HD 5319 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 5319 | |
Constellation | Cetus | |
Right ascension | (α) | 00h 55m 01.40s[1] |
Declination | (δ) | +00° 47′ 22.4″[1] |
Apparent magnitude | (mV) | 8.05 |
Distance | 370 ± 40[1] ly (110 ± 10[1] pc) | |
Spectral type | K3IV[2] | |
Orbital elements | ||
Semi-major axis | (a) | 1.6697 ± 0.0036[2] AU |
Eccentricity | (e) | 0.02 ± 0.03[2] |
Orbital period | (P) | 641 ± 2[2] d |
Argument of periastron |
(ω) | 97 ± 90[2]° |
Time of periastron | (T0) | 2,456,288 ± 790[2] JD |
Semi-amplitude | (K) | 31.6 ± 1.2[2] m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | 1.76 ± 0.07[2] MJ |
Discovery information | ||
Discovery date | January 11, 2007 | |
Discoverer(s) | Robinson et al.[3] | |
Discovery method | Doppler spectroscopy | |
Discovery site | California & Carnegie Planet Search | |
Discovery status | Published[3] | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 5319 b is a gas giant exoplanet discovered in 2007[3] in the constellation of Cetus. This planet has a minimum mass nearly two times that of Jupiter. The planet has an almost circular orbit, with an eccentricity of only 0.02 and a period of 641 days. An additional planet in the system was discovered in 2015 and may be in a 4:3 mean motion resonance with planet b.[2]
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
- 1 2 3 4 5 6 7 8 9 Giguere, Matthew J.; et al. (2015). "Newly Discovered Planets Orbiting HD 5319, HD 11506, HD 75784 and HD 10442 from the N2K Consortium". The Astrophysical Journal. 799 (1). 89. arXiv:1411.5374. Bibcode:2015ApJ...799...89G. doi:10.1088/0004-637X/799/1/89.
- 1 2 3 Robinson, Sarah E.; et al. (2007). "Two Jovian-Mass Planets in Earthlike Orbits". The Astrophysical Journal. 670 (2): 1391–1400. arXiv:0708.0832. Bibcode:2007ApJ...670.1391R. doi:10.1086/522106.
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