Temperature
5789 K
5604 to 6125
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Stellar HostProfile
Kepler-625
Unclassified star • 760.7 pc
Records
20
literature rows
Planets
2
system count
References
15
distinct source labels
TIC: TIC 137414304
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
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
Mass
1.04 Msun
1.00 to 1.22
Radius
0.96 Rsun
0.91 to 1.47
Age
1.51 Gyr
1.28 to 3.80
Distance
760.7 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.96 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-625
0.96 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-625 b
Transit
◌
Discovery
2016
Period
7.75 days
Radius
1.99 R⊕
Mass
—
Eq. Temp
—
Kepler-625 c
Transit
◌
Discovery
2016
Period
4.17 days
Radius
1.05 R⊕
Mass
—
Eq. Temp
—
Kepler-625 and Its Two Planets
Kepler-625 is a star 2,480 light-years away with two known planets. The host star is 1.51 billion years old and has a mass of 1.04 solar masses, a radius of 0.96 solar radii, and a temperature of 5790 K. Its mass is larger than the Sun's, while its radius is smaller.
Both planets were discovered by transit in 2016, the method that detects the slight dimming caused when a planet crosses in front of its star. Kepler-625 b is a Super-Earth with a radius of 1.99 Earth radii, larger than Earth's, and an orbital period of 7.75 days. Kepler-625 c is classified as Earth-like, with a radius of 1.05 Earth radii, also larger than Earth's, and an orbital period of 4.17 days. Among the listed planets, Kepler-625 c has the smallest radius and the shortest orbital period, while Kepler-625 b has the largest radius and the longest orbital period.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
Stellar refs
14
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6125 | 1.22 | 1.20 | 1.28 | — | — | 760.7 | Q1-Q8 KOI Table | TICv8 |
| 6077 | 1.17 | 1.07 | — | — | — | 760.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5789 | 1.04 | 0.96 | 1.51 | — | — | 760.7 | Morton et al. 2016 | TICv8 |
| 6042 | — | 1.42 | — | — | — | 760.7 | Berger et al. 2018 | TICv8 |
| 6077 | 1.17 | 1.07 | — | — | — | 760.7 | Q1-Q12 KOI Table | TICv8 |
| 5851 | — | 1.36 | — | — | — | 760.7 | Latham et al. 2005 | TICv8 |
| 6077 | 1.17 | 1.07 | — | — | — | 760.7 | Q1-Q12 KOI Table | TICv8 |
| 5604 | 1.00 | 0.91 | — | — | — | 760.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6042 | 1.20 | 1.40 | 3.80 | — | — | 760.7 | Fulton & Petigura 2018 | TICv8 |
| — | — | — | — | — | — | 760.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| — | — | — | — | — | — | 760.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6077 | 1.17 | 1.07 | — | — | — | 760.7 | Q1-Q16 KOI Table | TICv8 |
| 6125 | — | 1.20 | — | — | — | 760.7 | Batalha et al. 2013 | TICv8 |
| 6077 | 1.17 | 1.07 | — | — | — | 760.7 | Q1-Q16 KOI Table | TICv8 |
| 6125 | — | 1.20 | — | — | — | 760.7 | Q1-Q6 KOI Table | TICv8 |
| 6077 | 1.17 | 1.07 | — | — | — | 760.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5604 | 1.00 | 0.91 | — | — | — | 760.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6049.1 | 1.13 | 1.45 | — | 0.41 | — | 760.7 | TICv8 | TICv8 |
| 6125 | 1.22 | 1.20 | 1.28 | — | — | 760.7 | Q1-Q8 KOI Table | TICv8 |
| 5811 | — | 1.47 | — | 0.35 | — | 760.7 | Gaia DR2 | TICv8 |