HD 32518 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 32518 | |
Constellation | Camelopardalis | |
Right ascension | (α) | 05h 09m 36.72s[1] |
Declination | (δ) | +69° 38′ 21.9″[1] |
Apparent magnitude | (mV) | 6.436 |
Distance | 390 ± 30[1] ly (121 ± 8[1] pc) | |
Spectral type | K1III | |
Orbital elements | ||
Semi-major axis | (a) | 0.59 ± 0.03 AU |
Periastron | (q) | 0.58 AU |
Apastron | (Q) | 0.60 AU |
Eccentricity | (e) | 0.01 ± 0.03 |
Orbital period | (P) | 157.54 ± 0.38 d (0.4313 ± 0.001 y) |
Argument of periastron |
(ω) | 306.11 ± 126.71° |
Time of periastron | (T0) | 2452950.29 ± 13.66 JD |
Physical characteristics | ||
Minimum mass | (m sin i) | 3.04 ± 0.69 MJ |
Discovery information | ||
Discovery date | August 12, 2009 | |
Discoverer(s) | Döllinger et al. | |
Discovery method | Radial velocity | |
Discovery site | TLS | |
Discovery status | Published | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 32518 b is an extrasolar planet which orbits the K-type giant star HD 32518, located approximately 383 light years away in the constellation Camelopardalis. It has a minimum mass three times greater than Jupiter and orbits the intermediate-mass giant star at a distance of only 0.59 AU in a very circular orbit. The orbit takes 10.35 months to complete one round trip around the star.[2] This planet was detected by the radial velocity method on August 12, 2009.
References
- 1 2 3 4 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
- ↑ Döllinger, P.; et al. (2009). "Planetary companions around the K giant stars 11 Ursae Minoris and HD 32518". Astronomy and Astrophysics. 505 (3): 1311–1317. arXiv:0908.1753. Bibcode:2009A&A...505.1311D. doi:10.1051/0004-6361/200911702.
Coordinates: 05h 09m 36.7193s, +69° 38′ 21.844″
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