UGPS J072227.51−054031.2

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UGPS J072227.51−054031.2

Near-infrared discovery image of UGPS J0722-05
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]
Distance
13.4 ± 0.1 ly
(4.12 ± 0.04 pc)
Details
Gyr
Other designations
WISEPA J072227.27−054029.9[6] ,GJ 11075[7]
Database references
SIMBADdata
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]

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

  1. ^ 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

External links