Temperature
5304 K
5220.1 to 5304
G • 246.4 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: Zhou et al. 2014 • System source: TICv8
Temperature
5304 K
5220.1 to 5304
Mass
0.94 Msun
0.90 to 0.94
Radius
0.87 Rsun
0.87 to 0.88
Age
3.60 Gyr
single adopted value
Luminosity
-0.27 log(Lsun)
-0.28 to -0.27
Distance
246.4 pc
single adopted value
Spectral Type
G
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.87 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
HATS-5
0.87 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2014
Period
4.76 days
Radius
10.22 R⊕
Mass
75.32 M⊕
Eq. Temp
1025 K
HATS-5 is a G-type star 804 light-years away. Its mass is 0.936 solar masses and its radius is 0.871 solar radii, both smaller than the Sun's, and its temperature of 5300 K is cooler than the Sun's. It is 3.6 billion years old. One planet orbits this host.
That planet, HATS-5 b, is a Jupiter-like world discovered by the transit method in 2014. Its transit across the star's face produces a small dip in observed brightness, which can be tracked to establish the planet's period. It circles HATS-5 every 4.76 days. Its radius is 10.2 Earth radii, larger than Earth's, and its mass is 75.3 Earth masses, also larger than Earth's. Its mean density is 0.388 g/cm³, 0.0705 times Earth'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 |
|---|---|---|---|---|---|---|---|---|
| 5258 | — | 0.88 | — | — | — | 246.4 | ExoFOP | TICv8 |
| 5220.1 | — | 0.88 | — | -0.28 | — | 246.4 | Gaia DR2 | TICv8 |
| 5258 | 0.90 | 0.88 | — | -0.28 | — | 246.4 | TICv8 | TICv8 |
| 5304 | 0.94 | 0.87 | 3.60 | — | — | 246.4 | Bonomo et al. 2017 | TICv8 |
| 5304 | 0.94 | 0.87 | 3.60 | -0.27 | G | 246.4 | Zhou et al. 2014 | TICv8 |