OGLE-2005-BLG-169Lb

OGLE-2005-BLG-169Lb
Discovery
Discovered byMicroFUN,
PLANET/RoboNet, OGLE
Discovery date10 March 2006
Gravitational microlensing
Orbital characteristics
StarOGLE-2005-BLG-169L
Physical characteristics
Mass13.2±1.3 M🜨[1]
Temperature~70 K

OGLE-2005-BLG-169Lb is an extrasolar planet located approximately 2,700 parsecs (8,800 light-years) away in the constellation of Sagittarius, orbiting the star OGLE-2005-BLG-169L. This planet was discovered by the OGLE project using the gravitational microlensing method. Based on a most likely mass for the host star of 0.49 solar mass (Mβ˜‰), the planet has a mass of 13 times that of Earth (M🜨). Its mass and estimated temperature are close to those of Uranus. It is speculated that this planet may either be an ice giant like Uranus, or a "naked super-Earth" with a solid icy or rocky surface.[2][3]

See also

How a star can magnify and brighten the light of a background star when it passes in front of the distant star.[4]

References

  1. ↑ Batista, V.; et al. (July 30, 2015). "CONFIRMATION OF THE OGLE-2005-BLG-169 PLANET SIGNATURE AND ITS CHARACTERISTICS WITH LENS–SOURCE PROPER MOTION DETECTION". The Astrophysical Journal. 808 (2): 170. arXiv:1507.08914. Bibcode:2015ApJ...808..170B. doi:10.1088/0004-637X/808/2/170. S2CID 119212954.
  2. ↑ Gould, A.; Udalski, A.; et al. (May 24, 2006). "Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common". The Astrophysical Journal. 644 (1): L37. arXiv:astro-ph/0603276. Bibcode:2006ApJ...644L..37G. doi:10.1086/505421. S2CID 14270439.
  3. ↑ Quick, Lynnae C.; Roberge, Aki.; Mendoza, Guadalupe Tovar; Quintana, Elisa V.; Youngblood, Allison A. (4 October 2023). "Prospects for Cryovolcanic Activity on Cold Ocean Planets". The Astrophysical Journal. 956 (29): 29. Bibcode:2023ApJ...956...29Q. doi:10.3847/1538-4357/ace9b6.
  4. ↑ "Identifying Planets". Retrieved 3 August 2015.