Temperature
5471 K
5174.1 to 5495
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Stellar HostProfile
Kepler-1232
Unclassified star • 632.9 pc
Records
19
literature rows
Planets
1
system count
References
15
distinct source labels
TIC: TIC 351190880
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
0.92 Msun
0.82 to 0.92
Radius
0.89 Rsun
0.77 to 1.03
Age
4.79 Gyr
2.63 to 13.90
Distance
632.9 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1232
0.89 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1232 b
Transit
◌
Discovery
2016
Period
26.78 days
Radius
1.93 R⊕
Mass
—
Eq. Temp
—
Kepler-1232 b: A Super-Earth in a Distant System
Kepler-1232 is a star located 2060 light-years away. It is 4.79 billion years old and has 0.92 solar masses, 0.89 solar radii, and a temperature of 5470 K. Its mass estimate is smaller than the Sun's, and its temperature is cooler. One planet orbits this host.
That planet is Kepler-1232 b, a Super-Earth discovered by transit in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1232 b completes an orbit every 26.8 days and has a radius of 1.93 Earth radii, larger than Earth's. The Super-Earth class covers planets reaching 2.5 times Earth's radius, while an Earth-like planet stays within 1.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
19
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 |
|---|---|---|---|---|---|---|---|---|
| 5241 | 0.90 | 0.80 | — | -0.36 | — | 632.9 | TICv8 | TICv8 |
| 5495 | 0.91 | 0.98 | — | — | — | 632.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5495 | 0.91 | 0.98 | — | — | — | 632.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5495 | 0.91 | 0.98 | — | — | — | 632.9 | Q1-Q16 KOI Table | TICv8 |
| 5495 | 0.91 | 0.98 | — | — | — | 632.9 | Q1-Q12 KOI Table | TICv8 |
| 5295 | — | 0.95 | — | — | — | 632.9 | Q1-Q6 KOI Table | TICv8 |
| 5495 | 0.91 | 0.98 | — | — | — | 632.9 | Q1-Q12 KOI Table | TICv8 |
| 5214 | 0.84 | 0.77 | 2.63 | — | — | 632.9 | Fulton & Petigura 2018 | TICv8 |
| 5242 | 0.87 | 0.86 | — | — | — | 632.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5295 | — | 1.03 | — | — | — | 632.9 | Latham et al. 2005 | TICv8 |
| 5495 | 0.91 | 0.98 | — | — | — | 632.9 | Q1-Q16 KOI Table | TICv8 |
| 5295 | 0.88 | 0.95 | — | — | — | 632.9 | Batalha et al. 2013 | TICv8 |
| 5174.1 | — | 0.80 | — | -0.39 | — | 632.9 | Gaia DR2 | TICv8 |
| 5413 | 0.82 | 0.91 | 13.90 | — | — | 632.9 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 632.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5242 | 0.87 | 0.86 | — | — | — | 632.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5471 | 0.92 | 0.89 | 4.79 | — | — | 632.9 | Morton et al. 2016 | TICv8 |
| 5214 | — | 0.79 | — | — | — | 632.9 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 632.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |