Temperature
4897 K
4717 to 4988.5
Unclassified star • 426.1 pc
Records
21
literature rows
Planets
2
system count
References
15
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: Morton et al. 2016 • System source: TICv8
Temperature
4897 K
4717 to 4988.5
Mass
0.80 Msun
0.68 to 0.97
Radius
0.75 Rsun
0.67 to 1.87
Age
3.89 Gyr
3.89 to 13.90
Distance
426.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.75 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-975
0.75 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2016
Period
1.97 days
Radius
1.48 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2023
Period
5.06 days
Radius
10.69 R⊕
Mass
—
Eq. Temp
1168 K
Kepler-975 is a star located 1390 light-years away. Its reported mass estimate is smaller than the Sun's, at 0.8 solar masses, while its radius is 0.75 solar radii. The star is 3.89 billion years old and has a temperature of 4900 K, which is cooler than the Sun's. Two planets are known to orbit this host: Kepler-975 b and Kepler-975 c, both found by the transit method, in which a planet passes in front of its star and causes a small dip in observed brightness.
Kepler-975 b was discovered in 2016 and is an Earth-like planet, a size class that stays within 1.5 times Earth's radius. Its radius is 1.48 Earth radii, larger than Earth's, and it completes one orbit in 1.97 days. Among the listed planets, it has the shortest year and the smallest radius. Kepler-975 c, discovered in 2023, is Jupiter-like, a class that exceeds 4 times Earth's radius. It has a radius of 10.7 Earth radii and an orbital period of 5.06 days; among the listed planets, it has the longest year and the largest radius.
Provenance
Evidence Summary
Rows
21
Stellar refs
14
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q12 KOI Table | TICv8 |
| 4765 | 0.68 | 0.70 | 13.90 | — | — | 426.1 | Q1-Q8 KOI Table | TICv8 |
| 4783.7 | 0.77 | 0.81 | — | -0.51 | — | 426.1 | TICv8 | TICv8 |
| 4717 | — | 1.87 | — | — | — | 426.1 | Q1-Q6 KOI Table | TICv8 |
| 4801 | — | 0.80 | — | — | — | 426.1 | Berger et al. 2018 | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q16 KOI Table | TICv8 |
| 4765 | 0.68 | 0.70 | 13.90 | — | — | 426.1 | Q1-Q8 KOI Table | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q16 KOI Table | TICv8 |
| 4717 | — | 1.87 | — | — | — | 426.1 | Q1-Q6 KOI Table | TICv8 |
| 4801 | 0.84 | 0.79 | 4.90 | — | — | 426.1 | Fulton & Petigura 2018 | TICv8 |
| — | — | — | — | — | — | 426.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4717 | — | 1.71 | — | — | — | 426.1 | Latham et al. 2005 | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q12 KOI Table | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4717 | 0.97 | 1.87 | — | — | — | 426.1 | Batalha et al. 2013 | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4988.5 | — | 0.67 | — | -0.60 | — | 426.1 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 426.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4897 | 0.80 | 0.75 | 3.89 | — | — | 426.1 | Morton et al. 2016 | TICv8 |
| 4883 | 0.95 | 1.67 | — | — | — | 426.1 | Q1-Q17 DR25 KOI Table | TICv8 |