OGLE-TR-132
Star in the constellation Carina
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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.
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] |
| Distance | approx. 7,600 ly (approx. 2,300 pc) |
| Details | |
| Mass | 1.19[5] M☉ |
| Radius | 1.23[5] R☉ |
| Luminosity | 2.04[5] L☉ |
| Surface gravity (log g) | 4.33[5] cgs |
| Temperature | 6,210[5] K |
| Age | 7.4[3] Gyr |
| Other designations | |
| V742 Carinae, TIC 465144510[6] | |
| Database references | |
| SIMBAD | data |
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]
| 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 |