GD 165 B
Nomenclature and observation
The system GD 165 is named after Henry L. Giclas, an American Astronomer who lived throughout the 20th century.
GD 165 B was discovered in 1988 by Becklin and Zuckerman at the University of California, Los Angeles. GD 165 B was the first brown dwarf discovered to be cooler than M-Type stars and was initially assigned the spectral type ≥M10. It would not be recognized as a brown dwarf until 1999, when new spectral types L-Type and T-Type for objects cooler than M-type stars were established, reclassifying GD 165 B as L4.
Physical properties
GD 165 A is a pulsating white dwarf with a temperature of about 12,100 K, a mass of 0.64 M☉, and a radius of 0.0124 R☉. GD 165 A has an extremely dim luminosity of 0.0030L☉, making it completely invisible to the naked eye.
GD 165 B is an L-Type brown dwarf with a temperature of about 1,750 K, a mass of about 63 MJ, and a radius of 1.00 RJ. GD 165B is separated by 123±12 astronomical units from its host white dwarf. It is the second closest spacially resolved brown dwarf after PHL 5038, which has a separation of around 69 AU. It produces almost no light and is completely invisible to the naked eye.
See also
Other cooler than M brown dwarfs, discovered before 1998:
- Gliese 229 B - T6.5
- 2MASP J0345432+254023 - L0 (first isolated L-dwarf)
- DENIS-P J020529.0-115925 - L7
- DENIS-P J1058.7-1548 - L3
- DENIS-P J1228.2-1547 - L5
- Kelu-1 - L2
References
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