Temperature
6210 K
6210 to 6411
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Stellar HostProfile
OGLE-TR-132
Unclassified star • 2012.6 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 465144510
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Torres et al. 2008 • System source: TICv8
Mass
1.30 Msun
1.19 to 1.35
Radius
1.32 Rsun
1.04 to 1.43
Age
1.20 Gyr
0.70 to 1.70
Luminosity
0.37 log(Lsun)
0.31 to 0.37
Distance
2012.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.32 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
OGLE-TR-132
1.32 R☉
System Layout
Known planets
1 planets linked to this host
OGLE-TR-132 b
Transit
◌
Discovery
2004
Period
1.69 days
Radius
13.45 R⊕
Mass
375.0 M⊕
Eq. Temp
2013 K
OGLE-TR-132 and Its Jupiter-Like Planet
OGLE-TR-132 is a star 6560 light-years away with a spectral type of F5 V, a main-sequence dwarf. Its mass is 1.31 solar masses, its radius is 1.32 solar radii, and its temperature is 6210 K, all estimates larger or hotter than the Sun's corresponding values. The star's age is 1.2 billion years. One planet orbits this host.
That planet is OGLE-TR-132 b, a Jupiter-like world discovered by transit in 2004, meaning it was found through the small dip in starlight it causes as it crosses in front of its star. Its mass is 375 Earth masses, and its radius is 13.5 Earth radii, both larger than Earth's. Its mass is roughly 1.18 times Jupiter's mass. Its orbital period is 1.69 days, and its mean density is 0.849 g/cm³, 0.154 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6210 | 1.30 | 1.37 | 1.50 | — | — | 2012.6 | Southworth 2010 | TICv8 |
| 6411 | 1.34 | 1.41 | — | — | — | 2012.6 | Bouchy et al. 2004 | TICv8 |
| 6411 | 1.35 | 1.43 | 0.70 | — | — | 2012.6 | Moutou et al. 2004 | TICv8 |
| 6210 | 1.30 | 1.32 | 1.20 | 0.37 | — | 2012.6 | Torres et al. 2008 | TICv8 |
| — | — | — | — | — | F5 V | 2012.6 | Santos et al. 2006 | TICv8 |
| 6210 | 1.29 | 1.34 | 1.70 | — | — | 2012.6 | Southworth 2012 | TICv8 |
| 6210 | 1.26 | 1.34 | 1.30 | — | — | 2012.6 | Gillon et al. 2007 | TICv8 |
| 6210 | 1.30 | 1.32 | 1.20 | — | — | 2012.6 | Bonomo et al. 2017 | TICv8 |
| 6210 | 1.26 | 1.04 | — | — | — | 2012.6 | Mortier et al. 2013 | TICv8 |
| 6210 | 1.19 | 1.23 | — | 0.31 | — | 2012.6 | TICv8 | TICv8 |