DENIS-P J082303.1−491201 b
DENIS-P J082303.1-491201 b (alias 2MASS J08230313-4912012 b) is a substellar object, classified as either an exoplanet or a brown dwarf, orbiting DENIS-P J082303.1-491201,[4] an L1.5-type brown dwarf in the constellation Vela.[2]
Discovery[1] | |
---|---|
Discovered by | Sahlmann et al. (2013) |
Discovery site | ESO telescopes at the La Silla Paranal Observatory |
Discovery date | August 2013 |
Astrometry | |
Designations | |
2MASS J08230313-4912012 b[2] | |
Orbital characteristics[2] | |
0.36±0.01 AU | |
Eccentricity | 0.345+0.068 −0.064 |
246.36+1.38 −1.35 days | |
Inclination | 56.6+1.9 −2.1 deg |
36.3+7.2 −8.4 deg | |
Physical characteristics | |
Mass | 28.5±1.9 MJ[2] |
Temperature | 1670 |
Spectral type | L5.5[3] |
Discovery
DENIS-P J082303.1-491201 b was discovered by Sahlmann et al. (2013) using the ESO telescopes at the La Silla Paranal Observatory.[1] It is part of an ultracool binary system.[1]
Properties
It is located 20.77 parsecs (67.7 ly) from Earth. At 28.5±1.9 MJ,[2] it is listed as among the most massive planets in the NASA Exoplanet Archive.
It orbits the nearby L1.5-type brown dwarf DENIS-P J082303.1-491201, which is 7.5±0.7% the mass of our Sun,[1] and has an orbital period of about 246 days.[1][2]
See also
- Deep Near Infrared Survey of the Southern Sky
- DENIS-P J1058.7-1548
- DENIS-P J1228.2-1547
- DENIS-P J020529.0-115925
- DENIS-P J101807.5-285931
- List of exoplanet extremes
- List of exoplanets discovered using the Kepler spacecraft
References
- Sahlmann, J.; Lazorenko, P. F.; Ségransan, D.; Martín, E. L.; Queloz, D.; et al. (August 2013). "Astrometric orbit of a low-mass companion to an ultracool dwarf". Astronomy & Astrophysics. 556. A133. arXiv:1306.3225. Bibcode:2013A&A...556A.133S. doi:10.1051/0004-6361/201321871.
- "DENIS-P J082303.1-491201 b". Caltech. Retrieved 8 March 2014.
- A bot will complete this citation soon. Click here to jump the queue arXiv:1906.04166.
- "2MASS J08230313-4912012". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 March 2014.
External links
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