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2MASS J2126–8140

2MASS J21265040−8140293, also known as 2MASS J2126−8140,[3] is an exoplanet orbiting the red dwarf TYC 9486-927-1, 111.4±0.3[5] light-years away from Earth. Its estimated mass, age (10-45 million years), spectral type (L3), and Teff (1800 K) are similar to the well-studied planet β Pictoris b.[3] With an estimated distance of around 1 trillion kilometres from its host star, it is one of the largest solar systems ever found.[6]

2MASS J21265040−8140293
Discovery[1]
Discovered byK. L. Cruz, J. D. Kirkpatrick, A. J. Burgasser[2] [3]
Discovery date2009
Direct imaging
Orbital characteristics
6,900[3] AU (1.03×1012 km)
328,725,000 days (~900,000 years)
StarTYC 9486-927-1
Physical characteristics
Mass13.3 (± 1.7) [1] MJ
Temperature~1,800 K (1,530 °C; 2,780 °F)[1]
Spectral type
L3.0[4]
20.72 (G-band)[4]

See also edit

References edit

  1. ^ a b c "Planet 2MASS J2126-8140". Extrasolar Planets Encyclopaedia. 1995. Retrieved 2016-01-27.
  2. ^ Cruz, Kelle L.; Kirkpatrick, J. Davy; Burgasser, Adam J. (2009). "Young L Dwarfs Identified in the Field: A Preliminary Low-Gravity, Optical Spectral Sequence from L0 to L5". Astronomical Journal. 137 (2): 3445. arXiv:0812.0364. Bibcode:2009AJ....137.3345C. doi:10.1088/0004-6256/137/2/3345. S2CID 15376964.
  3. ^ a b c d N. Deacon; J. Schleider; S. Murphy (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.
  4. ^ a b 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, doi:10.1093/mnras/stz678, S2CID 119421722
  5. ^ 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.
  6. ^ "Astronomers find the largest solar system in the galaxy". exoplanets.nasa.gov. February 1, 2016. Retrieved January 20, 2022.

2mass, j2126, 8140, 2mass, j21265040, 8140293, also, known, 2mass, j2126, 8140, exoplanet, orbiting, dwarf, 9486, light, years, away, from, earth, estimated, mass, million, years, spectral, type, teff, 1800, similar, well, studied, planet, pictoris, with, esti. 2MASS J21265040 8140293 also known as 2MASS J2126 8140 3 is an exoplanet orbiting the red dwarf TYC 9486 927 1 111 4 0 3 5 light years away from Earth Its estimated mass age 10 45 million years spectral type L3 and Teff 1800 K are similar to the well studied planet b Pictoris b 3 With an estimated distance of around 1 trillion kilometres from its host star it is one of the largest solar systems ever found 6 2MASS J21265040 8140293Discovery 1 Discovered byK L Cruz J D Kirkpatrick A J Burgasser 2 3 Discovery date2009Detection methodDirect imagingOrbital characteristicsSemi major axis6 900 3 AU 1 03 1012 km Orbital period sidereal 328 725 000 days 900 000 years StarTYC 9486 927 1Physical characteristicsMass13 3 1 7 1 MJTemperature 1 800 K 1 530 C 2 780 F 1 Spectral typeL3 0 4 Apparent magnitude20 72 G band 4 See also editCOCONUTS 2bReferences edit a b c Planet 2MASS J2126 8140 Extrasolar Planets Encyclopaedia 1995 Retrieved 2016 01 27 Cruz Kelle L Kirkpatrick J Davy Burgasser Adam J 2009 Young L Dwarfs Identified in the Field A Preliminary Low Gravity Optical Spectral Sequence from L0 to L5 Astronomical Journal 137 2 3445 arXiv 0812 0364 Bibcode 2009AJ 137 3345C doi 10 1088 0004 6256 137 2 3345 S2CID 15376964 a b c d N Deacon J Schleider S Murphy 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 a b Jones H R A Caballero J A Beamin 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 doi 10 1093 mnras stz678 S2CID 119421722 Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR Astronomers find the largest solar system in the galaxy exoplanets nasa gov February 1 2016 Retrieved January 20 2022 nbsp This extrasolar planet related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title 2MASS J2126 8140 amp oldid 1191315068, wikipedia, wiki, book, books, library,

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