Temperature
6230 K
6086 to 6250
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Stellar HostProfile
Kepler-910
Unclassified star • 400.3 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 272178989
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
1.26 Msun
1.15 to 1.33
Radius
1.50 Rsun
1.22 to 1.57
Age
3.39 Gyr
2.65 to 3.39
Distance
400.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.50 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-910
1.50 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-910 b
Transit
◌
Discovery
2016
Period
2.36 days
Radius
0.82 R⊕
Mass
—
Eq. Temp
—
Kepler-910 and Its Sub-Earth Planet
Kepler-910 is a star 1310 light-years away with one known planet. The host star is 3.39 billion years old and has a mass of 1.26 solar masses, a radius of 1.5 solar radii, and a temperature of 6230 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's.
The planet, Kepler-910 b, was discovered by transit in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-910 b has an orbital period of 2.36 days and a radius of 0.82 Earth radii. Its reported radius estimate is smaller than Earth's, and it is classified as a Sub-Earth, a size class for planets smaller than Earth.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
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 |
|---|---|---|---|---|---|---|---|---|
| 6117.2 | 1.15 | 1.57 | — | 0.49 | — | 400.3 | TICv8 | TICv8 |
| 6086 | — | 1.22 | — | — | — | 400.3 | Latham et al. 2005 | TICv8 |
| 6134 | 1.22 | 1.29 | 2.65 | — | — | 400.3 | Q1-Q8 KOI Table | TICv8 |
| 6088 | — | 1.54 | — | 0.47 | — | 400.3 | Gaia DR2 | TICv8 |
| 6173 | 1.27 | 1.51 | — | — | — | 400.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6134 | — | 1.29 | — | — | — | 400.3 | Q1-Q6 KOI Table | TICv8 |
| 6230 | 1.26 | 1.50 | 3.39 | — | — | 400.3 | Morton et al. 2016 | TICv8 |
| 6230 | — | 1.51 | — | — | — | 400.3 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 400.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6173 | 1.27 | 1.51 | — | — | — | 400.3 | Q1-Q16 KOI Table | TICv8 |
| 6173 | 1.27 | 1.51 | — | — | — | 400.3 | Q1-Q12 KOI Table | TICv8 |
| 6230 | 1.26 | 1.49 | 3.02 | — | — | 400.3 | Fulton & Petigura 2018 | TICv8 |
| 6134 | 1.22 | 1.29 | — | — | — | 400.3 | Batalha et al. 2013 | TICv8 |
| 6250 | 1.33 | 1.54 | — | — | — | 400.3 | Q1-Q17 DR25 KOI Table | TICv8 |