HD 114762 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 114762 | |
Constellation | Coma Berenices | |
Right ascension | (α) | 13h 12m 19.7427s |
Declination | (δ) | +17° 31′ 01.643″ |
Apparent magnitude | (mV) | 7.3 |
Distance | 132.4 ly (40.6 pc) | |
Spectral type | F9V | |
Orbital elements | ||
Semi-major axis | (a) | ±0.001 0.353[2] AU |
Eccentricity | (e) | ±0.0048 0.3354[2] |
Orbital period | (P) | ±0.0030 83.9151[2] d |
Argument of periastron |
(ω) | ±1.01 201.28[2]° |
Time of periastron | (T0) | 449889.106±0.186 2[2] JD |
Semi-amplitude | (K) | ±3.52 612.48[2] m/s |
Physical characteristics | ||
Minimum mass | (m sin i) | ±0.063 11.069[3] MJ |
Maximum mass | (m sin i) | 63.2[4] MJ |
Discovery information | ||
Discovery date | 1989 | |
Discoverer(s) | David Latham, et al. | |
Discovery method | Doppler spectroscopy | |
Discovery status | Confirmed | |
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 114762 b is a massive gaseous[5][6] extrasolar planet,[7] approximately 132 light-years (40.6 pc) away in the constellation of Coma Berenices.[1][5] This optically undetected companion to the late F-type main-sequence star HD 114762 was discovered in 1989 by Latham, et al.,[6] and confirmed in an October 1991 paper by Cochran, et al.[8]
The companion orbits its star every 83.9 days at an approximate distance of 0.35 AU, with an orbital eccentricity of 0.34;[2] for comparison, this orbit is similar to that of Mercury but with twice the eccentricity.[8] Depending on inclination angle, it has a minimum mass of ±0.063 11.069 MJ (at 90°)[3] and a maximum mass of approximately 63.2 MJ (at 10°).[4]
HD 114762 b may be the first extrasolar planet ever detected, predating the 1992 pulsar planets found around PSR B1257+12 and main-sequence yellow dwarf 51 Pegasi.[9][10] By 2012, its status as an exoplanet was confirmed.[4][7] At an event celebrating the career of discover Dr. David Latham and attended by his colleagues and collaborators, the planet was informally dubbed "Latham's Planet".[11] However, this name has no official standing with the International Astronomical Union.
See also
References
- 1 2 Butler, R. P.; Wright, J. T.; Marcy, G. W.; Fischer, D. A.; Vogt, S. S.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701.
- 1 2 3 4 5 6 7 Kane, Stephen R.; Henry, Gregory W.; Dragomir, Diana; Fischer, Debra A.; Howard, Andrew W.; et al. (2011). "Revised Orbit and Transit Exclusion for HD 114762b". The Astrophysical Journal Letters 735 (2). L41. arXiv:1106.1434. Bibcode:2011ApJ...735L..41K. doi:10.1088/2041-8205/735/2/L41.
- 1 2 Wang, Sharon Xuesong; Wright, Jason T.; Cochran, William; Kane, Stephen R.; Henry, Gregory W.; et al. (2012). "The Discovery of HD 37605c and a Dispositive Null Detection of Transits of HD 37605b". The Astrophysical Journal 761 (1): 46–59. arXiv:1210.6985. Bibcode:2012ApJ...761...46W. doi:10.1088/0004-637X/761/1/46.
- 1 2 3 Kane, Stephen R.; Gelino, Dawn M. (July 2012). "Distinguishing between stellar and planetary companions with phase monitoring". Monthly Notices of the Royal Astronomical Society 424 (1): 779–788. arXiv:1205.5812. Bibcode:2012MNRAS.424..779K. doi:10.1111/j.1365-2966.2012.21265.x.
- 1 2 North, Gerald (2003). Astronomy in Depth. New York: Springer. p. 185. ISBN 9781852335809.
- 1 2 Latham, David W.; Mazeh, Tsevi; Stefanik, Robert P.; Mayor, Michel; Burki, Gilbert (4 May 1989). "The unseen companion of HD114762: a probable brown dwarf". Nature 339 (6219): 38–40. Bibcode:1989Natur.339...38L. doi:10.1038/339038a0.
- 1 2 "HD 114762b -- Extra-solar Confirmed Planet". SIMBAD. Retrieved 31 August 2014.
- 1 2 Cochran, William D.; Hatzes, Artie P.; Hancock, Terry J. (10 October 1991). "Constraints on the Companion Object to HD 114762". The Astrophysical Journal 380: L35–L38. Bibcode:1991ApJ...380L..35C. doi:10.1086/186167.
- ↑ Hale, Alan (1995). "On the Nature of the Companion to HD 114762". Publications of the Astronomical Society of the Pacific (The University of Chicago Press) 107 (707): 22–26. Bibcode:1995PASP..107...22H. doi:10.1086/133511. JSTOR 40680489.
- ↑ Marcy, Geoffrey W.; Butler, R. Paul; Vogt, Steven S.; Fischer, Debra; Liu, Michael C. (1999). "Two New Candidate Planets in Eccentric Orbits". The Astrophysical Journal 520 (1): 239–247. arXiv:astro-ph/9904275. Bibcode:1999ApJ...520..239M. doi:10.1086/307451.
- ↑ Johnson, John (2016). How do you find an Exoplanet?. New Jersey: Princeton University Press. p. 137. ISBN 978-0-691-15681-1.
Coordinates: 13h 12m 19.7427s, +17° 31′ 01.643″