Temperature
6366 K
6264 to 6532.2
Unclassified star • 341.1 pc
Records
25
literature rows
Planets
1
system count
References
26
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: Lund et al. 2014 • System source: TICv8
Temperature
6366 K
6264 to 6532.2
Mass
1.51 Msun
1.35 to 1.66
Radius
2 Rsun
1.81 to 2.71
Age
2.07 Gyr
1.78 to 2.40
Luminosity
0.77 log(Lsun)
0.69 to 0.81
Distance
341.1 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 2 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HAT-P-7
2 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2008
Period
2.20 days
Radius
16.93 R⊕
Mass
584.8 M⊕
Eq. Temp
—
HAT-P-7 is an F6 V star located 1110 light-years away. Its spectral type places it in the F class, hotter than the Sun's G class, and a trailing V marks it as a main-sequence dwarf. One planet orbits this host: HAT-P-7 b.
HAT-P-7 b is a Jupiter-like planet discovered by transit in 2008. That transit method detects a planet when it passes in front of its star from our viewpoint, causing a small dip in observed brightness. The planet's radius is 16.9 Earth radii, larger than Earth's, and its mass is 585 Earth masses, also larger than Earth's and roughly 1.84 times Jupiter's mass. Its mean density is 0.665 g/cm³, 0.121 times Earth's. HAT-P-7 b completes one orbit in 2.2 days.
The host star's reported mass estimate is 1.51 solar masses, larger than the Sun's, and its reported radius estimate is 2 solar radii, also larger than the Sun's. Its reported temperature is 6370 K, hotter than the Sun's, and its age is 2.07 billion years.
Provenance
Evidence Summary
Rows
25
Stellar refs
25
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6264 | 1.66 | 2.71 | 1.98 | — | — | 341.1 | Q1-Q8 KOI Table | TICv8 |
| 6532.2 | 1.35 | 1.99 | — | 0.81 | — | 341.1 | TICv8 | TICv8 |
| — | 1.35 | 1.99 | — | — | F6 V | 341.1 | Yang et al. 2025 | TICv8 |
| 6449 | 1.51 | 1.97 | 1.78 | — | — | 341.1 | Fulton & Petigura 2018 | TICv8 |
| 6350 | 1.51 | 2 | 2.07 | — | — | 341.1 | Bonomo et al. 2017 | TICv8 |
| — | — | — | — | — | — | 341.1 | Winn et al. 2009 | TICv8 |
| 6360 | 1.47 | 1.96 | 2.40 | — | — | 341.1 | Morton et al. 2016 | TICv8 |
| 6264 | — | 2.71 | — | — | — | 341.1 | Q1-Q6 KOI Table | TICv8 |
| 6350 | 1.47 | 1.84 | — | 0.69 | — | 341.1 | Pal et al. 2008 | TICv8 |
| 6532.2 | — | 1.99 | — | — | — | 341.1 | ExoFOP | TICv8 |
| 6449 | — | 1.99 | — | — | — | 341.1 | Berger et al. 2018 | TICv8 |
| 6441 | 1.47 | 1.84 | — | — | — | 341.1 | Wong et al. 2016 | TICv8 |
| 6264 | — | 2.71 | — | — | — | 341.1 | Batalha et al. 2013 | TICv8 |
| 6366 | 1.51 | 2 | 2.07 | 0.77 | — | 341.1 | Lund et al. 2014 | TICv8 |
| 6350 | 1.52 | 1.99 | — | — | — | 341.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6525 | 1.64 | 1.81 | — | — | — | 341.1 | Mortier et al. 2013 | TICv8 |
| 6350 | 1.52 | 1.99 | — | — | — | 341.1 | Q1-Q12 KOI Table | TICv8 |
| 6440 | 1.45 | 1.95 | — | — | — | 341.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | 1.36 | — | — | — | — | 341.1 | Knutson et al. 2014 | TICv8 |
| 6350 | 1.52 | 1.99 | — | — | — | 341.1 | Q1-Q16 KOI Table | TICv8 |
| 6350 | 1.51 | 1.96 | 2 | — | — | 341.1 | Southworth 2011 | TICv8 |
| 6350 | 1.47 | 1.84 | — | — | — | 341.1 | Esteves et al. 2015 | TICv8 |
| — | — | — | — | — | — | 341.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6423.8 | — | 2.01 | — | 0.79 | — | 341.1 | Gaia DR2 | TICv8 |
| 6389 | 1.56 | 2 | — | — | — | 341.1 | Stassun et al. 2017 | TICv8 |