Temperature
5581 K
5283 to 5642
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Stellar HostProfile
Kepler-1332
Unclassified star • 528.7 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 159578257
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
0.95 Msun
0.78 to 0.97
Radius
0.90 Rsun
0.76 to 0.99
Age
3.24 Gyr
1.30 to 5.25
Distance
528.7 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.90 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1332
0.90 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1332 b
Transit
◌
Discovery
2016
Period
11.87 days
Radius
1.37 R⊕
Mass
—
Eq. Temp
—
Kepler-1332 and Its Earth-Like Planet
Kepler-1332 is a star 1720 light-years away with one known planet. The host star is 3.24 billion years old and has a mass of 0.95 solar masses and a radius of 0.9 solar radii, both smaller than the Sun's, with a temperature of 5580 K that is cooler than the Sun's.
The lone planet, Kepler-1332 b, was discovered by transit in 2016, when it passed in front of its star and caused a small dip in observed brightness. It is classified as Earth-like, meaning it stays within 1.5 times Earth's radius, and its radius of 1.37 Earth radii is larger than Earth's. The planet completes one orbit every 11.9 days. No orbital period is recorded for the star itself; the recorded period belongs to the planet.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
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 |
|---|---|---|---|---|---|---|---|---|
| 5578 | 0.78 | 0.76 | — | — | — | 528.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5405 | — | 0.86 | — | — | — | 528.7 | Latham et al. 2005 | TICv8 |
| 5523 | 0.91 | 0.88 | — | — | — | 528.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 528.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5541.9 | 0.97 | 0.93 | — | -0.14 | — | 528.7 | TICv8 | TICv8 |
| 5581 | — | 0.93 | — | — | — | 528.7 | Berger et al. 2018 | TICv8 |
| 5578 | 0.78 | 0.76 | — | — | — | 528.7 | Q1-Q12 KOI Table | TICv8 |
| 5283 | — | 0.99 | — | -0.17 | — | 528.7 | Gaia DR2 | TICv8 |
| 5581 | 0.95 | 0.90 | 3.24 | — | — | 528.7 | Morton et al. 2016 | TICv8 |
| 5642 | 0.93 | 0.84 | 1.30 | — | — | 528.7 | Q1-Q8 KOI Table | TICv8 |
| 5578 | 0.78 | 0.76 | — | — | — | 528.7 | Q1-Q16 KOI Table | TICv8 |
| 5581 | 0.92 | 0.92 | 5.25 | — | — | 528.7 | Fulton & Petigura 2018 | TICv8 |