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Stellar HostProfile

Kepler-162

Unclassified star • 855.6 pc

Records

22

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 273036401

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

6089 K

5397 to 6089

20 values • 8 distinct

Mass

1.12 Msun

0.88 to 1.12

13 values • 5 distinct

Radius

1.20 Rsun

0.91 to 1.26

20 values • 10 distinct

Age

3.02 Gyr

3.02 to 5.60

4 values • 3 distinct

Distance

855.6 pc

single adopted value

22 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.20 R☉ • circles scaled linearly by radius

Sun

1.0 R☉ baseline

Kepler-162

1.20 R☉

System Layout

Known planets

2 planets linked to this host

Discovery

2014

Period

6.92 days

Radius

1.26 R⊕

Mass

Eq. Temp

Discovery

2014

Period

19.45 days

Radius

3.03 R⊕

Mass

Eq. Temp

Kepler-162 and Its Two Planets

Kepler-162 is a star 2790 light-years away with two planets orbiting it. The star is 3.02 billion years old, has a mass of 1.12 solar masses, a radius of 1.2 solar radii, and a temperature of 6090 K. Its mass estimate is larger than the Sun's, and its temperature is hotter 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-162 b is an Earth-like planet with a radius of 1.26 Earth radii and an orbital period of 6.92 days. Among the listed planets, it has the shortest year and the smallest radius. Kepler-162 c is a Neptune-like planet with a radius of 3.03 Earth radii and an orbital period of 19.4 days. Its radius estimate is larger than Earth's, and among the listed planets it has the longest year and the largest radius.

Provenance

Underlying measurements and references

Evidence Summary

Rows

22

Stellar refs

15

System refs

1

Distancestable

22 values • 1 distinct

Parallaxstable

22 values • 1 distinct

Temperaturedisputed

20 values • 8 distinct

Massdisputed

13 values • 5 distinct

Radiusdisputed

20 values • 10 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

17 values • 7 distinct

Metallicitydisputed

11 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
58150.880.95855.6Q1-Q17 DR24 KOI TableTICv8
57431.031.210.16855.6TICv8TICv8
56010.91855.6Q1-Q6 KOI TableTICv8
58150.880.95855.6Q1-Q12 KOI TableTICv8
58150.880.95855.6Q1-Q17 DR25 KOI TableTICv8
58150.880.95855.6Q1-Q16 KOI TableTICv8
53971.260.08855.6Gaia DR2TICv8
58160.96855.6Rowe et al. 2014TICv8
56011.04855.6Latham et al. 2005TICv8
58150.880.95855.6Q1-Q17 DR24 KOI TableTICv8
58380.950.985.60855.6Q1-Q8 KOI TableTICv8
56010.91855.6Q1-Q6 KOI TableTICv8
60891.121.203.02855.6Morton et al. 2016TICv8
58701.15855.6Berger et al. 2018TICv8
58150.880.95855.6Q1-Q17 DR25 KOI TableTICv8
855.6Q1-Q17 DR25 Supplemental KOI TableTICv8
58380.950.985.60855.6Q1-Q8 KOI TableTICv8
58150.880.95855.6Q1-Q16 KOI TableTICv8
855.6Q1-Q17 DR25 Supplemental KOI TableTICv8
58701.051.134.57855.6Fulton & Petigura 2018TICv8
56010.91855.6Batalha et al. 2013TICv8
58150.880.95855.6Q1-Q12 KOI TableTICv8