DEN 1048-3956

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DEN 1048-3956
Observation data
Epoch J2000      Equinox J2000
Constellation Antlia
Right ascension 10h 48m 14.640s[1]
Declination –39° 56′ 06.24″[1]
Apparent magnitude (V) 17.4[2]
Characteristics
Spectral type M9 V or L0
Apparent magnitude (J) 9.5[1]
Astrometry
Radial velocity (Rv) –10.1 ± 0.5[1] km/s
Proper motion (μ) RA: –1198 ± 10[1] mas/yr
Dec.: –970 ± 8[1] mas/yr
Parallax (π) 248.53 ± 1.18[2] mas
Distance 13.12 ± 0.06 ly
(4.02 ± 0.02 pc)
Absolute magnitude (MV) 19.37[2]
Details
Mass 0.07[2] M
Luminosity 0.00000356 L
Other designations
2MASS J10481463-3956062, 2MASSI J1048147-395606, 2MUCD 20385, DENIS-P J104814.9-395604, DENIS-P J104814.7-395606, DEN 1048-3956, USNO-B1.0 0500-00227632
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

DEN 1048-3956 is a brown dwarf about 13 light years from the Earth in the southern constellation of Antlia, among the closer interstellar objects to the Earth. This substellar object is very dim with an apparent magnitude of about 17,[2] and will require a telescope with a camera to be seen. It was discovered in 2000 by Xavier Delfosse (Institute of Astrophysics of the Canary Islands, now Observatoire de Grenoble) and Thierry Forveille (Canada-France-Hawaii Telescope Corporation), with the assistance of nine other astronomers.

In 2005 a powerful flare from this object was detected by radio astronomy.[3]

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