ChaHα8

Binary brown dwarf in the constellation Chamaleon From Wikipedia, the free encyclopedia

ChaHα8

ChaHα8 (also written ChaHa8 when Greek letters are unavailable) is a binary brown dwarf about 640 light-years (200 parsecs) from Earth in the constellation Chamaeleon. The designation indicates that it is in the Chamaeleon I star-forming region and that it displays hydrogen-alpha emission. It was discovered in 2000.[5]

Quick Facts Constellation, Right ascension ...
ChaHα8
Thumb
ChaHα8 with the Spitzer Space Telescope
Observation data
Epoch J2000      Equinox J2000
Constellation Chamaeleon
Right ascension 11h 07m 46.091s[1]
Declination −77° 40 08.92[1]
Apparent magnitude (V) 20.1[2]
Characteristics
Spectral type M5.75–M6.5[3]
Astrometry
Proper motion (μ) RA: -23.455 mas/yr[1]
Dec.: 0.453 mas/yr[1]
Parallax (π)5.0899±0.0792 mas[1]
Distance641 ± 10 ly
(196 ± 3 pc)
Orbit[4]
Period (P)1895±132 d
Semi-major axis (a)1.02±0.061.17±0.07 AU
Eccentricity (e)0.59±0.22
Periastron epoch (T)2453163±214 JD
Argument of periastron (ω)
(secondary)
106±26°
Semi-amplitude (K1)
(primary)
2.433±0.44 km/s
Details
ChaHα8 A
Mass0.07–0.10[3] M
Temperature2910–3024[3] K
Rotational velocity (v sin i)15.5±2.6[3] km/s
Age~3[3] Myr
ChaHα8 B
Mass25±731±8[4] MJup
Other designations
2MASS J11074610-7740089, CHSM 10837, SBC9 3352, Cha Hα 8[2]
Database references
SIMBADdata
Close

It was found in 2007 to have a low-mass substellar companion in orbit around it via radial velocity observations.[3] The companion has a mass of 25–31 Jupiter masses, and the pair orbit each other with a period of 5.2 years and an eccentricity of 0.59.[4]

References

Loading related searches...

Wikiwand - on

Seamless Wikipedia browsing. On steroids.