Temperature
3638 K
3482 to 3885
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Stellar HostProfile
Kepler-1652
Unclassified star
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 27187450
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
0.40 Msun
0.36 to 0.55
Radius
0.38 Rsun
0.35 to 0.64
Age
3.20 Gyr
3.20 to 13.90
Luminosity
-1.64 log(Lsun)
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.38 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1652
0.38 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1652 b
Transit
◌
Discovery
2017
Period
38.10 days
Radius
1.60 R⊕
Mass
—
Eq. Temp
268 K
Kepler-1652 and Its Super-Earth
Kepler-1652 is a single known star, and one planet has been identified in its orbit. The star is 3.2 billion years old, with a mass of 0.404 solar masses and a radius of 0.382 solar radii. Its reported temperature is 3640 K. The star's reported mass estimate is smaller than the Sun's, and its reported radius estimate is also smaller than the Sun's. Its reported temperature is cooler than the Sun's.
The host star's one known planet is Kepler-1652 b, a Super-Earth discovered by transit in 2017. 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-1652 b completes an orbit in 38.1 days. Its radius is 1.6 Earth radii, larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 3735 | — | 0.53 | — | — | — | — | Q1-Q6 KOI Table | TICv8 |
| 3885 | 0.52 | 0.50 | 13.90 | — | — | — | Q1-Q8 KOI Table | TICv8 |
| 3554 | 0.43 | 0.40 | — | — | — | — | Q1-Q17 DR25 KOI Table | TICv8 |
| 3482 | 0.36 | 0.35 | — | — | — | — | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | — | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 3638 | 0.40 | 0.38 | 3.20 | -1.64 | — | — | Torres et al. 2017 | TICv8 |
| 3482 | 0.36 | 0.35 | — | — | — | — | Q1-Q16 KOI Table | TICv8 |
| 3482 | 0.36 | 0.35 | — | — | — | — | Q1-Q17 DR24 KOI Table | TICv8 |
| 3735 | 0.55 | 0.53 | — | — | — | — | Batalha et al. 2013 | TICv8 |
| 3735 | — | 0.64 | — | — | — | — | Latham et al. 2005 | TICv8 |
| 3757.7 | — | — | — | — | — | — | Gaia DR2 | TICv8 |