Temperature
6311 K
6311 to 6501
F6 V • 281.3 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: Psaridi et al. 2022 • System source: TICv8
Temperature
6311 K
6311 to 6501
Mass
1.35 Msun
1.33 to 1.35
Radius
1.81 Rsun
1.75 to 1.81
Age
2.60 Gyr
single adopted value
Luminosity
0.67 log(Lsun)
0.67 to 0.69
Distance
281.3 pc
single adopted value
Spectral Type
F6 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.81 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-1107
1.81 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2022
Period
4.08 days
Radius
14.57 R⊕
Mass
1064.7 M⊕
Eq. Temp
1728 K
TOI-1107 is an F6 V star located 918 light-years away. The star is 2.6 billion years old and has a mass of 1.35 solar masses, a radius of 1.81 solar radii, and a temperature of 6310 K. Its mass and radius are larger than the Sun's, and it is hotter than the Sun. An F-type star falls between the Sun's G class and the hotter A class; the trailing "V" indicates a main-sequence dwarf.
One planet is known to orbit TOI-1107. TOI-1107 b was discovered by the transit method in 2022, when the planet passed in front of its star and caused a small dip in brightness. Its radius of 14.6 Earth radii makes it a Jupiter-like planet, larger than Earth and well past the four-Earth-radii threshold for that class. It completes an orbit every 4.08 days.
TOI-1107 b has a mass of 1060 Earth masses, which is larger than Earth's and roughly 3.35 times Jupiter's mass. Its mean density is 1.9 g/cm³, 0.344 times Earth's.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1