Temperature
3410 K
3304 to 3673
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Stellar HostProfile
Kepler-1650
Unclassified star • 134.4 pc
Records
14
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 273502299
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: Mann et al. 2017 • System source: TICv8
Mass
0.33 Msun
0.24 to 0.50
Radius
0.33 Rsun
0.26 to 1.12
Luminosity
-1.87 log(Lsun)
-1.87 to -1.78
Distance
134.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.33 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1650
0.33 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1650 b
Transit
◌
Discovery
2017
Period
1.54 days
Radius
0.96 R⊕
Mass
—
Eq. Temp
—
Kepler-1650 b: A Sub-Earth Planet
Kepler-1650 is a star 438 light-years away with one known planet. The star has a mass of 0.326 solar masses, a radius of 0.334 solar radii, and a temperature of 3410 K. Its reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet, Kepler-1650 b, was discovered in 2017 by the transit method, in which 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-1650 b completes an orbit every 1.54 days. Its radius is 0.96 Earth radii, placing it in the Sub-Earth size class, which compares radius with Earth's and indicates a planet smaller than Earth.
Provenance
Underlying measurements and references
Evidence Summary
Rows
14
Stellar refs
14
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 |
|---|---|---|---|---|---|---|---|---|
| 3364 | 0.26 | 0.27 | — | — | — | 134.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 3310.2 | — | — | — | — | — | 134.4 | Gaia DR2 | TICv8 |
| — | — | — | 3.82 | — | — | 134.4 | Gaidos et al. 2024 | TICv8 |
| 3523 | 0.50 | 0.51 | — | — | — | 134.4 | Batalha et al. 2013 | TICv8 |
| 3419 | 0.35 | 0.37 | — | -1.78 | — | 134.4 | TICv8 | TICv8 |
| 3304 | 0.24 | 0.26 | — | — | — | 134.4 | Q1-Q12 KOI Table | TICv8 |
| 3523 | — | 0.51 | — | — | — | 134.4 | Q1-Q6 KOI Table | TICv8 |
| 3304 | 0.24 | 0.26 | — | — | — | 134.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 3673 | 0.49 | 0.48 | 13.90 | — | — | 134.4 | Q1-Q8 KOI Table | TICv8 |
| 3356 | — | 0.37 | — | — | — | 134.4 | Berger et al. 2018 | TICv8 |
| 3304 | 0.24 | 0.26 | — | — | — | 134.4 | Q1-Q16 KOI Table | TICv8 |
| 3523 | — | 1.12 | — | — | — | 134.4 | Latham et al. 2005 | TICv8 |
| 3410 | 0.33 | 0.33 | — | -1.87 | — | 134.4 | Mann et al. 2017 | TICv8 |
| — | — | — | — | — | — | 134.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |