Temperature
5543 K
5374 to 5826
Unclassified star • 1238.8 pc
Records
22
literature rows
Planets
2
system count
References
16
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
5543 K
5374 to 5826
Mass
0.90 Msun
0.89 to 0.98
Radius
0.86 Rsun
0.54 to 1.24
Age
4.17 Gyr
0.40 to 4.90
Distance
1238.8 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.86 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-375
0.86 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
12.13 days
Radius
1.45 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
19.99 days
Radius
2.65 R⊕
Mass
—
Eq. Temp
—
Kepler-375 is a star 4040 light-years away with two known planets. The host star is estimated to be 4.17 billion years old, with a mass of 0.9 solar masses and a radius of 0.86 solar radii. Its temperature is 5540 K. The star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
Both planets were discovered by transit in 2014. Kepler-375 b is classified as Earth-like, with a radius of 1.45 Earth radii and an orbital period of 12.1 days. Kepler-375 c is classified as Neptune-like, with a radius of 2.65 Earth radii and an orbital period of 20 days. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods. Among the listed planets, Kepler-375 b has the shortest year and the smallest radius by reported estimates, while Kepler-375 c has the longest year and the largest radius by reported estimates. Kepler-375 c's reported radius estimate is larger than Earth's.
Provenance
Evidence Summary
Rows
22
Stellar refs
15
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 1238.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5615 | — | 0.54 | — | — | — | 1238.8 | Latham et al. 2005 | TICv8 |
| 5615 | — | 0.78 | — | — | — | 1238.8 | Q1-Q6 KOI Table | TICv8 |
| 5821 | 0.94 | 0.85 | — | — | — | 1238.8 | Q1-Q12 KOI Table | TICv8 |
| 5500 | 0.92 | 1.24 | — | — | — | 1238.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5826 | — | 0.84 | — | — | — | 1238.8 | Rowe et al. 2014 | TICv8 |
| 5826 | 0.98 | 0.88 | 0.40 | — | — | 1238.8 | Q1-Q8 KOI Table | TICv8 |
| 5543 | 0.90 | 0.86 | 4.17 | — | — | 1238.8 | Morton et al. 2016 | TICv8 |
| 5821 | 0.94 | 0.85 | — | — | — | 1238.8 | Q1-Q12 KOI Table | TICv8 |
| 5821 | 0.94 | 0.85 | — | — | — | 1238.8 | Q1-Q16 KOI Table | TICv8 |
| 5500 | 0.92 | 1.24 | — | — | — | 1238.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5615 | — | 0.78 | — | — | — | 1238.8 | Q1-Q6 KOI Table | TICv8 |
| 5483 | — | 0.90 | — | — | — | 1238.8 | Berger et al. 2018 | TICv8 |
| 5821 | 0.94 | 0.85 | — | — | — | 1238.8 | Q1-Q16 KOI Table | TICv8 |
| 5821 | 0.94 | 0.85 | — | — | — | 1238.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5483 | 0.89 | 0.87 | 4.90 | — | — | 1238.8 | Fulton & Petigura 2018 | TICv8 |
| — | — | — | — | — | — | 1238.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5374 | — | 0.95 | — | -0.17 | — | 1238.8 | Gaia DR2 | TICv8 |
| 5826 | 0.98 | 0.88 | 0.40 | — | — | 1238.8 | Q1-Q8 KOI Table | TICv8 |
| 5821 | 0.94 | 0.85 | — | — | — | 1238.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5615 | 0.89 | 0.78 | — | — | — | 1238.8 | Batalha et al. 2013 | TICv8 |
| 5499 | 0.96 | 0.91 | — | -0.16 | — | 1238.8 | TICv8 | TICv8 |