Temperature
4985 K
4944 to 5073.2
K2 • 240.7 pc
Records
5
literature rows
Planets
1
system count
References
6
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. 2015 • System source: TICv8
Temperature
4985 K
4944 to 5073.2
Mass
0.85 Msun
0.82 to 0.85
Radius
0.81 Rsun
0.69 to 0.81
Age
7.80 Gyr
single adopted value
Luminosity
-0.43 log(Lsun)
-0.54 to -0.43
Distance
240.7 pc
single adopted value
Spectral Type
K2
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.81 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HATS-7
0.81 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2015
Period
3.19 days
Radius
6.31 R⊕
Mass
38.14 M⊕
Eq. Temp
1084 K
HATS-7 is a K2 star located 785 light-years away, with a mass of 0.849 solar masses and a radius of 0.815 solar radii. Its temperature is 4990 K, and it is 7.8 billion years old. This system hosts one known planet.
That planet is HATS-7 b, a Jupiter-like world discovered by the transit method in 2015. It has a mass of 38.1 Earth masses and a radius of 6.31 Earth radii, orbiting its star every 3.19 days. Its mean density is 0.836 g/cm³, which is 0.152 times Earth's. The star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
Provenance
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4944 | — | 0.78 | — | — | — | 240.7 | ExoFOP | TICv8 |
| 5073.2 | — | 0.69 | — | -0.54 | — | 240.7 | Gaia DR2 | TICv8 |
| 4964.9 | 0.82 | 0.78 | — | -0.48 | — | 240.7 | TICv8 | TICv8 |
| 4985 | 0.85 | 0.81 | 7.80 | — | — | 240.7 | Bonomo et al. 2017 | TICv8 |
| 4985 | 0.85 | 0.81 | 7.80 | -0.43 | K2 | 240.7 | Bakos et al. 2015 | TICv8 |