OGLE 2003-BLG-235L
Sign in to saveAlso known as MOA 2003-BLG-53
OGLE-2003-BLG-235L (MOA-2003-BLG-53L) is a star in the constellation of Sagittarius. The first gravitational microlensing event for which a planet orbiting the lens was detected around this star. The event occurred in during July 2003. Two groups observed and independently detected the event: the Optical Gravitational Lensing Experiment (OGLE) and the Microlensing Observations in Astrophysics (MOA), hence, the double designation. It is an orange dwarf star of spectral type K, which is accompanied by a giant planet.
Astronomical data · SIMBAD
- Object type
- *
- Spectral type
- GIV
- Coordinates
- RA 271.3181° · Dec -28.8950°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Instance of
- star
- Constellation
- Sagittarius
- Child body
- OGLE-2003-BLG-235Lb
- Distance from Earth
- 5260
- Mass
- 0.56
Show 5 more facts
- right ascension
- 271.318125
- declination
- -28.895000
- epoch
- J2000.0
- spectral class
- GIV
- catalog code
- OGLE-2003-BLG-235
Sources (1)
via Wikidata · CC0
~2 min read
Encyclopedic overview
5 sectionsContents
- Lens system
- Planetary system
- See also
- References
- External links
OGLE-2003-BLG-235L (MOA-2003-BLG-53L) is a star in the constellation of Sagittarius. The first gravitational microlensing event for which a planet orbiting the lens was detected around this star. The event occurred in during July 2003. Two groups observed and independently detected the event: the Optical Gravitational Lensing Experiment (OGLE) and the Microlensing Observations in Astrophysics (MOA), hence, the double designation. It is an orange dwarf star of spectral type K, which is accompanied by a giant planet.
==Lens system== OGLE-2003-BLG-235L and MOA-2003-BLG-53L is the designation given to the star in the lens system. In 2004, analysis of the light curve produced as it passed in front of the source star allowed detection of an exoplanet orbiting the star with a mass 0.0039 times that of the host star (this would put it in the jovian mass range). The star was originally assumed to be a red dwarf star, since they are the most common type of star in the galaxy.
Excerpted from Wikipedia’s “OGLE 2003-BLG-235L” article, available under the CC BY-SA 4.0 licence.