Temperature
5620 K
5476.4 to 5620
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Stellar HostProfile
HAT-P-36
G5 V • 294.4 pc
Records
9
literature rows
Planets
1
system count
References
10
distinct source labels
TIC: TIC 373693175
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: Mancini et al. 2015 • System source: TICv8
Mass
1.03 Msun
0.78 to 1.05
Radius
1.04 Rsun
1 to 1.11
Age
4.50 Gyr
4.50 to 6.60
Distance
294.4 pc
single adopted value
Spectral Type
G5 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.04 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HAT-P-36
1.04 R☉
System Layout
Known planets
1 planets linked to this host
HAT-P-36 b
Transit
◌
Discovery
2011
Period
1.33 days
Radius
14.31 R⊕
Mass
587.4 M⊕
Eq. Temp
1781.0 K
HAT-P-36 and Its Jupiter-Like Planet
HAT-P-36 is a star 960 light-years away with a spectral type of G5 V, a G-type main-sequence dwarf. It has an age of 4.5 billion years, a mass of 1.03 solar masses, a radius of 1.04 solar radii, and a temperature of 5620 K. Its reported radius estimate is larger than the Sun's, and its reported temperature is cooler than the Sun's. One planet orbits this host.
That planet is HAT-P-36 b, a Jupiter-like world discovered by transit in 2011. It has a mass of 587 Earth masses, roughly 1.85 times Jupiter's mass, and a radius of 14.3 Earth radii. Both its reported mass estimate and its reported radius estimate are larger than Earth's. Its orbital period is 1.33 days. Its mean density is 1.1 g/cm³, 0.2 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
9
Stellar refs
9
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5476.4 | — | 1.10 | — | -9.30e-3 | — | 294.4 | Gaia DR2 | TICv8 |
| 5560 | 0.78 | 1 | — | — | — | 294.4 | Stassun et al. 2017 | TICv8 |
| 5555.1 | 0.98 | 1.07 | — | -5.58e-3 | — | 294.4 | TICv8 | TICv8 |
| 5620 | 1.03 | 1.04 | 4.50 | — | G5 V | 294.4 | Mancini et al. 2015 | TICv8 |
| 5555.1 | — | 1.07 | — | — | — | 294.4 | ExoFOP | TICv8 |
| 5560 | 1.02 | 1.10 | 6.60 | — | — | 294.4 | Bonomo et al. 2017 | TICv8 |
| 5560 | 1.02 | 1.10 | — | 0.01 | — | 294.4 | Bakos et al. 2012 | TICv8 |
| 5620 | 1.03 | 1.04 | — | — | — | 294.4 | Chakrabarty & Sengupta 2019 | TICv8 |
| 5560 | 1.05 | 1.11 | — | 0.02 | — | 294.4 | Wang et al. 2019 | TICv8 |