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Stellar HostProfile

Kepler-46

Unclassified star • 777.1 pc

Records

24

literature rows

Planets

3

system count

References

18

distinct source labels

TIC: TIC 158992508

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: Nesvorný et al. 2012 • System source: TICv8

Temperature

5155 K

4998.6 to 5309

22 values • 9 distinct

Mass

0.90 Msun

0.80 to 0.92

16 values • 7 distinct

Radius

0.94 Rsun

0.75 to 0.94

22 values • 10 distinct

Age

9.70 Gyr

2.34 to 9.70

6 values • 4 distinct

Luminosity

-0.26 log(Lsun)

-0.39 to -0.25

4 values • 4 distinct

Distance

777.1 pc

single adopted value

24 values • 1 distinct

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.94 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-46

0.94 R☉

System Layout

Known planets

3 planets linked to this host

◌

Discovery

2012

Period

33.60 days

Radius

9.06 R⊕

Mass

1907 M⊕

Eq. Temp

543 K

Kepler-46 c

Transit Timing Variations

◌

Discovery

2012

Period

57.01 days

Radius

—

Mass

119.5 M⊕

Eq. Temp

455 K

◌

Discovery

2014

Period

6.77 days

Radius

1.64 R⊕

Mass

—

Eq. Temp

—

Kepler-46 and Its Three Planets

Kepler-46 is a K-type star located 2530 light-years away, with three planets known to orbit it. The star is estimated to be 9.7 billion years old, with a mass of 0.902 solar masses, a radius of 0.938 solar radii, and a temperature of 5160 K. Its mass and radius are both smaller than the Sun's, and it is cooler than the Sun.

Kepler-46 b is a Jupiter-like planet discovered by transit in 2012. It has a reported upper limit of 1907 Earth masses, an orbital period of 33.6 days, and a radius of 9.06 Earth radii, larger than Earth's. Kepler-46 c was discovered in 2012 by transit timing variations, with a mass of 119 Earth masses, larger than Earth's, and an orbital period of 57 days. Kepler-46 d, a Super-Earth discovered by transit in 2014, has an orbital period of 6.77 days and a radius of 1.64 Earth radii.

Among the listed planets, Kepler-46 d has the shortest year, at 6.77 days. Kepler-46 b has the second-shortest year, at 33.6 days, and Kepler-46 c has the longest year, at 57 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

24

Stellar refs

17

System refs

1

Distancestable

24 values • 1 distinct

Parallaxstable

24 values • 1 distinct

Temperaturedisputed

22 values • 9 distinct

Massdisputed

16 values • 7 distinct

Radiusdisputed

22 values • 10 distinct

Agedisputed

6 values • 4 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

19 values • 5 distinct

Metallicitydisputed

13 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
51490.880.93———777.1Q1-Q17 DR24 KOI TableTICv8
——————777.1Q1-Q17 DR25 Supplemental KOI TableTICv8
51270.800.75———777.1Batalha et al. 2013TICv8
51490.880.93———777.1Q1-Q17 DR25 KOI TableTICv8
5127—0.75———777.1Q1-Q6 KOI TableTICv8
52320.920.938.32——777.1Morton et al. 2016TICv8
4998.6—0.85—-0.39—777.1Gaia DR2TICv8
5127—0.81———777.1Latham et al. 2005TICv8
51490.880.93———777.1Q1-Q17 DR25 KOI TableTICv8
52890.820.764.50——777.1Q1-Q8 KOI TableTICv8
5309—0.79———777.1Rowe et al. 2014TICv8
51620.880.802.34——777.1Fulton & Petigura 2018TICv8
51490.880.93———777.1Q1-Q12 KOI TableTICv8
51490.880.93———777.1Q1-Q16 KOI TableTICv8
52890.820.764.50——777.1Q1-Q8 KOI TableTICv8
51490.880.93———777.1Q1-Q16 KOI TableTICv8
51490.880.93———777.1Q1-Q17 DR24 KOI TableTICv8
51550.900.949.70-0.25—777.1Saad-Olivera et al. 2017TICv8
51550.900.949.70-0.26—777.1Nesvorný et al. 2012TICv8
5127—0.75———777.1Q1-Q6 KOI TableTICv8
5162—0.81———777.1Berger et al. 2018TICv8
51490.880.93———777.1Q1-Q12 KOI TableTICv8
50710.850.84—-0.38—777.1TICv8TICv8
——————777.1Q1-Q17 DR25 Supplemental KOI TableTICv8