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Stellar HostProfile

Kepler-388

Unclassified star

Records

19

literature rows

Planets

2

system count

References

13

distinct source labels

TIC: TIC 164786156

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

4584 K

4359 to 4584

17 values • 6 distinct

Mass

0.73 Msun

0.59 to 0.73

12 values • 4 distinct

Radius

0.69 Rsun

0.56 to 1.01

17 values • 7 distinct

Age

3.98 Gyr

3.98 to 13.90

3 values • 2 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.69 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-388

0.69 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

3.17 days

Radius

0.81 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

13.30 days

Radius

0.86 R⊕

Mass

—

Eq. Temp

—

Kepler-388 and Its Two Sub-Earth Planets

Kepler-388 is a star with two known planets, both discovered by transit in 2014. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods. The star's reported mass estimate is 0.73 solar masses, its reported radius estimate is 0.69 solar radii, and its reported temperature is 4580 K, all smaller or cooler than the Sun's corresponding values. Its age is 3.98 billion years.

Kepler-388 b and Kepler-388 c are both Sub-Earths, a size class comparing radius with Earth's: a Sub-Earth is smaller than Earth. Kepler-388 b has a reported radius estimate of 0.81 Earth radii, smaller than Earth's, and an orbital period of 3.17 days. Kepler-388 c has a reported radius estimate of 0.86 Earth radii, also smaller than Earth's, and an orbital period of 13.3 days. Among the listed planets, Kepler-388 b has the shortest year and the smallest radius by reported estimates, while Kepler-388 c has the longest year and the largest radius by reported estimates.

Provenance

Underlying measurements and references

Evidence Summary

Rows

19

Stellar refs

12

System refs

1

Temperaturedisputed

17 values • 6 distinct

Massdisputed

12 values • 4 distinct

Radiusdisputed

17 values • 7 distinct

Agedisputed

3 values • 2 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

16 values • 6 distinct

Metallicitydisputed

10 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
45000.630.63————Q1-Q17 DR25 KOI TableTICv8
45000.630.63————Q1-Q17 DR24 KOI TableTICv8
4498—0.59————Rowe et al. 2014TICv8
45300.640.6113.90———Q1-Q8 KOI TableTICv8
43590.590.56————Batalha et al. 2013TICv8
45000.630.63————Q1-Q12 KOI TableTICv8
45000.630.63————Q1-Q16 KOI TableTICv8
45300.640.6113.90———Q1-Q8 KOI TableTICv8
45000.630.63————Q1-Q17 DR25 KOI TableTICv8
45000.630.63————Q1-Q17 DR24 KOI TableTICv8
4359—0.56————Q1-Q6 KOI TableTICv8
4452.8—1.01—-0.44——Gaia DR2TICv8
45000.630.63————Q1-Q12 KOI TableTICv8
4359—0.56————Q1-Q6 KOI TableTICv8
45840.730.693.98———Morton et al. 2016TICv8
4359—0.67————Latham et al. 2005TICv8
———————Q1-Q17 DR25 Supplemental KOI TableTICv8
45000.630.63————Q1-Q16 KOI TableTICv8
———————Q1-Q17 DR25 Supplemental KOI TableTICv8