UGPS J072227.51−054031.2
Appearance
Coordinates: 07h 22m 27.29s, −05° 40′ 30.0″
Observation data J2000.0 Equinox J2000.0
| |
---|---|
Constellation | Monoceros
|
Right ascension | 07h 22m 27.29s[1] |
Declination | −05° 40′ 30.0″[2] |
Characteristics | |
Spectral type | T9[2] |
Apparent magnitude (i (AB SDSS)) | 24.32 ± 0.12[3] |
Apparent magnitude (z) | 20.51 ± 0.09[1][4] |
Apparent magnitude (Y) | 17.37 ± 0.02[1] |
Apparent magnitude (J) | 16.52 ± 0.02[1] |
Apparent magnitude (H) | 16.90 ± 0.02[1] |
Apparent magnitude (K) | 17.07 ± 0.08[1] |
Apparent magnitude (L') | 13.4 ± 0.3[1] |
Apparent magnitude (N) | 10.28 ± 0.24[1] |
Details | |
Gyr | |
Other designations | |
Database references | |
SIMBAD | data |
Monoceros |
UGPS J072227.51−054031.2 (designation often abbreviated to UGPS 0722−05) is a brown dwarf of late T type, or possibly a rogue planet located approximately 4.1 parsecs (13 light-years) from Earth.[3]
History of observations
Discovery
The
milliarcseconds. The object was initially reported to be at an even closer distance of 2.9 parsecs, which would have placed it among the ten nearest stars to the Sun[8] but later measurements revealed that the object was in fact located at a greater distance than initially thought, at 4.1+0.6
−0.5 parsecs.[1]
−0.5 parsecs.[1]
Space motion
UGPS 0722−05 has proper motion of about 970 milliarcseconds per year.[3]
Radial velocity of UGPS 0722-05, measured by Bochanski et al. and published in 2011, is 46.9 ± 2.5 km/s.[4][~ 1]
Properties
The object is roughly the volume of Jupiter, but is estimated to have 5–40 Jupiter masses (MJ).[1] This would make it less massive than ε Indi Ba. Planets have a mass of less than about 13 Jupiter masses. Infrared spectra shows the object contains water vapor and methane and has a surface temperature of approximately 480–560 kelvins.[1]
Notes
- ^ Positive value of radial velocity indicates that UGPS 0722−05 currently moves away from us. A significant excess of radial velocity (46.9 km/s) over tangential velocity (19 km/s) indicates that UGPS 0722-05 was much closer to us in past (assuming proper motion and parallax from Leggett et al. (2012), minimal distance from Solar system to UGPS 0722-05 was 5.0 ly about 72000 BC, and probably it was one of the nearest Solar neighbors at the time).
References
- ^ S2CID 16032606.
- ^ S2CID 286881.
- ^ S2CID 14171934.
- ^ S2CID 39168611.
- ^ S2CID 30379513.
- S2CID 16850733.
- doi:10.1051/0004-6361/202244250. Catalogue can be accessed here.
- arXiv:1004.0317v1 [astro-ph.SR].
External links