←Back to Exoplanets
ExoplanetDetail

KELT-8 b

Host star KELT-8 • 18.16 R⊕ • 3.24 d orbit

Records

8

archive rows

Discovery

2015

Transit

Radius

18.16 R⊕

default parameter set

Mass

209.8 M⊕

default parameter set

KELT-8

temperature unconstrained

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: Stassun et al. 2017

Host Star

KELT-8

Stable across source rows

KELT-8

Discovery Method

Transit

Consistent across records

Transit (8)

Discovery Year

2015

Stable across source rows

2015

Orbital Period

3.24 day

3.24 to 3.24

8 values • 6 distinct

Radius

18.16 Rearth

18.16 to 21.05

4 values • 3 distinct

Mass

209.8 Mearth

209.8 to 275.6

3 values • 3 distinct

Scale Comparison

Radius against familiar reference worlds

Current adopted radius: 18.16 R⊕ • circles scaled linearly by radius

Earth

1.0 R⊕ baseline

KELT-8 b

18.16 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

4 values • 3 distinct

Massdisputed

3 values • 3 distinct

Eq. Tempdisputed

2 values • 2 distinct

YearMethodFacilityTelescopePeriodRadiusMassEq. TempReference
2015TransitKELTMamiya 645 80mm f/1.93.24 day20.85 Rearth275.6 Mearth1675 KFulton et al. 2015
2015TransitKELTMamiya 645 80mm f/1.93.24 day21.05 Rearth—1428.2 KExoFOP
2015TransitKELTMamiya 645 80mm f/1.93.24 day———Ivshina & Winn 2022
2015TransitKELTMamiya 645 80mm f/1.93.24 day18.16 Rearth209.8 Mearth—Stassun et al. 2017
2015TransitKELTMamiya 645 80mm f/1.93.24 day20.85 Rearth272.7 Mearth—Bonomo et al. 2017
2015TransitKELTMamiya 645 80mm f/1.93.24 day———Mallonn et al. 2019
2015TransitKELTMamiya 645 80mm f/1.93.24 day———Patel & Espinoza 2022
2015TransitKELTMamiya 645 80mm f/1.93.24 day———Kokori et al. 2023