HD 16175 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 16175 | |
Constellation | Andromeda | |
Right ascension | (α) | 02h 37m 01.9111s[1] |
Declination | (δ) | +42° 03′ 45.468″[1] |
Apparent magnitude | (mV) | 7.28 |
Distance | ±3 190[1] ly (±0.9 58.3[1] pc) | |
Spectral type | G0 | |
Orbital elements | ||
Semi-major axis | (a) | ±0.076 2.148[2] AU |
Eccentricity | (e) | ±0.020 0.637[2] |
Orbital period | (P) | ±2.8 995.4[2] d |
Argument of periastron |
(ω) | ±2.2 221.5[2]° |
Time of periastron | (T0) | 455801.4±2.6 2[2] JD |
Semi-amplitude | (K) | ±2.5 51.75[2] m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | ±0.37 4.77[2] MJ |
Discovery information | ||
Discovery date | ||
Discoverer(s) | Peek "et al." | |
Discovery method | radial velocity | |
Discovery site | Lick Observatory | |
Discovery status | Published[3] | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 16175 b is an extrasolar planet located approximately 190 light-years away in the constellation of Andromeda, orbiting the star HD 16175. This planet masses 4.8 times that of Jupiter. However, the mass is only a minimum since the inclination of the orbit is not known. This planet orbits at about 2.2 astronomical units, taking 2.73 years to revolve around the star. The orbit of the planet is highly noncircular with an eccentricity at 0.64.[2]
Discovery
The discovery was made using radial velocity measurements taken between November 2004 and March 2009 with the Coudé Auxiliary and C. Donald Shane telescopes at Lick Observatory.[3]
See also
References
- 1 2 3 4 Brown, A. G. A; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics. 595. A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512. Gaia Data Release 1 catalog entry
- 1 2 3 4 5 6 7 8 Díaz, R. F.; et al. (2016). "The SOPHIE search for northern extrasolar planets. XI. Three new companions and an orbit update: Giant planets in the habitable zone". Astronomy and Astrophysics. 591. A146. arXiv:1604.07610. Bibcode:2016A&A...591A.146D. doi:10.1051/0004-6361/201628331.
- 1 2 Peek, John Asher; et al. (2009). "Old, rich, and eccentric: two jovian planets orbiting evolved metal-rich stars". Publications of the Astronomical Society of the Pacific. 121 (880): 613–620. arXiv:0904.2786. Bibcode:2009PASP..121..613P. doi:10.1086/599862.
External links
- "HD 16175". Exoplanets. Retrieved 2008-08-24.
Coordinates:
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