Astronomy:HD 111232 b
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Short description: Extrasolar planet in the constellation of Musca
| Discovery | |
|---|---|
| Discovered by | Mayor et al. |
| Discovery site | La Silla Observatory, Chile |
| Discovery date | 30 June 2003 |
| Doppler Spectroscopy (CORALIE) | |
| Orbital characteristics[1] | |
| 2.148+0.088 −0.097 astronomical unit|AU | |
| Eccentricity | 0.214+0.005 −0.003 |
| Orbital period | 3.201+0.002 −0.001 yr |
| Inclination | 93.521°+16.622° −18.063° |
| Longitude of ascending node | 358.306°+52.528° −32.102° |
| astron|astron|helion}} | 2452361.045+4.144 −3.497 |
| 94.142°+0.920° −0.719° | |
| Semi-amplitude | 160.429+0.573 −0.509 m/s |
| Star | HD 111232 |
| Physical characteristics[1] | |
| Mass | 7.965+1.128 −0.479 Jupiter mass |
HD 111232 b is an extrasolar planet that orbits at almost 2 AU with a minimum mass of 6.8 times that of Jupiter. This planet was discovered in the La Silla Observatory by Michel Mayor using the CORALIE spectrograph on 30 June 2003, along with six other planets, including HD 41004 Ab, HD 65216 b, HD 169830 c, HD 216770 b, HD 10647 b, and HD 142415 b.[2]
An astrometric measurement of the planet's inclination and true mass was published in 2022 as part of Gaia DR3.[3]
References
- ↑ 1.0 1.1 Feng, Fabo et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series 262 (21): 21. doi:10.3847/1538-4365/ac7e57. Bibcode: 2022ApJS..262...21F.
- ↑ Mayor, M. et al. (2004). "The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE". Astronomy and Astrophysics 415 (1): 391–402. doi:10.1051/0004-6361:20034250. Bibcode: 2004A&A...415..391M. http://www.aanda.org/articles/aa/full/2004/07/aa0250/aa0250.html.
- ↑ Gaia Collaboration et al. (2023). "Gaia Data Release 3". Astronomy & Astrophysics 674: A34. doi:10.1051/0004-6361/202243782.
External links
Coordinates: 
12h 48m 51.7543s, −68° 25′ 30.544″
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