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Stellar HostProfile

Kepler-347

Unclassified star • 1298.9 pc

Records

25

literature rows

Planets

3

system count

References

16

distinct source labels

TIC: TIC 299158566

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

Temperature

5892 K

5592 to 6092

22 values • 9 distinct

Mass

1.05 Msun

0.92 to 1.07

17 values • 6 distinct

Radius

1.06 Rsun

0.86 to 1.48

22 values • 11 distinct

Age

3.89 Gyr

0.30 to 11.75

3 values • 3 distinct

Distance

1298.9 pc

single adopted value

25 values • 1 distinct

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 1.06 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-347

1.06 R☉

System Layout

Known planets

3 planets linked to this host

◌

Discovery

2014

Period

12.80 days

Radius

1.97 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

27.32 days

Radius

1.75 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2023

Period

85.52 days

Radius

3.04 R⊕

Mass

—

Eq. Temp

482 K

Kepler-347 and Its Three Worlds

Kepler-347 is a star 4240 light-years away with three known planets. The host is 3.89 billion years old, has 1.05 solar masses, 1.06 solar radii, and a temperature of 5890 K, which is hotter than the Sun's. All three planets were found by transit, the method that detects the slight dimming caused when a planet crosses in front of its star, and repeated dips help establish orbital periods.

Kepler-347 b and Kepler-347 c are both Super-Earths, a size class that reaches 2.5 times Earth's radius. Kepler-347 b has a radius of 1.97 Earth radii - larger than Earth's - and completes an orbit in 12.8 days, the shortest year among the listed planets. Kepler-347 c has a radius of 1.75 Earth radii, the smallest among the listed planets, and an orbital period of 27.3 days, the second-shortest year. Kepler-347 d is Neptune-like, a class reaching 4 times Earth's radius. Its radius of 3.04 Earth radii is the largest among the listed planets and larger than Earth's, and its orbital period of 85.5 days is the longest year among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

25

Stellar refs

15

System refs

1

Distancestable

25 values • 1 distinct

Parallaxstable

25 values • 1 distinct

Temperaturedisputed

22 values • 9 distinct

Massdisputed

17 values • 6 distinct

Radiusdisputed

22 values • 11 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

19 values • 8 distinct

Metallicitydisputed

15 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
58331.051.45—0.34—1298.9TICv8TICv8
60641.060.960.30——1298.9Q1-Q8 KOI TableTICv8
60921.071.00———1298.9Q1-Q16 KOI TableTICv8
5817—0.93———1298.9Q1-Q6 KOI TableTICv8
559211.45———1298.9Q1-Q17 DR25 KOI TableTICv8
559211.45———1298.9Q1-Q17 DR25 KOI TableTICv8
5767.2—1.48—0.34—1298.9Gaia DR2TICv8
58921.051.063.89——1298.9Morton et al. 2016TICv8
60921.071.00———1298.9Q1-Q12 KOI TableTICv8
——————1298.9Q1-Q17 DR25 Supplemental KOI TableTICv8
5817—0.86———1298.9Latham et al. 2005TICv8
5704—1.48———1298.9Berger et al. 2018TICv8
60921.071.00———1298.9Q1-Q17 DR24 KOI TableTICv8
60921.071.00———1298.9Q1-Q17 DR24 KOI TableTICv8
60921.071.00———1298.9Q1-Q12 KOI TableTICv8
60921.071.00———1298.9Q1-Q12 KOI TableTICv8
58171.040.93———1298.9Batalha et al. 2013TICv8
60921.071.00———1298.9Q1-Q16 KOI TableTICv8
——————1298.9Q1-Q17 DR25 Supplemental KOI TableTICv8
60921.071.00———1298.9Q1-Q17 DR24 KOI TableTICv8
——————1298.9Q1-Q17 DR25 Supplemental KOI TableTICv8
57040.921.4411.75——1298.9Fulton & Petigura 2018TICv8
6088—1.00———1298.9Rowe et al. 2014TICv8
60921.071.00———1298.9Q1-Q16 KOI TableTICv8
559211.45———1298.9Q1-Q17 DR25 KOI TableTICv8