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Stellar HostProfile

Kepler-432

Unclassified star • 848.0 pc

Records

17

literature rows

Planets

2

system count

References

18

distinct source labels

TIC: TIC 26817004

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: Quinn et al. 2015 • System source: TICv8

Temperature

4995 K

4850 to 5061

15 values • 8 distinct

Mass

1.32 Msun

1.32 to 1.49

9 values • 6 distinct

Radius

4.06 Rsun

3.29 to 4.16

15 values • 10 distinct

Age

4.20 Gyr

2.63 to 4.20

4 values • 3 distinct

Distance

848.0 pc

single adopted value

17 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 4.06 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-432

4.06 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2015

Period

52.50 days

Radius

12.83 R⊕

Mass

1719.5 M⊕

Eq. Temp

—

Kepler-432 c

Radial Velocity

◌

Discovery

2015

Period

406.2 days

Radius

—

Mass

772.3 M⊕

Eq. Temp

—

Kepler-432: A Distant Star With Two Known Worlds

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

Underlying measurements and references

Evidence Summary

Rows

17

Stellar refs

17

System refs

1

Distancestable

17 values • 1 distinct

Parallaxstable

17 values • 1 distinct

Temperaturedisputed

15 values • 8 distinct

Massdisputed

9 values • 6 distinct

Radiusdisputed

15 values • 10 distinct

Agedisputed

4 values • 3 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

10 values • 5 distinct

Metallicitydisputed

9 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————848.0Q1-Q17 DR25 Supplemental KOI TableTICv8
49951.354.124.20——848.0Bonomo et al. 2017TICv8
5061—3.29———848.0Q1-Q6 KOI TableTICv8
49951.354.16———848.0Q1-Q16 KOI TableTICv8
5061—3.29———848.0Batalha et al. 2013TICv8
48501.354.16———848.0Ciceri et al. 2015TICv8
5002—4.00———848.0Berger et al. 2018TICv8
50611.343.293.87——848.0Q1-Q8 KOI TableTICv8
4950—3.58———848.0Latham et al. 2005TICv8
49951.324.064.20——848.0Quinn et al. 2015TICv8
50021.493.932.63——848.0Fulton & Petigura 2018TICv8
——————848.0Huber et al. 2013TICv8
49951.354.16———848.0Q1-Q17 DR24 KOI TableTICv8
49951.354.16———848.0Q1-Q12 KOI TableTICv8
4982.0—3.97———848.0TICv8TICv8
4941.8—3.96—0.93—848.0Gaia DR2TICv8
49761.354.16———848.0Q1-Q17 DR25 KOI TableTICv8