←Back to Stellar Hosts
Stellar HostProfile

Kepler-1181

Unclassified star • 938.4 pc

Records

17

literature rows

Planets

2

system count

References

13

distinct source labels

TIC: TIC 394176812

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

6176 K

6176 to 6841

15 values • 7 distinct

Mass

1.17 Msun

1.17 to 1.34

12 values • 6 distinct

Radius

1.30 Rsun

1.19 to 1.36

15 values • 8 distinct

Age

3.24 Gyr

single adopted value

1 values • 1 distinct

Distance

938.4 pc

single adopted value

17 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.30 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-1181

1.30 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2016

Period

4.89 days

Radius

1.57 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2023

Period

8.93 days

Radius

1.83 R⊕

Mass

—

Eq. Temp

1124 K

Kepler-1181 and Its Two Super-Earths

Kepler-1181 is a star located 3060 light-years away, and two planets have been found orbiting it. The host star is estimated to be 3.24 billion years old, with a mass of 1.17 solar masses and a radius of 1.3 solar radii. Its reported temperature is 6180 K, hotter than the Sun's, and both its mass and radius are larger than the Sun's.

Both known planets are classified as Super-Earths, a size class that reaches up to 2.5 times Earth's radius. Kepler-1181 b was discovered by transit in 2016. It completes an orbit in 4.89 days, among the listed planets the shortest year, and has a radius of 1.57 Earth radii, the smallest radius among the listed planets. Kepler-1181 c was discovered by transit in 2023. It orbits in 8.93 days, the longest year among the listed planets, and has a radius of 1.83 Earth radii, the largest radius among the listed planets. Both planets' reported radius estimates are larger than Earth's. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness, and repeated dips help establish orbital periods.

Provenance

Underlying measurements and references

Evidence Summary

Rows

17

Stellar refs

12

System refs

1

Distancestable

17 values • 1 distinct

Parallaxstable

17 values • 1 distinct

Temperaturedisputed

15 values • 7 distinct

Massdisputed

12 values • 6 distinct

Radiusdisputed

15 values • 8 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

13 values • 6 distinct

Metallicitydisputed

10 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
63331.241.25———938.4Q1-Q8 KOI TableTICv8
——————938.4Q1-Q17 DR25 Supplemental KOI TableTICv8
63331.221.25———938.4Batalha et al. 2013TICv8
61761.171.303.24——938.4Morton et al. 2016TICv8
66801.331.32———938.4Q1-Q16 KOI TableTICv8
66801.331.32———938.4Q1-Q12 KOI TableTICv8
66801.331.32———938.4Q1-Q12 KOI TableTICv8
6333—1.25———938.4Q1-Q6 KOI TableTICv8
6495.31.331.36—0.47—938.4TICv8TICv8
66881.341.35———938.4Q1-Q17 DR25 KOI TableTICv8
66801.331.32———938.4Q1-Q17 DR24 KOI TableTICv8
66881.341.35———938.4Q1-Q17 DR25 KOI TableTICv8
66801.331.32———938.4Q1-Q17 DR24 KOI TableTICv8
——————938.4Q1-Q17 DR25 Supplemental KOI TableTICv8
66801.331.32———938.4Q1-Q16 KOI TableTICv8
6841—1.19—0.45—938.4Gaia DR2TICv8
6689—1.33———938.4Berger et al. 2018TICv8