2MASS J00361617 1821104
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pisces |
| Right ascension | 00h 36m 16.112s[1] |
| Declination | 18° 21′ 10.29″[1] |
| Apparent magnitude (V) | 21.33±0.06[2] |
| Characteristics | |
| Evolutionary stage | Brown dwarf[2] |
| Spectral type | L3.5[2] |
| Apparent magnitude (J) | 12.44[2] |
| Apparent magnitude (H) | 11.58[2] |
| Apparent magnitude (K) | 11.03[2] |
| B−V color index | 1.7±0.2[2] |
| Astrometry | |
| Radial velocity (Rv) | 21.7±3.0[2] km/s |
| Proper motion (μ) | RA: 901.582 mas/yr[1] Dec.: 124.354 mas/yr[1] |
| Parallax (π) | 114.4735 ± 0.1381 mas[1] |
| Distance | 28.49 ± 0.03 ly (8.74 ± 0.01 pc) |
| Details | |
| Radius | 1.01±0.07[3] RJup |
| Temperature | 1300–2000[citation needed] K |
| Rotation | 3.08±0.05 h[4] |
| Other designations | |
| Database references | |
| SIMBAD | data |
2MASS J00361617 1821104 (abbreviated to 2MASS 0036 1821) is a brown dwarf, located in 28.6 light-years from Earth in the constellation Pisces. It was discovered in 2000 by I. Neill Reid et al. Kinematically, it does not belong to any known moving group, been grouped with other "field stars".[5]
2MASS 0036 1821 is of spectral type L3.5, the surface temperature is 1300-2000 Kelvin. As with other brown dwarfs of spectral type L, its spectrum is dominated of metal hydrides and alkali metals. Its position shifts due to its proper motion by 0.9071 arcseconds per year.
The surface of 2MASS 0036 1821 is completely covered by clouds, although cloud deck appear to be thin (less than ten optical depths)[4] Because of unusually rapid rotation, it is possessing a strong magnetic field over 1000 G at the photosphere level,[6] and is well known for its radio emissions.[7]
2MASS 0036 1821 is likely a binary separated by 0.4 astronomical units. Assuming an age of 0.5-5 Billion years, the A component has a mass estimate of 51-76 MJ and the B component has a mass estimate of 47-74 MJ.[8]
See also
[edit]References
[edit]- ^ a b c d 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.
- ^ a b c d e f g h Reid, I. Neill; et al. (January 2000), "Four Nearby L Dwarfs", The Astronomical Journal, 119 (1): 369–377, arXiv:astro-ph/9909336, Bibcode:2000AJ....119..369R, doi:10.1086/301177.
- ^ Vos, Johanna M.; Biller, Beth A.; Allers, Katelyn N.; Faherty, Jacqueline K.; Liu, Michael C.; Metchev, Stanimir; Eriksson, Simon; Manjavacas, Elena; Dupuy, Trent J.; Janson, Markus; Radigan-Hoffman, Jacqueline; Crossfield, Ian; Bonnefoy, Mickaël; Best, William M. J.; Homeier, Derek; Schlieder, Joshua E.; Brandner, Wolfgang; Henning, Thomas; Bonavita, Mariangela; Buenzli, Esther (2020), "Spitzer Variability Properties of Low-gravity L Dwarfs", The Astronomical Journal, 160 (1): 38, arXiv:2005.12854, Bibcode:2020AJ....160...38V, doi:10.3847/1538-3881/ab9642, S2CID 218889787
- ^ a b Sanghavi, Suniti; Shporer, Avi (2018), "Photopolarimetric Characteristics of Brown Dwarfs. I. Uniform Cloud Decks", The Astrophysical Journal, 866 (1): 28, arXiv:1705.05041, Bibcode:2018ApJ...866...28S, doi:10.3847/1538-4357/aadf94, S2CID 55544773
- ^ Riedel, Adric R.; Ditomasso, Victoria; Rice, Emily L.; Alam, Munazza K.; Abrahams, Ellianna; Crook, James; Cruz, Kelle L.; Faherty, Jacqueline K. (2019), "Radial Velocities, Space Motions, and Nearby Young Moving Group Memberships of Eleven Candidate Young Brown Dwarfs", The Astronomical Journal, 157 (6): 247, arXiv:1904.10579, Bibcode:2019AJ....157..247R, doi:10.3847/1538-3881/ab1915, S2CID 129945848
- ^ Guenther, E. W.; Zapatero-Osorio, María Rosa; Mehner, A.; Martín, Eduardo L. (2009), "Short-term spectroscopic monitoring of two cool dwarfs with strong magnetic fields", Astronomy & Astrophysics, 498 (1): 281–287, arXiv:0903.2340, Bibcode:2009A&A...498..281G, doi:10.1051/0004-6361/200810216, S2CID 18611224
- ^ Zic, Andrew; Lynch, Christene; Murphy, Tara; Kaplan, David L.; Chandra, Poonam (February 2019), "Low-frequency GMRT observations of ultra-cool dwarfs", Monthly Notices of the Royal Astronomical Society, 483 (1): 614–623, arXiv:1811.09294, doi:10.1093/mnras/sty3163
- ^ Pope, Benjamin; Martinache, Frantz; Tuthill, Peter (2013-04-01). "Dancing in the Dark: New Brown Dwarf Binaries from Kernel Phase Interferometry". The Astrophysical Journal. 767 (2): 110. arXiv:1302.6682. Bibcode:2013ApJ...767..110P. doi:10.1088/0004-637X/767/2/110. ISSN 0004-637X.
External links
[edit]- Entry at DwarfArchives.org Archived 2019-06-10 at the Wayback Machine
- Discovery paper
- Simbad
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