TYC 9486-927-1: Difference between revisions
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==Planetary system== |
==Planetary system== |
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[[2MASS J21265040-8140293]] planet orbits TYC 9486-927-1 at a projected separation of {{Val|7400|u=AU}}.<ref name=Smart2019>{{citation|arxiv=1902.07571|title=The Gaia Ultra-Cool Dwarf Sample – II: Structure at the end of the main sequence|year=2019}}</ref> With a mass from 11.6 to 15 [[Jupiter]] masses, it is considered to be either a star, a brown dwarf, or a giant planet.<ref name=banyan/><ref name=reid/> |
[[2MASS J21265040-8140293]] planet orbits TYC 9486-927-1 at a projected separation of {{Val|7400|u=AU}}.<ref name=Smart2019>{{citation|arxiv=1902.07571|title=The Gaia Ultra-Cool Dwarf Sample – II: Structure at the end of the main sequence|year=2019|doi=10.1093/mnras/stz678|last1=Jones|first1=H R A.|last2=Caballero|first2=J. A.|last3=Beamín|first3=J. C.|last4=Barrado|first4=D.|last5=Sarro|first5=L. M.|last6=Marocco|first6=F.|last7=Smart|first7=R. L.|journal=Monthly Notices of the Royal Astronomical Society|volume=485|issue=3|pages=4423–4440|bibcode=2019MNRAS.485.4423S|s2cid=119421722}}</ref> With a mass from 11.6 to 15 [[Jupiter]] masses, it is considered to be either a star, a brown dwarf, or a giant planet.<ref name=banyan/><ref name=reid/> |
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==References== |
==References== |
Revision as of 01:14, 16 November 2020
Observation data Epoch Equinox | |
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Constellation | Octans |
Right ascension | 21h 25m 27.4899s[1] |
Declination | –81° 38′ 27.673″[1] |
Apparent magnitude (V) | 11.821[1] |
Characteristics | |
Spectral type | M1 V[2] |
Astrometry | |
Radial velocity (Rv) | 8.7 ± 4.6[2] km/s |
Proper motion (μ) | RA: 59.843 mas/yr Dec.: -107.723 mas/yr |
Parallax (π) | 29.2836 ± 0.0690 mas[3] |
Distance | 111.4 ± 0.3 ly (34.15 ± 0.08 pc) |
Details | |
Mass | 0.53[4] M☉ |
Temperature | 3,490[5] K |
Rotational velocity (v sin i) | 43.5 ± 1.2[5] km/s |
Age | 10-45[5] Myr |
Other designations | |
2MASS J21252752-8138278, | |
Database references | |
SIMBAD | data |
TYC 9486-927-1 (also known as 2MASS J21252752-8138278) is a primary of a ternary star system located at a distance of 26.7 parsecs from Earth in the southern direction in the constellation of Octans. It is a dwarf (luminosity class V) red (spectral class M1) variable by rotation.
TYC 9486-927-1 has rapid rotation and coronal and chromospheric activity suggestive of a young age. Observations and multi-epoch radial velocity data suggest that TYC 9486-927-1 is a single, rapidly rotating star rather than a spectroscopic or tight, visual binary. However, it is still possible that TYC 9486-927-1 is an equal mass binary with a face-on orbit and close separation.[2]
The secondary stellar companion is the 2MASS J21121598–8128452. It is a red dwarf star of spectral class M5.5. Its projected separation from the primary is the ∼62700 AU. The tertiary companion is the 2MASS J21121598–8128452 - a young brown dwarf of spectral class M6.5 at projected separation of the 31000 AU from the primary.[4]
Planetary system
2MASS J21265040-8140293 planet orbits TYC 9486-927-1 at a projected separation of 7400 AU.[4] With a mass from 11.6 to 15 Jupiter masses, it is considered to be either a star, a brown dwarf, or a giant planet.[6][7]
References
- ^ a b c Zacharias, N.; Finch, C. T.; Girard, T. M.; Henden, A.; Bartlett, J. L.; Monet, D. G.; Zacharias, M. I. (2012). "VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)". VizieR On-line Data Catalog: I/322A. Originally Published in: 2012yCat.1322....0Z; 2013AJ....145...44Z. 1322. Bibcode:2012yCat.1322....0Z.
- ^ a b c Torres, C. A. O.; Quast, G. R.; Da Silva, L.; de la Reza, R.; Melo, C. H. F.; Sterzik, M. (2006). "Search for associations containing young stars (SACY). I. Sample and searching method". Astronomy and Astrophysics. 460 (3): 695. arXiv:astro-ph/0609258. Bibcode:2006A&A...460..695T. doi:10.1051/0004-6361:20065602. S2CID 16080025.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c Jones, H R A.; Caballero, J. A.; Beamín, J. C.; Barrado, D.; Sarro, L. M.; Marocco, F.; Smart, R. L. (2019), "The Gaia Ultra-Cool Dwarf Sample – II: Structure at the end of the main sequence", Monthly Notices of the Royal Astronomical Society, 485 (3): 4423–4440, arXiv:1902.07571, Bibcode:2019MNRAS.485.4423S, doi:10.1093/mnras/stz678, S2CID 119421722
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c Deacon, N. R.; Schlieder, J. E.; Murphy, S. J. (2016). "A nearby young M dwarf with a wide, possibly planetary-mass companion". Monthly Notices of the Royal Astronomical Society. 457 (3): 3191. arXiv:1601.06162. Bibcode:2016MNRAS.457.3191D. doi:10.1093/mnras/stw172. S2CID 18220333.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Gagné, Jonathan; Lafrenière, David; Doyon, René; Malo, Lison; Artigau, Étienne (2014). "BANYAN. II. Very Low Mass and Substellar Candidate Members to Nearby, Young Kinematic Groups with Previously Known Signs of Youth". The Astrophysical Journal. 783 (2): 121. arXiv:1312.5864. Bibcode:2014ApJ...783..121G. doi:10.1088/0004-637X/783/2/121. S2CID 119251619.
- ^ Reid, I. Neill; Cruz, Kelle L.; Kirkpatrick, J. Davy; Allen, Peter R.; Mungall, F.; Liebert, James; Lowrance, Patrick; Sweet, Anne (2008). "Meeting the Cool Neighbors. X. Ultracool Dwarfs from the 2MASS All-Sky Data Release". The Astronomical Journal. 136 (3): 1290. arXiv:0806.3413. Bibcode:2008AJ....136.1290R. doi:10.1088/0004-6256/136/3/1290.