Jump to content

TYC 9486-927-1: Difference between revisions

From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
"M6.5" → "M6 or M7" to match the ambiguity in Smart et al. (2019)
"6,900.0" → "6,900" and removed tildes per MOS:UNCERTAINTY; added commas per MOS:DIGITS
Line 49: Line 49:
TYC 9486-927-1 has rapid rotation and [[stellar corona|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.<ref name=sacy/>
TYC 9486-927-1 has rapid rotation and [[stellar corona|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.<ref name=sacy/>


The secondary stellar companion is [[2MASS J21121598–8128452]]. It is a red dwarf star of spectral class M5.5. Its projected separation from the primary is the ∼62700 [[astronomical unit|AU]]. The tertiary companion is [[2MASS J21192028–8145446]] - a young brown dwarf of spectral class M6 or M7 at projected separation of the 31000 [[astronomical units|AU]] from the primary.<ref name=Smart2019/>{{rp|7}}
The secondary stellar companion is [[2MASS J21121598–8128452]]. It is a red dwarf star of spectral class M5.5. Its projected separation from the primary is the 62,700 [[astronomical unit|AU]]. The tertiary companion is [[2MASS J21192028–8145446]] - a young brown dwarf of spectral class M6 or M7 at projected separation of the 31,000 [[astronomical units|AU]] from the primary.<ref name=Smart2019/>{{rp|7}}


==Planetary system==
==Planetary system==
Line 60: Line 60:
{{OrbitboxPlanet
{{OrbitboxPlanet
| exoplanet = [[2MASS J2126-8140]]
| exoplanet = [[2MASS J2126-8140]]
| mass = 13.3 (± 1.7) <ref name=Exoplanet.eu>{{cite web
| mass = 13.3 (± 1.7)<ref name=Exoplanet.eu>{{cite web
|url = http://exoplanet.eu/catalog/2m_j2126-81_b
|url = http://exoplanet.eu/catalog/2m_j2126-81_b
|title = Planet 2MASS J2126-8140
|title = Planet 2MASS J2126-8140
Line 69: Line 69:
| radius = <!-- Radius of the planet, in Jupiter radii -->
| radius = <!-- Radius of the planet, in Jupiter radii -->
| radius_earth = <!-- Radius of the planet, in Earth radii -->
| radius_earth = <!-- Radius of the planet, in Earth radii -->
| semimajor = 6,900.0<ref name=Exoplanet.eu/>
| semimajor = 6,900<ref name=deacon/>
| period = 328 725 000
| period = 328 725 000
| eccentricity = <!--Eccentricity of the planet-->
| eccentricity = <!--Eccentricity of the planet-->

Revision as of 23:23, 7 January 2021

TYC 9486-927-1 1
Observation data
Epoch       Equinox
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]
Distance111.4 ± 0.3 ly
(34.15 ± 0.08 pc)
Details
Mass0.53[4] M☉
Temperature3,490[5] K
Rotational velocity (v sin i)43.5 ± 1.2[5] km/s
Age10-45[5] Myr
Other designations
2MASS J21252752-8138278,
Database references
SIMBADdata

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 2MASS J21121598–8128452. It is a red dwarf star of spectral class M5.5. Its projected separation from the primary is the 62,700 AU. The tertiary companion is 2MASS J21192028–8145446 - a young brown dwarf of spectral class M6 or M7 at projected separation of the 31,000 AU from the primary.[4]: 7 

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]

The TYC 9486-927-1 planetary system
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
([[d]]s) 		Eccentricity Inclination Radius
2MASS J2126-8140 13.3 (± 1.7)[8] MJ 6,900[5] 328 725 000 — — —

References

  1. ^ 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.
  2. ^ 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.
  3. ^ 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.
  4. ^ 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)
  5. ^ a b c d 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)
  6. ^ 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.
  7. ^ 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.
  8. ^ "Planet 2MASS J2126-8140". exoplanet.eu. Retrieved 2016-01-27.
Retrieved from "https://en.wikipedia.org/w/index.php?title=TYC_9486-927-1&oldid=998983909"