Temperature
5773 K
5675 to 6053
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Stellar HostProfile
Kepler-200
Unclassified star • 665.9 pc
Records
21
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 120252452
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
0.98 Msun
0.88 to 1.05
Radius
0.95 Rsun
0.92 to 1.33
Age
3.63 Gyr
3.63 to 6.30
Distance
665.9 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.95 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-200
0.95 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-200 b
Transit
◌
Discovery
2014
Period
8.59 days
Radius
2.13 R⊕
Mass
—
Eq. Temp
—
Kepler-200 c
Transit
◌
Discovery
2014
Period
10.22 days
Radius
1.59 R⊕
Mass
—
Eq. Temp
—
Kepler-200 and Its Two Super-Earths
Kepler-200 is a star 2170 light-years away with two planets orbiting it. The host star has a mass of 0.98 solar masses, a radius of 0.95 solar radii, a temperature of 5770 K, and an age of 3.63 billion years.
Both planets are Super-Earths discovered by transit in 2014. Kepler-200 b has an orbital period of 8.59 days and a radius of 2.13 Earth radii. Kepler-200 c has an orbital period of 10.2 days and a radius of 1.59 Earth radii. Among the listed planets, Kepler-200 b has the shortest year and the largest radius, while Kepler-200 c has the longest year and the smallest radius. The reported radius estimates of both planets are larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
21
Stellar refs
15
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 |
|---|---|---|---|---|---|---|---|---|
| 6034 | 1.04 | 1.28 | 6.30 | — | — | 665.9 | Q1-Q8 KOI Table | TICv8 |
| 6053 | 1.04 | 1.28 | — | — | — | 665.9 | Q1-Q16 KOI Table | TICv8 |
| 6053 | 1.04 | 1.28 | — | — | — | 665.9 | Q1-Q12 KOI Table | TICv8 |
| 5756 | — | 0.96 | — | -0.04 | — | 665.9 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 665.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5838.6 | 1.05 | 0.99 | — | 7.78e-3 | — | 665.9 | TICv8 | TICv8 |
| — | — | — | — | — | — | 665.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6034 | 1.04 | 1.28 | 6.30 | — | — | 665.9 | Q1-Q8 KOI Table | TICv8 |
| 5773 | 0.98 | 0.95 | 3.63 | — | — | 665.9 | Morton et al. 2016 | TICv8 |
| 5675 | 0.88 | 0.92 | — | — | — | 665.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5799 | — | 1.33 | — | — | — | 665.9 | Latham et al. 2005 | TICv8 |
| 5785 | 0.97 | 0.97 | 3.98 | — | — | 665.9 | Fulton & Petigura 2018 | TICv8 |
| 5799 | — | 1.26 | — | — | — | 665.9 | Batalha et al. 2013 | TICv8 |
| 5678 | — | 0.94 | — | — | — | 665.9 | Rowe et al. 2014 | TICv8 |
| 5675 | 0.88 | 0.92 | — | — | — | 665.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6053 | 1.04 | 1.28 | — | — | — | 665.9 | Q1-Q16 KOI Table | TICv8 |
| 5785 | — | 0.99 | — | — | — | 665.9 | Berger et al. 2018 | TICv8 |
| 6053 | 1.04 | 1.28 | — | — | — | 665.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6053 | 1.04 | 1.28 | — | — | — | 665.9 | Q1-Q12 KOI Table | TICv8 |
| 6053 | 1.04 | 1.28 | — | — | — | 665.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5799 | — | 1.26 | — | — | — | 665.9 | Q1-Q6 KOI Table | TICv8 |