Temperature
5325 K
5272.3 to 5718
G9 V • 74.80 pc
Records
6
literature rows
Planets
2
system count
References
6
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: Carleo et al. 2020 • System source: TICv8
Temperature
5325 K
5272.3 to 5718
Mass
0.85 Msun
0.83 to 0.92
Radius
0.87 Rsun
0.86 to 0.88
Age
9.40 Gyr
9.40 to 10.90
Distance
74.80 pc
single adopted value
Spectral Type
G9 V
Consistent across records
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.87 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
TOI-421
0.87 R☉
System Layout
2 planets linked to this host
TOI-421 is a star system 244 light-years away. Its host star is a G9 V dwarf, a Sun-like class of main-sequence star, with a reported mass of 0.852 solar masses, a radius of 0.871 solar radii, a temperature of 5330 K, and an age of 9.4 billion years. The star's reported mass and radius estimates are both smaller than the Sun's, and its reported temperature is cooler than the Sun's. Two planets orbit this host.
TOI-421 b is a Neptune-like world discovered in 2020 by the transit method. It has a mass of 6.7 Earth masses, a radius of 2.64 Earth radii, and an orbital period of 5.2 days. Its reported radius and mass estimates are both larger than Earth's, and its mean density is 2.01 g/cm³, 0.364 times Earth's. Among the listed planets, TOI-421 b has the shortest year by reported estimates and the smallest radius and reported mass.
TOI-421 c is a Jupiter-like world, also discovered in 2020 by the transit method. It has a mass of 14.1 Earth masses, a radius of 5.09 Earth radii, and an orbital period of 16.1 days. Its reported radius and mass estimates are larger than Earth's, and its mean density is 0.589 g/cm³, 0.107 times Earth's. Among the listed planets, TOI-421 c has the longest year by reported estimates and the largest radius and reported mass.
A transit occurs when a planet crosses in front of its star from our viewpoint, dimming the observed light; repeated dips help establish these orbital periods.
Provenance
Evidence Summary
Rows
6
Stellar refs
5
System refs
1