OGLE-TR-132

Star in the constellation Carina From Wikipedia, the free encyclopedia

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,[3] it is slightly hotter and more luminous than the Sun.

Quick facts Constellation, Right ascension ...
OGLE-TR-132

Light curve showing the March 11, 2009 planet transit across OGLE-TR-132
Credit: Adapted from Adams et al. (2011)[1]
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Carina[2]
Right ascension 10h 50m 34.59s[3]
Declination −61° 57 26.1[3]
Apparent magnitude (V) 15.72[2]
Characteristics
Evolutionary stage subgiant[3]
Spectral type F[4]
Astrometry
Proper motion (μ) RA: −5.463[3] mas/yr
Dec.: +3.058[3] mas/yr
Parallax (π)0.4290±0.0450 mas[3]
Distanceapprox. 7,600 ly
(approx. 2,300 pc)
Details
Mass1.19[5] M
Radius1.23[5] R
Luminosity2.04[5] L
Surface gravity (log g)4.33[5] cgs
Temperature6,210[5] K
Age7.4[3] Gyr
Other designations
V742 Carinae, TIC 465144510[6]
Database references
SIMBADdata
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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.[2] 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.[4]

More information Companion (in order from star), Mass ...
The OGLE-TR-132 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b 1.14 ± 0.12 MJ 0.0306 ± 0.0008 1.689868 ± 0.000003 0 1.15+0.80
−0.13
[4] RJ
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See also

References

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