Temperature
6148 K
5975 to 6435
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Stellar HostProfile
Kepler-1655
G0 V • 213.3 pc
Records
15
literature rows
Planets
1
system count
References
16
distinct source labels
TIC: TIC 120973167
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: Haywood et al. 2018 • System source: TICv8
Mass
1.03 Msun
0.92 to 1.12
Radius
1.03 Rsun
1.02 to 1.39
Age
2.56 Gyr
2.56 to 7.80
Distance
213.3 pc
single adopted value
Spectral Type
G0 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.03 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1655
1.03 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1655 b
Transit
◌
Discovery
2018
Period
11.87 days
Radius
2.21 R⊕
Mass
5.40 M⊕
Eq. Temp
938 K
Kepler-1655 and Its Super-Earth
Kepler-1655 is a G0 V star, a Sun-like main-sequence dwarf, located 696 light-years away. The star is 2.56 billion years old and has a mass of 1.03 solar masses, a radius of 1.03 solar radii, and a temperature of 6150 K. Its reported radius estimate is larger than the Sun's, and its reported temperature is hotter than the Sun's. One planet is known to orbit this star.
Kepler-1655 b is a Super-Earth discovered by transit in 2018. It has an orbital period of 11.9 days, a mass of 5.4 Earth masses, and a radius of 2.21 Earth radii. Its reported radius estimate is larger than Earth's, and its reported mass estimate is larger than Earth's. The planet's mean density is 2.75 g/cm³, 0.498 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
15
Stellar refs
15
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6435 | — | 1.39 | — | — | — | 213.3 | Latham et al. 2005 | TICv8 |
| 6134 | — | 1.02 | — | 0.12 | — | 213.3 | Gaia DR2 | TICv8 |
| 5975 | 0.96 | 1.17 | 7.80 | — | — | 213.3 | Q1-Q8 KOI Table | TICv8 |
| 5975 | — | 1.17 | — | — | — | 213.3 | Batalha et al. 2013 | TICv8 |
| 6134 | 1.03 | 1.04 | — | — | — | 213.3 | Q1-Q16 KOI Table | TICv8 |
| 6148 | 1.03 | 1.03 | 2.56 | — | — | 213.3 | Bonomo et al. 2023 | TICv8 |
| 5975 | — | 1.17 | — | — | — | 213.3 | Q1-Q6 KOI Table | TICv8 |
| 6148 | 1.03 | 1.03 | 2.56 | — | G0 V | 213.3 | Haywood et al. 2018 | TICv8 |
| 6002 | 0.92 | 1.05 | 7.24 | — | — | 213.3 | Fulton & Petigura 2018 | TICv8 |
| 6134 | 1.03 | 1.04 | — | — | — | 213.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 213.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6147 | 1.01 | 1.04 | — | — | — | 213.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6002 | — | 1.06 | — | — | — | 213.3 | Berger et al. 2018 | TICv8 |
| 6134 | 1.03 | 1.04 | — | — | — | 213.3 | Q1-Q12 KOI Table | TICv8 |
| 6043.4 | 1.12 | 1.08 | — | 0.14 | — | 213.3 | TICv8 | TICv8 |