | 
| Other designations | |
| Database references | |
| SIMBAD | data | 
| Extrasolar Planets Encyclopaedia | data | 
| Data sources: | |
| Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) | |
HD 210702 is an orange subgiant star located approximately 179 light-years away in the constellation of Pegasus. With a mass of 1.8 times that of the Sun, the star spent its main-sequence life as an A-type star. The visual luminosity is 11.38 times that of the Sun and it is 182.4 light years away. The magnitude is near the naked-eye limit, but binoculars can easily see it.
The star shows variability in its radial velocity consistent with a planet-mass companion in a Keplerian orbit,[3] and one was duly discovered in April 2007, from observations at Lick and Keck Observatories in Mount Hamilton (California) and Mauna Kea (Hawai'i), USA.
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius | 
|---|---|---|---|---|---|---|
| b | >1.9 MJ | 1.2 | 354.8 ± 1.1 | 0.094 ± 0.052 | — | — | 
See also
References
- 1 2 3 4 5 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 7 Bun'ei Sato; et al. (2012). "Substellar Companions to Seven Evolved Intermediate-Mass Stars". PASJ. arXiv:1207.3141. Bibcode:2012PASJ...64..135S. doi:10.1093/pasj/64.6.135.
- ↑ Johnson, John Asher; et al. (2007). "Retired A Stars and Their Companions: Exoplanets Orbiting Three Intermediate-Mass Subgiants". The Astrophysical Journal 665 (1): 785–793. arXiv:0704.2455. Bibcode:2007ApJ...665..785J. doi:10.1086/519677.
Coordinates:  22h 11m 51.3311s, +16° 02′ 25.983″
 22h 11m 51.3311s, +16° 02′ 25.983″
| 
 | ||||||||||||||||||||||||||||||||||
This article is issued from Wikipedia - version of the Tuesday, May 05, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.