Temperature
5725 K
5638.8 to 5760
G3 V • 114.3 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: Luque et al. 2019 • System source: TICv8
Temperature
5725 K
5638.8 to 5760
Mass
1 Msun
1 to 1.03
Radius
1.09 Rsun
1.09 to 1.17
Age
6.80 Gyr
single adopted value
Distance
114.3 pc
single adopted value
Spectral Type
G3 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.09 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
K2-292
1.09 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2019
Period
16.98 days
Radius
2.63 R⊕
Mass
24.50 M⊕
Eq. Temp
795 K
K2-292 is a G3 V star located 373 light-years away, and it hosts one known planet. The star is a main-sequence dwarf with a spectral class similar to the Sun's. It is estimated to be 6.8 billion years old, with a mass of 1 solar masses, a radius of 1.09 solar radii, and a temperature of 5730 K. Its reported radius estimate is larger than the Sun's.
The planet K2-292 b was discovered in 2019 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. It is classified as Neptune-like, a size class for planets reaching up to 4 times Earth's radius. K2-292 b has an orbital period of 17 days, a mass of 24.5 Earth masses, and a radius of 2.63 Earth radii. Its reported mass and radius estimates are both larger than Earth's. Its mean density is 7.42 g/cm³, 1.35 times Earth's.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1