Temperature
4647 K
4360 to 4647
←Back to Stellar Hosts
Stellar HostProfile
Kepler-1032
Unclassified star • 673.0 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 122139228
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
0.77 Msun
0.54 to 0.77
Radius
0.71 Rsun
0.52 to 0.80
Age
1.86 Gyr
1.86 to 13.90
Distance
673.0 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.71 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1032
0.71 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1032 b
Transit
◌
Discovery
2016
Period
3.29 days
Radius
1.87 R⊕
Mass
—
Eq. Temp
—
Kepler-1032 and Its Super-Earth
Kepler-1032 is a star located 2200 light-years away, and it hosts one known planet. The star is estimated to be 1.86 billion years old. Its mass is 0.77 solar masses, its radius is 0.71 solar radii, and its temperature is 4650 K. The star's reported mass estimate is smaller than the Sun's, and its reported radius estimate is smaller than the Sun's. Its reported temperature is cooler than the Sun's.
The planet Kepler-1032 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-1032 b is classified as a Super-Earth, a size class that reaches 2.5 times Earth's radius. It orbits its star every 3.29 days and has a radius of 1.87 Earth radii. Its reported radius estimate 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
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4360 | — | 0.79 | — | — | — | 673.0 | Latham et al. 2005 | TICv8 |
| 4484 | 0.58 | 0.59 | — | — | — | 673.0 | Q1-Q12 KOI Table | TICv8 |
| 4360 | — | 0.52 | — | — | — | 673.0 | Q1-Q6 KOI Table | TICv8 |
| 4481 | — | 0.80 | — | — | — | 673.0 | Berger et al. 2018 | TICv8 |
| 4484 | 0.58 | 0.59 | — | — | — | 673.0 | Q1-Q16 KOI Table | TICv8 |
| 4484 | 0.58 | 0.59 | — | — | — | 673.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4423 | — | 0.80 | — | -0.66 | — | 673.0 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 673.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4484 | 0.58 | 0.59 | — | — | — | 673.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4446 | — | — | — | — | — | 673.0 | TICv8 | TICv8 |
| 4574 | 0.64 | 0.62 | 13.90 | — | — | 673.0 | Q1-Q8 KOI Table | TICv8 |
| 4647 | 0.77 | 0.71 | 1.86 | — | — | 673.0 | Morton et al. 2016 | TICv8 |
| 4360 | 0.54 | 0.52 | — | — | — | 673.0 | Batalha et al. 2013 | TICv8 |