OGLE-2005-BLG-169Lb
Sign in to saveAlso known as NAME EWS 2005-BLG-169b
OGLE-2005-BLG-169Lb is an extrasolar planet located approximately 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 (), the planet has a mass of 13 times that of Earth (). 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.
Key facts
- Planet.name
- OGLE-2005-BLG-169Lb
- Planet.discoverer
- MicroFUN,PLANET/RoboNet, OGLE
- Planet.discovered
- 10 March 2006
- Planet.discovery_method
- Gravitational microlensing
- Planet.apsis
- astron
- Planet.star
- OGLE-2005-BLG-169L
- Planet.mass
- 13.2±1.3
- Planet.single_temperature
- ~70 K
via Wikipedia infobox
Wikidata facts
- Constellation
- Sagittarius
- Parent body
- OGLE-2005-BLG-169L
- Mass
- 0.0415
- Image
- OGLE-2005-BLG-169Lb.jpg
Show 6 more facts
- discovery method
- gravitational microlensing
- time of discovery or invention
- 2006-06-00
- epoch
- J2000.0
- right ascension
- 271.522167
- semi-major axis of an orbit
- 4
- declination
- -30.73263889
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
3 sectionsContents
- See also
- References
- External links
OGLE-2005-BLG-169Lb is an extrasolar planet located approximately 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 (), the planet has a mass of 13 times that of Earth (). 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.
==See also== thumb|How a star can magnify and brighten the light of a background star when it passes in front of the distant star. OGLE-2005-BLG-390Lb Optical Gravitational Lensing Experiment (OGLE)
Excerpted from Wikipedia’s “OGLE-2005-BLG-169Lb” article, available under the CC BY-SA 4.0 licence.