Temperature
6290 K
6290 to 6414
F8 • 127.8 pc
Records
18
literature rows
Planets
2
system count
References
19
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: Bakos et al. 2007 • System source: TICv8
Temperature
6290 K
6290 to 6414
Mass
1.30 Msun
1.28 to 1.93
Radius
1.47 Rsun
1.39 to 1.73
Age
2.60 Gyr
0.40 to 2.60
Luminosity
0.48 log(Lsun)
0.48 to 0.65
Distance
127.8 pc
single adopted value
Spectral Type
F8
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.47 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HAT-P-2
1.47 R☉
System Layout
2 planets linked to this host
HAT-P-2 is an F8 star located 417 light-years away. The star is 2.6 billion years old and has a mass of 1.3 solar masses, a radius of 1.47 solar radii, and a temperature of 6290 K. Its reported mass and radius are larger than the Sun's, and it is hotter than the Sun. Two planets are known to orbit this host.
HAT-P-2 b was discovered in 2007 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. The planet has a minimum mass of 2740 Earth masses, roughly 8.62 times Jupiter's mass, and an orbital period of 5.63 days - the shortest year among the listed planets.
HAT-P-2 c was discovered in 2023 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. It has a mass of 3400 Earth masses, roughly 10.7 times Jupiter's mass, and an orbital period of 8500 days - the longest year among the listed planets.
Provenance
Evidence Summary
Rows
18
Stellar refs
18
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6412 | 1.93 | 1.71 | — | — | — | 127.8 | Stassun et al. 2017 | TICv8 |
| 6290 | 1.36 | 1.64 | 2.60 | 0.58 | — | 127.8 | Pal et al. 2010 | TICv8 |
| 6290 | 1.31 | 1.51 | 2.60 | 0.51 | — | 127.8 | Torres et al. 2008 | TICv8 |
| 6338.4 | — | 1.73 | — | 0.64 | — | 127.8 | Gaia DR2 | TICv8 |
| 6290 | 1.28 | 1.68 | 2.60 | — | — | 127.8 | Southworth 2010 | TICv8 |
| 6290 | 1.36 | 1.64 | 2.60 | — | — | 127.8 | Bonomo et al. 2017 | TICv8 |
| — | 1.36 | — | — | — | — | 127.8 | Knutson et al. 2014 | TICv8 |
| 6412.8 | 1.29 | 1.70 | — | 0.65 | — | 127.8 | TICv8 | TICv8 |
| 6414 | 1.34 | 1.54 | — | — | — | 127.8 | Tsantaki et al. 2014 | TICv8 |
| — | — | — | — | — | — | 127.8 | de Wit et al. 2017 | TICv8 |
| — | — | — | — | — | F8 | 127.8 | Cannon & Pickering 1918 | TICv8 |
| — | 1.33 | — | — | — | — | 127.8 | de Beurs et al. 2023 | TICv8 |
| 6290 | 1.30 | 1.47 | 2.60 | 0.48 | F8 | 127.8 | Bakos et al. 2007 | TICv8 |
| 6300 | — | — | 0.40 | — | F8 V | 127.8 | Salz et al. 2015 | TICv8 |
| 6412.8 | — | 1.70 | — | — | — | 127.8 | ExoFOP | TICv8 |
| — | 1.30 | 1.42 | — | — | — | 127.8 | Loeillet et al. 2008 | TICv8 |
| — | — | — | — | — | — | 127.8 | Garai et al. 2017 | TICv8 |
| 6380 | 1.33 | 1.39 | 1.44 | 0.53 | F8 | 127.8 | Ment et al. 2018 | TICv8 |