Temperature
5315 K
5100 to 5626
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Stellar HostProfile
Kepler-800
Unclassified star • 1019.3 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 158275161
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
0.85 Msun
0.85 to 0.92
Radius
0.82 Rsun
0.78 to 0.86
Age
4.68 Gyr
1.10 to 4.68
Distance
1019.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.82 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-800
0.82 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-800 b
Transit
◌
Discovery
2016
Period
14.13 days
Radius
2.85 R⊕
Mass
—
Eq. Temp
—
Kepler-800 and Its Neptune-Like Planet
Kepler-800 is a star 3320 light-years away with one known planet. The host star is 4.68 billion years old and has a mass of 0.85 solar masses and a radius of 0.82 solar radii. Its temperature is 5320 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.
The planet Kepler-800 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-800 b is Neptune-like and orbits every 14.1 days. Its radius is 2.85 Earth radii, larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| 5418 | — | 0.80 | — | — | — | 1019.3 | Q1-Q6 KOI Table | TICv8 |
| 5626 | 0.91 | 0.82 | — | — | — | 1019.3 | Q1-Q16 KOI Table | TICv8 |
| 5626 | 0.91 | 0.82 | — | — | — | 1019.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5418 | — | 0.80 | — | — | — | 1019.3 | Batalha et al. 2013 | TICv8 |
| 5626 | 0.91 | 0.82 | — | — | — | 1019.3 | Q1-Q12 KOI Table | TICv8 |
| 5418 | — | 0.81 | — | — | — | 1019.3 | Latham et al. 2005 | TICv8 |
| 5293 | 0.91 | 0.79 | — | -0.36 | — | 1019.3 | TICv8 | TICv8 |
| 5100 | — | 0.86 | — | -0.35 | — | 1019.3 | Gaia DR2 | TICv8 |
| 5616 | 0.91 | 0.82 | — | — | — | 1019.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5621 | — | 0.78 | — | — | — | 1019.3 | Berger et al. 2018 | TICv8 |
| 5612 | 0.92 | 0.83 | 1.10 | — | — | 1019.3 | Q1-Q8 KOI Table | TICv8 |
| 5315 | 0.85 | 0.82 | 4.68 | — | — | 1019.3 | Morton et al. 2016 | TICv8 |
| — | — | — | — | — | — | 1019.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |