2MASS J01225093−2439505
Multiplicity surveys did not detect any stellar companions to 2MASS J01225093−2439505 as of 2016.
Planetary system
In 2013, one superjovian planet (may be a brown dwarf), named 2MASS J01225093−2439505 b, was discovered by direct imaging. The measured planetary temperature is 1600±100 K, and it exhibits an unusual, short-lived atmospheric dust type due to its relatively low surface gravity and young age. The planetary spectrum is classified as L3.7±1.0. The planetary rotation axis is inclined to its orbit, obliquity is 33
−9°, while the orbit is well aligned with the equatorial plane of the star, misalignment is 1
−1°. The planet is rotating rapidly, with a period of 6.8±1.8 hours.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 19.5±7.5 MJ | 50 | — | — | 103 −6° |
1.04±0.18 RJ |
References
- ^ "LEHPM 1481". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-08.
- ^ Bowler, Brendan P.; Liu, Michael C.; Shkolnik, Evgenya L.; Dupuy, Trent J. (2013). "Planets Around Low-Mass Stars. III. A Young Dusty L Dwarf Companion at the Deuterium-Burning Limit". The Astrophysical Journal. 774 (1): 55. arXiv:1307.2237. Bibcode:2013ApJ...774...55B. doi:10.1088/0004-637X/774/1/55. S2CID 119107288.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ Hinkley, Sasha; Bowler, Brendan P.; Vigan, Arthur; Aller, Kimberly M.; Liu, Michael C.; Mawet, Dimitri; Matthews, Elisabeth; Wahhaj, Zahed; Kraus, Stefan; Baraffe, Isabelle; Chabrier, Gilles (2015). "Early Results from VLT Sphere: Long-Slit Spectroscopy of 2Mass 0122–2439 B, A Young Companion Near the Deuterium Burning Limit". The Astrophysical Journal. 805 (1): L10. arXiv:1504.07240. Bibcode:2015ApJ...805L..10H. doi:10.1088/2041-8205/805/1/L10. S2CID 20992122.
- ^ Bryan, Marta L.; Chiang, Eugene; Bowler, Brendan P.; Morley, Caroline V.; Millholland, Sarah; Blunt, Sarah; Ashok, Katelyn B.; Nielsen, Eric; Ngo, Henry; Mawet, Dimitri; Knutson, Heather A. (2020). "Obliquity Constraints on an Extrasolar Planetary-mass Companion". The Astronomical Journal. 159 (4): 181. arXiv:2002.11131. Bibcode:2020AJ....159..181B. doi:10.3847/1538-3881/ab76c6. S2CID 211505793.
- ^ Zhou, Yifan; Apai, Dániel; Lew, Ben W. P.; Schneider, Glenn; Manjavacas, Elena; Bedin, Luigi R.; Cowan, Nicolas B.; Marley, Mark S.; Radigan, Jacqueline; Karalidi, Theodora; Lowrance, Patrick J.; Miles-Páez, Paulo A.; Metchev, Stanimir; Burgasser, Adam J. (2019). "Cloud Atlas: High-contrast Time-resolved Observations of Planetary-mass Companions". The Astronomical Journal. 157 (3): 128. arXiv:1902.00085. Bibcode:2019AJ....157..128Z. doi:10.3847/1538-3881/ab037f. S2CID 119074052.
- ^ Bryan, Marta L.; Bowler, Brendan P.; Knutson, Heather A.; Kraus, Adam L.; Hinkley, Sasha; Mawet, Dimitri; Nielsen, Eric L.; Blunt, Sarah C. (2016). "Searching for Scatterers: High-Contrast Imaging of Young Stars Hosting Wide-Separation Planetary-Mass Companions". The Astrophysical Journal. 827 (2): 100. arXiv:1606.06744. Bibcode:2016ApJ...827..100B. doi:10.3847/0004-637X/827/2/100. S2CID 8681056.
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