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OGLE-2006-BLG-109Lc

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(Redirected from OGLE-2006-BLG-109L c) Saturn-sized planet orbiting OGLE-2006-BLG-109L
OGLE-2006-BLG-109Lc
OGLE-2006-BLG-109 c's orbit compared to
Jupiter's orbit (5.2AU) in our Solar System.
Discovery
Discovered byGaudi and
Bennett et al.
Discovery date14 February 2008
Detection methodGravitational microlensing
Orbital characteristics
Semi-major axis4.5 AU
Eccentricity0.15
Orbital period (sidereal)4931 ± 1750 d
13.5 ± 4.79 y
Inclination64 ± 8
StarOGLE-2006-BLG-109L
Physical characteristics
Mean radius0.994 RJ
(11.42 R🜨) (estimate)
Mass0.27 MJ
(85.8 ME)
Temperature59 ± 7

OGLE-2006-BLG-109Lc is an extrasolar planet approximately 4,925 light-years away in the constellation of Sagittarius. The planet was detected orbiting the star OGLE-2006-BLG-109L in 2008 by a research team using Microlensing. The host star is about 50% the mass of the Sun and the planet is about 90% the mass of Saturn.

See also

References

  1. ^ "OGLE-2006-BLG-109L c". NASA Exoplanet Exploration. Retrieved January 5, 2024.
  2. "Discovery of a Jupiter/Saturn Analog in OGLE-2006-BLG-109". MicroFUN (Microlensing Follow-Up Network). Retrieved 2008-06-27.
  3. Gaudi, B. S.; et al. (2008). "Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing". Science. 319 (5865): 927–930. arXiv:0802.1920. Bibcode:2008Sci...319..927G. doi:10.1126/science.1151947. PMID 18276883. S2CID 119281787.

External links



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