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PSO J318.5−22

PSO J318.5−22

PSO J318.5-22 (red object) imaged by the Pan-STARRS PS1 telescope in 2013
Discovery
Discovery site	Pan-STARRS PS1 telescope, Haleakalā
Discovery date	2013
Detection method	Direct imaging
Designations
Alternative names	2MASS J21140802-2251358, PSO J318.5338-22.8603, TIC 24266526, WISE J211408.13-225137.3
Physical characteristics
Mean radius	1.38±0.02 RJ[1][2]
Mass	6.92±0.68 MJ[1][2]
Sidereal rotation period	8.6±0.1 h[3]
Axial tilt	56.2±8.1° (to plane of sky)[3]
Temperature	1275 K[4]
Spectral type	L7

PSO J318.5−22 is a rogue planet, an extrasolar objectofplanetary mass that does not orbit a parent star.^[5][6] It is approximately 80 light-years away and belongs to the Beta Pictoris moving group.^[7] The object was discovered in 2013 in images taken by the Pan-STARRS PS1 wide-field telescope. PSO J318.5-22's age is inferred to be 12 million years, the same age as the Beta Pictoris group.^[8] Based on its calculated temperature and age, it is classified under the brown dwarf spectral type L7.^[9]

The team leader, Michael Liu of the Institute for Astronomy at the University of Hawaii, stated, "We have never before seen an object free-floating in space that looks like this. It has all the characteristics of young planets found around other stars, but it is drifting out there all alone."^[10] Current theories about such objects include the possibility that gravitational perturbations may have kicked them out of their planetary systems soon after they formed through planetary accretion, or they may have been formed by some other means.^[11] Estimated temperatures inside its clouds exceed 1,100 K (800 °C). The clouds, made of hot dust and molten iron, show how widespread clouds are in planets and planet-like objects.^[12] However, by 2020, modeling showed that the brightness variability could not be unambiguously attributed to clouds.^[4]

See also[edit]

• CFBDSIR 2149−0403
• 2MASS J1119–1137
• Jupiter
• Kepler-22b

References[edit]