Cha 110913-773444

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Cha 110913-773444

Cha 110913-773444 (middle) compared to the Sun (left) and Jupiter (right)
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Chamaeleon
Right ascension 11h 09m 13.63s
Declination -77° 34' 44.6"
Apparent magnitude (V) +21.59
Characteristics
Spectral type L-dwarf
U-B color index ?
B-V color index ?
Variable type ?
Astrometry
Radial velocity (Rv) ? km/s
Proper motion (μ) RA: ? mas/yr
Dec.: ? mas/yr
Parallax (π) ? ± ? mas
Distance 163 ly (50 pc)
Absolute magnitude (MV) +18.1
Details
Mass 8 (+7 to -3) MJ, 0.008 M
Radius 1.8 RJ, 0.18 R
Luminosity 0.000096 L
Temperature 1,350 K
Metallicity ?
Rotation ?
Age 0.5–10 x 106 years
Database references
SIMBAD data

Cha 110913-773444 (sometimes abbreviated Cha 110913) is an astronomical object surrounded by what appears to be a protoplanetary disk. There is no consensus yet among scientists whether to classify the object as a Sub-brown dwarf (with planets) or a rogue planet (with moons). It is even smaller than OTS 44 which had been the smallest known brown dwarf prior to the discovery of Cha 110913-773444.

Cha 110913-773444 was discovered by Kevin Luhman and others at Pennsylvania State University using the Spitzer Space Telescope and the Hubble Space Telescope, as well as two earthbound telescopes in Chile.

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