Temperature
4995 K
4850 to 5061
Unclassified star • 848.0 pc
Records
17
literature rows
Planets
2
system count
References
18
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Quinn et al. 2015 • System source: TICv8
Temperature
4995 K
4850 to 5061
Mass
1.32 Msun
1.32 to 1.49
Radius
4.06 Rsun
3.29 to 4.16
Age
4.20 Gyr
2.63 to 4.20
Distance
848.0 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 4.06 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-432
4.06 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2015
Period
52.50 days
Radius
12.83 R⊕
Mass
1719.5 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2015
Period
406.2 days
Radius
—
Mass
772.3 M⊕
Eq. Temp
—
Kepler-432 is a star located 2770 light-years away. It has 1.32 solar masses and 4.06 solar radii, making it larger than the Sun in both mass and radius. Its temperature is 5000 K, cooler than the Sun, and it is 4.2 billion years old. Two planets are known to orbit this host.
The first, Kepler-432 b, was discovered in 2015 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. This Jupiter-like planet has a radius of 12.8 Earth radii, larger than Earth's, and a mass of 1720 Earth masses, roughly 5.41 times Jupiter's mass. It completes an orbit in 52.5 days, the shortest year among the listed planets.
Kepler-432 c was also discovered in 2015, using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. Its minimum mass is 772 Earth masses, 2.43 times Jupiter's mass. This planet takes 406 days to orbit its star, the longest year among the listed planets.
Provenance
Evidence Summary
Rows
17
Stellar refs
17
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 848.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4995 | 1.35 | 4.12 | 4.20 | — | — | 848.0 | Bonomo et al. 2017 | TICv8 |
| 5061 | — | 3.29 | — | — | — | 848.0 | Q1-Q6 KOI Table | TICv8 |
| 4995 | 1.35 | 4.16 | — | — | — | 848.0 | Q1-Q16 KOI Table | TICv8 |
| 5061 | — | 3.29 | — | — | — | 848.0 | Batalha et al. 2013 | TICv8 |
| 4850 | 1.35 | 4.16 | — | — | — | 848.0 | Ciceri et al. 2015 | TICv8 |
| 5002 | — | 4.00 | — | — | — | 848.0 | Berger et al. 2018 | TICv8 |
| 5061 | 1.34 | 3.29 | 3.87 | — | — | 848.0 | Q1-Q8 KOI Table | TICv8 |
| 4950 | — | 3.58 | — | — | — | 848.0 | Latham et al. 2005 | TICv8 |
| 4995 | 1.32 | 4.06 | 4.20 | — | — | 848.0 | Quinn et al. 2015 | TICv8 |
| 5002 | 1.49 | 3.93 | 2.63 | — | — | 848.0 | Fulton & Petigura 2018 | TICv8 |
| — | — | — | — | — | — | 848.0 | Huber et al. 2013 | TICv8 |
| 4995 | 1.35 | 4.16 | — | — | — | 848.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4995 | 1.35 | 4.16 | — | — | — | 848.0 | Q1-Q12 KOI Table | TICv8 |
| 4982.0 | — | 3.97 | — | — | — | 848.0 | TICv8 | TICv8 |
| 4941.8 | — | 3.96 | — | 0.93 | — | 848.0 | Gaia DR2 | TICv8 |
| 4976 | 1.35 | 4.16 | — | — | — | 848.0 | Q1-Q17 DR25 KOI Table | TICv8 |