Temperature
6346 K
5931.2 to 6346
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Stellar HostProfile
HATS-24
F V • 494.2 pc
Records
6
literature rows
Planets
1
system count
References
7
distinct source labels
TIC: TIC 380589029
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: Bento et al. 2017 • System source: TICv8
Mass
1.21 Msun
1.07 to 1.22
Radius
1.17 Rsun
1.12 to 1.19
Age
0.88 Gyr
0.88 to 3.70
Luminosity
0.29 log(Lsun)
0.19 to 0.29
Distance
494.2 pc
single adopted value
Spectral Type
F V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.17 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
HATS-24
1.17 R☉
System Layout
Known planets
1 planets linked to this host
HATS-24 b
Transit
◌
Discovery
2017
Period
1.35 days
Radius
15.64 R⊕
Mass
718.3 M⊕
Eq. Temp
2166 K
HATS-24 b: A Close-Orbiting Giant Around an F-Type Star
HATS-24 is a single star located 1610 light-years away. It is an F V star, a class hotter than the Sun, with a temperature of 6350 K, a mass of 1.21 solar masses, and a radius of 1.17 solar radii. Its age is 0.88 billion years. The star is orbited by one planet, HATS-24 b.
HATS-24 b is a Jupiter-like planet, a class that exceeds four times Earth's radius, and it was discovered in 2017 by the transit method, in which a planet passes in front of its star and causes a small dip in observed brightness. Its radius is 15.6 Earth radii, larger than Earth's, and its mass is 718 Earth masses, also larger than Earth's and roughly 2.26 times Jupiter's mass. Its mean density is 1.04 g/cm³, 0.188 times Earth's. The planet completes an orbit in 1.35 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
6
Stellar refs
6
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 |
|---|---|---|---|---|---|---|---|---|
| 6346 | 1.21 | 1.17 | 0.88 | 0.29 | F V | 494.2 | Bento et al. 2017 | TICv8 |
| 5931.2 | — | 1.18 | — | 0.19 | — | 494.2 | Gaia DR2 | TICv8 |
| 6346 | — | 1.15 | — | — | — | 494.2 | ExoFOP | TICv8 |
| 6125 | 1.07 | 1.12 | 3.70 | 0.19 | — | 494.2 | Oliveira et al. 2019 | TICv8 |
| 6185 | 1.18 | 1.15 | — | 0.24 | — | 494.2 | TICv8 | TICv8 |
| 6346 | 1.22 | 1.19 | — | — | — | 494.2 | Gajdoš et al. 2021 | TICv8 |