Temperature
5185 K
5084 to 5224
K • 134.6 pc
Records
15
literature rows
Planets
1
system count
References
15
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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. 2007 • System source: TICv8
Temperature
5185 K
5084 to 5224
Mass
0.94 Msun
0.89 to 1.06
Radius
0.82 Rsun
0.80 to 0.87
Age
0.40 Gyr
0.40 to 7.50
Luminosity
-0.35 log(Lsun)
-0.36 to -0.34
Distance
134.6 pc
single adopted value
Spectral Type
K
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.82 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HAT-P-3
0.82 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2007
Period
2.90 days
Radius
10.54 R⊕
Mass
206.6 M⊕
Eq. Temp
—
HAT-P-3 is a K-type star located 439 light-years away. Its reported mass estimate is 0.936 solar masses and its reported radius estimate is 0.824 solar radii, both smaller than the Sun's. The star's reported temperature is 5190 K, cooler than the Sun's, and its age is 0.4 billion years. One planet orbits this host.
That planet is HAT-P-3 b, a Jupiter-like world discovered in 2007 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. It has a mass of 207 Earth masses and a radius of 10.5 Earth radii, both larger than Earth's. Its orbital period is 2.9 days, and its mean density is 0.973 g/cm³, 0.177 times Earth's.
Provenance
Evidence Summary
Rows
15
Stellar refs
14
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5185 | 0.93 | 0.83 | 1.50 | -0.35 | — | 134.6 | Torres et al. 2008 | TICv8 |
| 5224 | — | 0.82 | — | — | — | 134.6 | ExoFOP | TICv8 |
| 5185 | 0.93 | 0.83 | 1.50 | — | — | 134.6 | Bonomo et al. 2017 | TICv8 |
| 5190 | 0.93 | 0.85 | 2.90 | — | — | 134.6 | Mancini et al. 2018 | TICv8 |
| 5185 | 0.94 | 0.82 | 0.40 | -0.35 | K | 134.6 | Torres et al. 2007 | TICv8 |
| 5190 | — | 0.85 | 2.90 | — | K1 | 134.6 | Bourrier et al. 2023 | TICv8 |
| 5185 | — | — | — | — | — | 134.6 | Nascimbeni et al. 2011 | TICv8 |
| 5185 | 1.06 | 0.87 | — | — | — | 134.6 | Stassun et al. 2017 | TICv8 |
| 5224 | 0.89 | 0.82 | — | -0.34 | — | 134.6 | TICv8 | TICv8 |
| — | — | 0.83 | — | — | — | 134.6 | Gibson et al. 2010 | TICv8 |
| 5185 | 0.92 | 0.80 | 1.60 | -0.36 | — | 134.6 | Chan et al. 2011 | TICv8 |
| 5093.7 | — | 0.86 | — | -0.34 | — | 134.6 | Gaia DR2 | TICv8 |
| 5185 | 0.90 | 0.87 | 7.50 | — | — | 134.6 | Southworth 2012 | TICv8 |
| — | — | — | — | — | K1 V | 134.6 | Torres et al. 2007 | TICv8 |
| 5084 | 0.92 | 0.80 | 1.60 | -0.36 | K | 134.6 | Ment et al. 2018 | TICv8 |