2MASS 1503+2525

2MASS J15031961+2525196 (2MASS 1503+2525) is a nearby brown dwarf of spectral type T5.5,[2] located in constellation Boötes at approximately 20.7 light-years from Earth.[3]

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]
Database references
SIMBADdata

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

Currently 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.[3]

2MASS 1503+2525 distance estimates

SourceParallax, masDistance, pcDistance, lyRef.
Burgasser et al. (2003)~7.8~25.4[2]
Dupuy & Liu (2012)157.2 ± 2.26.36 ± 0.0920.7 ± 0.3[3]

Non-trigonometric distance estimates are marked in italic. The best estimate is marked in bold.

gollark: https://drive.google.com/drive/folders/1OL0D5ujUX3Eyd3xcSbeXaEWe0nRmT5U1?usp=sharing↑ GPT-2 instance trained on my Discord messages
gollark: Anyway, thanks to bizarre Google projects, people who actually know what they're doing, and Python, you can quite easily train GPT-2s on arbitrary collections of data and achieve reasonable quality.
gollark: Added to your psychological profile.
gollark: GPT-2 is a something something transformers something something 117 million parameters something something natural language processing something something deep learning.
gollark: No, it's MUCH more advanced.

References

  1. "2MASS J15031961+2525196 -- Brown Dwarf (M<0.08solMass)". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-09-19.
  2. Burgasser, A. 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.
  3. 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.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.