Temperature
6075 K
4637.0 to 6220
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Stellar HostProfile
OGLE-TR-10
Unclassified star • 1345.0 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 130150682
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: Southworth 2010 • System source: TICv8
Mass
1.28 Msun
1 to 1.28
Radius
1.52 Rsun
0.97 to 1.52
Age
3.10 Gyr
3.10 to 3.20
Distance
1345.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.52 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
OGLE-TR-10
1.52 R☉
System Layout
Known planets
1 planets linked to this host
OGLE-TR-10 b
Transit
◌
Discovery
2004
Period
3.10 days
Radius
14.01 R⊕
Mass
197.0 M⊕
Eq. Temp
—
OGLE-TR-10 and Its Jupiter-Like Planet
OGLE-TR-10 is a star 4390 light-years away with a spectral type of G2 V, a Sun-like classification. It is 3.1 billion years old, has 1.28 solar masses, and has a radius of 1.52 solar radii. Its temperature is 6080 K. Its reported mass estimate is larger than the Sun's, its reported radius estimate is larger than the Sun's, and its reported temperature is hotter than the Sun's. One planet orbits this host.
That planet is OGLE-TR-10 b, a Jupiter-like world discovered by the transit method in 2004. Its mass is 197 Earth masses, and its radius is 14 Earth radii. Both its reported mass estimate and its reported radius estimate are larger than Earth's. Its mean density is 0.395 g/cm³, 0.0716 times Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. OGLE-TR-10 b completes an orbit every 3.1 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
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 |
|---|---|---|---|---|---|---|---|---|
| 5800 | 1.02 | 1.09 | — | — | — | 1345.0 | Holman et al. 2007 | TICv8 |
| 5960 | 1.10 | 1.14 | — | — | — | 1345.0 | Pont et al. 2007 | TICv8 |
| 5750 | 1 | 1 | — | — | — | 1345.0 | Konacki et al. 2005 | TICv8 |
| 4637.0 | — | 1.49 | — | -0.03 | — | 1345.0 | Gaia DR2 | TICv8 |
| 6075 | 1.17 | 1.14 | — | — | — | 1345.0 | Santos et al. 2006 | TICv8 |
| — | — | — | — | — | G2 V | 1345.0 | Dreizler et al. 2002 | TICv8 |
| 5950 | 1.14 | 1.17 | — | 0.19 | — | 1345.0 | Torres et al. 2008 | TICv8 |
| 6075 | 1.14 | 0.97 | — | — | — | 1345.0 | Mortier et al. 2013 | TICv8 |
| 6075 | 1.14 | 1.24 | — | 0.28 | — | 1345.0 | TICv8 | TICv8 |
| 6220 | 1.22 | 1.21 | — | — | — | 1345.0 | Bouchy et al. 2005 | TICv8 |
| 6075 | 1.28 | 1.52 | 3.10 | — | — | 1345.0 | Southworth 2010 | TICv8 |
| 5950 | 1.14 | 1.17 | 3.20 | — | — | 1345.0 | Bonomo et al. 2017 | TICv8 |