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ExoplanetDetail

K2-122 b

Host star K2-122 • 1.16 R⊕ • 2.22 d orbit

Records

8

archive rows

Discovery

2017

Transit

Radius

1.16 R⊕

default parameter set

Mass

—

default parameter set

K2-122

769 K equilibrium

Canonical Summary

Adopted planet values from the default parameter set

Values come from the archive's default parameter set. Missing values stay missing. Ranges and counts describe all source rows.

Selected source: Castro-González et al. 2022

Host Star

K2-122

Stable across source rows

K2-122

Discovery Method

Transit

Consistent across records

Transit (8)

Discovery Year

2017

Stable across source rows

2017

Orbital Period

2.22 day

2.22 to 2.22

8 values • 8 distinct

Semi-Major Axis

0.04 au

0.03 to 0.04

4 values • 4 distinct

Radius

1.16 Rearth

1.16 to 1.30

6 values • 6 distinct

Equilibrium Temperature

769 K

769 to 814

2 values • 2 distinct

Scale Comparison

Radius against familiar reference worlds

Current adopted radius: 1.16 R⊕ • circles scaled linearly by radius

Earth

1.0 R⊕ baseline

K2-122 b

1.16 R⊕

Jupiter

11.2 R⊕ reference

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Refs

8

Methods

1

Discoverystable

8 values • 1 distinct

Facilitystable

8 values • 1 distinct

Periodstable

8 values • 1 distinct

Radiusdisputed

6 values • 6 distinct

Eq. Tempdisputed

2 values • 2 distinct

YearMethodFacilityTelescopePeriodRadiusMassEq. TempReference
2017TransitK20.95 m Kepler Telescope2.22 day1.16 Rearth—769 KCastro-González et al. 2022
2017TransitK20.95 m Kepler Telescope2.22 day———Pope et al. 2016
2017TransitK20.95 m Kepler Telescope2.22 day1.28 Rearth——Dressing et al. 2017
2017TransitK20.95 m Kepler Telescope2.22 day1.30 Rearth——Petigura et al. 2018
2017TransitK20.95 m Kepler Telescope2.22 day1.21 Rearth—814 KLivingston et al. 2018
2017TransitK20.95 m Kepler Telescope2.22 day1.17 Rearth——Kruse et al. 2019
2017TransitK20.95 m Kepler Telescope2.22 day———Barros et al. 2016
2017TransitK20.95 m Kepler Telescope2.22 day1.22 Rearth——Hirano et al. 2018