Temperature
5730 K
5665 to 5730
←Back to Stellar Hosts
Stellar HostProfile
TOI-1710
G5 V • 81.23 pc
Records
6
literature rows
Planets
1
system count
References
7
distinct source labels
TIC: TIC 445805961
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: Orell-Miquel et al. 2024 • System source: TICv8
Mass
0.99 Msun
0.98 to 1.03
Radius
0.95 Rsun
0.95 to 0.98
Age
2.80 Gyr
1.50 to 4.20
Luminosity
-0.05 log(Lsun)
-0.06 to -0.05
Distance
81.23 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: 0.95 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-1710
0.95 R☉
System Layout
Known planets
1 planets linked to this host
TOI-1710 b
Transit
◌
Discovery
2022
Period
24.28 days
Radius
5.26 R⊕
Mass
13.20 M⊕
Eq. Temp
—
TOI-1710 b: A Jupiter-Like Planet Orbiting a Sun-Like Star
TOI-1710 is a G-type main-sequence dwarf located 265 light-years away, with a spectral type of G5 V. The star has a mass of 0.99 solar masses, a radius of 0.95 solar radii, and a temperature of 5730 K. Its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's. The star is estimated to be 2.8 billion years old.
One planet orbits this host: TOI-1710 b. Discovered in 2022 by the transit method, it is classified as Jupiter-like. It completes an orbit every 24.3 days. Its radius is 5.06 Earth radii, larger than Earth's, and its mass is 19.1 Earth masses, also larger than Earth's. Its mean density is 0.812 g/cm³, which is 0.147 times Earth's.
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 |
|---|---|---|---|---|---|---|---|---|
| 5665 | 0.98 | 0.97 | 4.20 | — | G5 V | 81.23 | König et al. 2022 | TICv8 |
| 5675 | 1.01 | 0.98 | — | -0.05 | — | 81.23 | TICv8 | TICv8 |
| — | — | 0.97 | 2.90 | — | — | 81.23 | Mantovan et al. 2026 | TICv8 |
| 5675 | — | 0.98 | — | — | — | 81.23 | ExoFOP | TICv8 |
| 5684 | 1.03 | 0.96 | 1.50 | -0.06 | — | 81.23 | MacDougall et al. 2023 | TICv8 |
| 5730 | 0.99 | 0.95 | 2.80 | -0.05 | G5 V | 81.23 | Orell-Miquel et al. 2024 | TICv8 |