←Back to Stellar Hosts
Stellar HostProfile

Kepler-170

Unclassified star • 738.7 pc

Records

23

literature rows

Planets

2

system count

References

17

distinct source labels

TIC: TIC 120253745

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

5600 K

5417 to 5679

20 values • 8 distinct

Mass

1.03 Msun

0.96 to 1.09

14 values • 7 distinct

Radius

1 Rsun

0.99 to 1.27

21 values • 10 distinct

Age

3.63 Gyr

1.58 to 3.63

4 values • 3 distinct

Distance

738.7 pc

single adopted value

23 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-170

1 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

7.93 days

Radius

3.20 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

16.67 days

Radius

2.86 R⊕

Mass

—

Eq. Temp

—

Kepler-170 and Its Two Neptune-like Planets

Kepler-170 is a star located 2410 light-years away, and two planets have been found orbiting it. The host star is 3.63 billion years old, holds 1.03 solar masses, measures 1 solar radius, and has a temperature of 5600 K, which is cooler than the Sun's.

Both planets were discovered by transit in 2014, the method in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Kepler-170 b is a Neptune-like planet with an orbital period of 7.93 days and a radius of 3.2 Earth radii. Kepler-170 c is also Neptune-like, with an orbital period of 16.7 days and a radius of 2.86 Earth radii. Both radii are larger than Earth's, and among the listed planets Kepler-170 b has both the shortest year and the largest radius, while Kepler-170 c has the longest year and the smallest radius.

Provenance

Underlying measurements and references

Evidence Summary

Rows

23

Stellar refs

16

System refs

1

Distancestable

23 values • 1 distinct

Parallaxstable

23 values • 1 distinct

Temperaturedisputed

20 values • 8 distinct

Massdisputed

14 values • 7 distinct

Radiusdisputed

21 values • 10 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

17 values • 6 distinct

Metallicitydisputed

11 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
56551.080.99———738.7Q1-Q16 KOI TableTICv8
56791.091.031.80——738.7Q1-Q8 KOI TableTICv8
56551.080.99———738.7Q1-Q16 KOI TableTICv8
5679—1.03———738.7Rowe et al. 2014TICv8
56551.080.99———738.7Q1-Q17 DR24 KOI TableTICv8
56551.080.99———738.7Q1-Q12 KOI TableTICv8
56551.080.99———738.7Q1-Q17 DR24 KOI TableTICv8
5679—1.04———738.7Batalha et al. 2013TICv8
5679—1.04———738.7Q1-Q6 KOI TableTICv8
56741.091.03———738.7Q1-Q17 DR25 KOI TableTICv8
——————738.7Q1-Q17 DR25 Supplemental KOI TableTICv8
5497—1.27———738.7Latham et al. 2005TICv8
56551.080.99———738.7Q1-Q12 KOI TableTICv8
56741.091.03———738.7Q1-Q17 DR25 KOI TableTICv8
55731.070.991.58——738.7Fulton & Petigura 2018TICv8
56001.0313.63——738.7Morton et al. 2016TICv8
5417—1.01—-0.10—738.7Gaia DR2TICv8
——————738.7Q1-Q17 DR25 Supplemental KOI TableTICv8
—1.080.99———738.7Hadden et al. 2014TICv8
5573—1.00———738.7Berger et al. 2018TICv8
5679—1.04———738.7Q1-Q6 KOI TableTICv8
56791.091.031.80——738.7Q1-Q8 KOI TableTICv8
54830.961.04—-0.05—738.7TICv8TICv8