Temperature
5445 K
5359.0 to 5445
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Stellar HostProfile
TOI-6041
G7 • 72.47 pc
Records
3
literature rows
Planets
2
system count
References
4
distinct source labels
TIC: TIC 192415680
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: Heidari et al. 2026 • System source: TICv8
Mass
0.89 Msun
0.89 to 0.93
Radius
0.88 Rsun
0.85 to 0.88
Age
7.90 Gyr
single adopted value
Luminosity
-0.21 log(Lsun)
-0.28 to -0.21
Distance
72.47 pc
single adopted value
Spectral Type
G7
Consistent across records
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.88 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-6041
0.88 R☉
System Layout
Known planets
2 planets linked to this host
TOI-6041 b
Transit
◌
Discovery
2025
Period
26.05 days
Radius
4.55 R⊕
Mass
28.90 M⊕
Eq. Temp
605.6 K
TOI-6041 c
Radial Velocity
◌
Discovery
2025
Period
88 days
Radius
—
Mass
77.90 M⊕
Eq. Temp
403.5 K
TOI-6041: A Sun-Like Star With Two Known Planets
TOI-6041 is a G7 star 236 light-years away. It is estimated to be 7.9 billion years old, with a reported mass of 0.885 solar masses and a radius of 0.879 solar radii. Its temperature of 5450 K is cooler than the Sun's. Two planets are known to orbit this star.
TOI-6041 b was discovered by the transit method in 2025. It is a Jupiter-like planet with a reported radius of 4.55 Earth radii, larger than Earth's. Its mass is reported as an upper limit of 28.9 Earth masses, and its orbital period is 26 days, the shortest year among the listed planets. TOI-6041 c was found by radial velocity, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. Its minimum mass is 77.9 Earth masses, larger than Earth's, and its orbital period is 88 days, the longest year among the listed planets.
The star's reported mass and radius estimates are both smaller than the Sun's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
3
Stellar refs
3
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable