Temperature
4965 K
4905 to 5132
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Stellar HostProfile
Kepler-1195
Unclassified star • 918.6 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 120252007
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
0.74 Msun
0.68 to 0.84
Radius
0.71 Rsun
0.67 to 0.83
Age
4.47 Gyr
4.47 to 9.80
Distance
918.6 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.71 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1195
0.71 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1195 b
Transit
◌
Discovery
2016
Period
8.50 days
Radius
2.08 R⊕
Mass
—
Eq. Temp
—
Kepler-1195 b: A Super-Earth in a Distant System
Kepler-1195 is a star located 3000 light-years away. It is 4.47 billion years old and has a mass of 0.74 solar masses, a radius of 0.71 solar radii, and a temperature of 4970 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's. One planet is known in this system.
That planet, Kepler-1195 b, is a Super-Earth discovered by the transit method in 2016. 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. Kepler-1195 b orbits every 8.5 days and has a radius of 2.08 Earth radii, larger than Earth's. Planet size classes compare radius with Earth's, and a Super-Earth reaches 2.5 times Earth's radius.
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 |
|---|---|---|---|---|---|---|---|---|
| 4961 | 0.68 | 0.67 | — | — | — | 918.6 | Batalha et al. 2013 | TICv8 |
| 5043 | 0.84 | 0.78 | — | -0.45 | — | 918.6 | TICv8 | TICv8 |
| 5093 | 0.71 | 0.71 | — | — | — | 918.6 | Q1-Q12 KOI Table | TICv8 |
| 5132 | 0.77 | 0.75 | 9.80 | — | — | 918.6 | Q1-Q8 KOI Table | TICv8 |
| 4905 | — | 0.79 | — | -0.49 | — | 918.6 | Gaia DR2 | TICv8 |
| 5093 | 0.71 | 0.71 | — | — | — | 918.6 | Q1-Q16 KOI Table | TICv8 |
| 4961 | — | 0.81 | — | — | — | 918.6 | Latham et al. 2005 | TICv8 |
| 4961 | — | 0.67 | — | — | — | 918.6 | Q1-Q6 KOI Table | TICv8 |
| 5093 | 0.71 | 0.71 | — | — | — | 918.6 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5093 | 0.71 | 0.71 | — | — | — | 918.6 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 918.6 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5093 | — | 0.83 | — | — | — | 918.6 | Berger et al. 2018 | TICv8 |
| 4965 | 0.74 | 0.71 | 4.47 | — | — | 918.6 | Morton et al. 2016 | TICv8 |