2MASS J15031961+2525196
Observation data
Epoch J2000[1]      Equinox J2000[1]
Constellation Boötes
Right ascension 15h 03m 19.613s[1]
Declination 25° 25′ 19.68″[1]
Characteristics
Spectral type T5[2]
Astrometry
Radial velocity (Rv)33±14[3] km/s
Proper motion (μ) RA: 87.414±0.613[4] mas/yr
Dec.: 557.780±0.695[4] mas/yr
Parallax (π)155.7758 ± 0.7557 mas[4]
Distance20.9 ± 0.1 ly
(6.42 ± 0.03 pc)
Other designations
Gaia DR2 1267906854386665088, 2MASS J15031961+2525196, SDSS J150319.64+252522.4[1]
Database references
SIMBADdata
2MASS 1503+2525 is located in the constellation Boötes
2MASS 1503+2525 is located in the constellation Boötes
2MASS 1503+2525
Location of 2MASS 1503+2525 in the constellation Boötes

2MASS J15031961+2525196 (2MASS 1503+2525) is a nearby brown dwarf of spectral type T5.5,[5] located in the constellation of Boötes at approximately 20.7 light-years from Earth.[6]

History of observations

Discovery

2MASS 1503+2525 was discovered in 2003 by Adam J. Burgasser et al. in wide-field search for T dwarfs using the Two Micron All Sky Survey (2MASS).

Distance

Originally the most precise distance estimate of 2MASS 1503+2525 is a trigonometric parallax, published by Dupuy and Liu in 2012: 157.2 ± 2.2 mas, corresponding to a distance 6.36 ± 0.09 pc, or 20.7 ± 0.3 ly.[6] The parallax was further refined by Gaia mission in 2018 to 154.9208±1.1025mas. The brown dwarf 2MASS 1503+2525 lies in local void 6.5 parsecs across, where relatively few stars and brown dwarfs are located.[7]

Physical properties

The 2MASS J15031961+2525196 is the spectral standard of the spectral class T5.[8]

References

  1. 1 2 3 4 5 "2MASS J15031961+2525196 -- Brown Dwarf (M<0.08solMass)". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-09-19.
  2. ↑ Martin, Emily C.; Mace, Gregory N.; McLean, Ian S.; Logsdon, Sarah E.; Rice, Emily L.; Kirkpatrick, J. Davy; Burgasser, Adam J.; McGovern, Mark R.; Prato, Lisa (2017), "Surface Gravities for 228 M, L, and T Dwarfs in the NIRSPEC Brown Dwarf Spectroscopic Survey", The Astrophysical Journal, 838 (1): 73, arXiv:1703.03811, Bibcode:2017ApJ...838...73M, doi:10.3847/1538-4357/aa6338, S2CID 28337547
  3. ↑ Robert, Jasmin; Gagné, Jonathan; Artigau, Étienne; Lafrenière, David; Nadeau, Daniel; Doyon, René; Malo, Lison; Albert, Loïc; Simard, Corinne; Gagliuffi, Daniella C. Bardalez; Burgasser, Adam J. (2016), "A Brown Dwarf Census from the Simp Survey", The Astrophysical Journal, 830 (2): 144, arXiv:1607.06117, Bibcode:2016ApJ...830..144R, doi:10.3847/0004-637X/830/2/144, S2CID 119192461
  4. 1 2 3 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.
  5. ↑ Burgasser, Adam J.; Kirkpatrick, J. Davy; McElwain, Michael W.; Cutri, Roc M.; Burgasser, Albert J.; Skrutskie, Michael F. (2003). "The 2Mass Wide-Field T Dwarf Search. I. Discovery of a Bright T Dwarf within 10 Parsecs of the Sun". The Astronomical Journal. 125 (2): 850–857. arXiv:astro-ph/0211117. Bibcode:2003AJ....125..850B. doi:10.1086/345975. S2CID 15764829.
  6. 1 2 Dupuy, Trent J.; Liu, Michael C. (2012). "The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition". The Astrophysical Journal Supplement. 201 (2): 19. arXiv:1201.2465. Bibcode:2012ApJS..201...19D. doi:10.1088/0067-0049/201/2/19. S2CID 119256363.
  7. ↑ Bihain, G.; Scholz, R.-D. (2016), "A non-uniform distribution of the nearest brown dwarfs", Astronomy & Astrophysics, 589: A26, arXiv:1603.00714, Bibcode:2016A&A...589A..26B, doi:10.1051/0004-6361/201528007, S2CID 119102741
  8. ↑ Tinney, C. G.; Kirkpatrick, J. Davy; Faherty, Jacqueline K.; Mace, Gregory N.; Cushing, Mike; Gelino, Christopher R.; Burgasser, Adam J.; Sheppard, Scott S.; Wright, Edward L. (2018), "New y and T Dwarfs from WISE Identified by Methane Imaging", The Astrophysical Journal Supplement Series, 236 (2): 28, arXiv:1804.00362, Bibcode:2018ApJS..236...28T, doi:10.3847/1538-4365/aabad3, S2CID 54970570


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