Temperature
5715 K
5708 to 5715
G3 V • 156.5 pc
Records
3
literature rows
Planets
1
system count
References
4
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Manni et al. 2025 • System source: TICv8
Temperature
5715 K
5708 to 5715
Mass
0.90 Msun
0.90 to 1.02
Radius
1.08 Rsun
1.05 to 1.08
Age
10.20 Gyr
single adopted value
Luminosity
0.05 log(Lsun)
0.02 to 0.05
Distance
156.5 pc
single adopted value
Spectral Type
G3 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.08 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-5795
1.08 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2025
Period
6.14 days
Radius
5.62 R⊕
Mass
23.66 M⊕
Eq. Temp
1136.8 K
TOI-5795 is a G-type dwarf star 511 light-years away, a Sun-like class of star that is cooler than the Sun at 5720 K. Its radius is 1.08 solar radii, making it larger than the Sun, while its mass of 0.901 solar masses is smaller. The star is also ancient, with an age of 10.2 billion years. One planet orbits this host.
That planet, TOI-5795 b, is a Jupiter-like world discovered in 2025 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Its radius is 5.62 Earth radii, larger than Earth's, and its mass is 23.7 Earth masses, also larger than Earth's. TOI-5795 b completes an orbit every 6.14 days.
The planet's mean density is 0.734 g/cm³, 0.133 times Earth's.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1