OGLE-TR-132
Sign in to saveAlso known as V742 Carinae
thumb|left|A light curve showing the March 11, 2009 planet transit across OGLE-TR-132. Adapted from Adams et al. (2011) OGLE-TR-132 is a distant magnitude 15.72 star in the star fields of the constellation Carina. Because of its great distance, about 4,900 light-years, and location in the crowded field it was not notable in any way. Because its apparent brightness changes when one of its planets transits, the star has been given the variable star designation V742 Carinae. The spectral type of the star is type F. A yellow-white, very metal-rich subgiant, it is slightly hotter and more luminous
Astronomical data · SIMBAD
- Object type
- V*
- Spectral type
- F
- Distance
- 7,603 light-years
- Coordinates
- RA 162.6441° · Dec -61.9573°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Constellation
- Carina
- Child body
- OGLE-TR-132b
- Distance from Earth
- 2012.62
- Radius
- 1.234
- Mass
- 1.19
- Image
- Sky Field with OGLE-TR-132.jpg
Show 13 more facts
- spectral class
- F8V
- catalog code
- OGLE-TR 132
- epoch
- J2000.0
- effective temperature
- 6210
- apparent magnitude
- 16.474056
- right ascension component of proper motion
- -5.547
- metallicity
- 0.37
- parallax
- 0.429
- surface gravity
- 32000
- declination component of proper motion
- 3.058
- right ascension
- 162.64414327838
- declination
- -61.95726074723999
- Commons category
- OGLE-TR-132
Sources (1)
via Wikidata · CC0
~1 min read
Encyclopedic overview
4 sectionsContents
- Planetary system
- See also
- References
- External links
thumb|left|A light curve showing the March 11, 2009 planet transit across OGLE-TR-132. Adapted from Adams et al. (2011) OGLE-TR-132 is a distant magnitude 15.72 star in the star fields of the constellation Carina. Because of its great distance, about 4,900 light-years, and location in the crowded field it was not notable in any way. Because its apparent brightness changes when one of its planets transits, the star has been given the variable star designation V742 Carinae. The spectral type of the star is type F. A yellow-white, very metal-rich subgiant, it is slightly hotter and more luminous than the Sun.
== Planetary system == In 2003 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements were necessary to calculate the mass of the body. In 2004 the object was proved to be a new transiting extrasolar planet, OGLE-TR-132b.
Excerpted from Wikipedia’s “OGLE-TR-132” article, available under the CC BY-SA 4.0 licence.