Temperature
6149 K
5748 to 6149
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Stellar HostProfile
HATS-36
G0 V • 856.4 pc
Records
7
literature rows
Planets
1
system count
References
8
distinct source labels
TIC: TIC 119262291
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Bayliss et al. 2018 • System source: TICv8
Mass
1.22 Msun
1.06 to 1.22
Radius
1.16 Rsun
1.09 to 1.16
Age
0.62 Gyr
single adopted value
Luminosity
0.21 log(Lsun)
0.07 to 0.21
Distance
856.4 pc
single adopted value
Spectral Type
G0 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.16 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HATS-36
1.16 R☉
System Layout
Known planets
1 planets linked to this host
HATS-36 b
Transit
◌
Discovery
2018
Period
4.18 days
Radius
12.92 R⊕
Mass
—
Eq. Temp
1203 K
HATS-36 and Its Jupiter-like Planet
HATS-36 is a G0 V star located 2790 light-years away. Its spectral type marks it as a Sun-like, main-sequence dwarf. Its age is 0.62 billion years. Its reported mass estimate is 1.22 solar masses, larger than the Sun's, and its reported radius estimate is 1.16 solar radii, also larger than the Sun's. The star's reported temperature of 6150 K is hotter than the Sun's. One planet is known to orbit this star.
HATS-36 b is a Jupiter-like planet discovered in 2018 by the transit method, in which a planet passing in front of its star from our viewpoint causes a small dip in observed brightness, and repeated dips help establish orbital periods. It orbits every 4.18 days and has a radius of 12.9 Earth radii, which is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
7
Stellar refs
7
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | 1.15 | — | — | — | 856.4 | Petigura et al. 2018 | TICv8 |
| 5859 | 1.06 | 1.09 | — | 0.10 | — | 856.4 | TICv8 | TICv8 |
| — | — | 1.09 | — | — | — | 856.4 | Kruse et al. 2019 | TICv8 |
| 5950 | 1.10 | 1.10 | — | — | — | 856.4 | Livingston et al. 2018 | TICv8 |
| 6149 | 1.22 | 1.16 | 0.62 | 0.21 | G0 V | 856.4 | Bayliss et al. 2018 | TICv8 |
| 5748 | — | 1.09 | — | 0.07 | — | 856.4 | Gaia DR2 | TICv8 |
| 5859 | — | 1.09 | — | — | — | 856.4 | ExoFOP | TICv8 |