Temperature
4299 K
4061 to 4299
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Stellar HostProfile
Kepler-1105
Unclassified star • 318.0 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 123231917
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
0.71 Msun
0.55 to 0.71
Radius
0.68 Rsun
0.52 to 0.81
Age
8.71 Gyr
8.71 to 13.90
Distance
318.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.68 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1105
0.68 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1105 b
Transit
◌
Discovery
2016
Period
4.42 days
Radius
2.01 R⊕
Mass
—
Eq. Temp
—
Kepler-1105 and Its Super-Earth
Kepler-1105 is a star located 1040 light-years away, and it hosts one known planet. The star is estimated to be 8.71 billion years old, with a reported mass of 0.71 solar masses and a reported radius of 0.68 solar radii. Its reported temperature is 4300 K.
The planet, Kepler-1105 b, was discovered in 2016 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Repeated dips help establish orbital periods. Kepler-1105 b is a Super-Earth, a size class that reaches 2.5 times Earth's radius. It has an orbital period of 4.42 days and a radius of 2.01 Earth radii, which is 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 |
|---|---|---|---|---|---|---|---|---|
| 4299 | — | 0.58 | — | — | — | 318.0 | Berger et al. 2018 | TICv8 |
| 4189 | 0.67 | 0.66 | — | — | — | 318.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4230 | 0.58 | 0.55 | 13.90 | — | — | 318.0 | Q1-Q8 KOI Table | TICv8 |
| 4114 | 0.64 | 0.66 | — | -0.95 | — | 318.0 | TICv8 | TICv8 |
| 4061 | — | 0.52 | — | — | — | 318.0 | Q1-Q6 KOI Table | TICv8 |
| 4299 | 0.71 | 0.70 | — | — | — | 318.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4189 | 0.67 | 0.66 | — | — | — | 318.0 | Q1-Q12 KOI Table | TICv8 |
| 4061 | 0.55 | 0.52 | — | — | — | 318.0 | Batalha et al. 2013 | TICv8 |
| 4135.1 | — | 0.63 | — | -0.99 | — | 318.0 | Gaia DR2 | TICv8 |
| 4061 | — | 0.81 | — | — | — | 318.0 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 318.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4299 | 0.71 | 0.68 | 8.71 | — | — | 318.0 | Morton et al. 2016 | TICv8 |
| 4189 | 0.67 | 0.66 | — | — | — | 318.0 | Q1-Q16 KOI Table | TICv8 |