Temperature
4807 K
4655 to 4821
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Stellar HostProfile
Kepler-1653
Unclassified star
Records
8
literature rows
Planets
1
system count
References
9
distinct source labels
TIC: TIC 184561612
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: Torres et al. 2017 • System source: TICv8
Mass
0.72 Msun
0.68 to 0.77
Radius
0.69 Rsun
0.69 to 1.06
Age
7.70 Gyr
single adopted value
Luminosity
-0.64 log(Lsun)
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.69 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1653
0.69 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1653 b
Transit
◌
Discovery
2017
Period
140.3 days
Radius
2.17 R⊕
Mass
—
Eq. Temp
284 K
Kepler-1653 and Its Super-Earth
Kepler-1653 is a star with one known planet. The star is estimated to be 7.7 billion years old, with a mass of 0.719 solar masses and a radius of 0.693 solar radii. Its temperature is 4810 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-1653 b is classified as a Super-Earth. A Super-Earth is a size class that reaches 2.5 times Earth's radius; the class describes radius, not composition. Kepler-1653 b has a radius of 2.17 Earth radii, larger than Earth's, and an orbital period of 140 days. It was discovered by the transit method in 2017.
A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness.
Provenance
Underlying measurements and references
Evidence Summary
Rows
8
Stellar refs
8
System refs
1
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4771 | 0.68 | 0.70 | — | — | — | — | Q1-Q16 KOI Table | TICv8 |
| 4771 | 0.68 | 0.70 | — | — | — | — | Q1-Q17 DR24 KOI Table | TICv8 |
| 4821 | 0.77 | 0.79 | — | — | — | — | Q1-Q17 DR25 KOI Table | TICv8 |
| 4771 | 0.68 | 0.70 | — | — | — | — | Q1-Q12 KOI Table | TICv8 |
| 4807 | 0.72 | 0.69 | 7.70 | -0.64 | — | — | Torres et al. 2017 | TICv8 |
| — | — | — | — | — | — | — | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4807 | — | 1.06 | — | — | — | — | Berger et al. 2018 | TICv8 |
| 4655 | — | 0.76 | — | — | — | — | Latham et al. 2005 | TICv8 |