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ExoplanetDetail

WASP-62 b

Host star WASP-62 • 15.06 R⊕ • 4.41 d orbit

Records

12

archive rows

Discovery

Transit

Radius

15.06 R⊕

median non-null value

Mass

180.8 M⊕

median non-null value

WASP-62

1647.2 K equilibrium

Quick Summary

Fast scan of the current planet profile

This first pass still reads from the currently available detail payload. Canonical adopted summaries will replace first-row values in the next backend pass.

Host Star

WASP-62

Discovery

Transit

Year

2012

Period

4.41 day

Radius

14.80 Rearth

Mass

165.3 Mearth

Eq. Temp

Scale Comparison

Radius against familiar reference worlds

Current adopted radius: 15.06 R⊕ • circles scaled linearly by radius

Earth

1.0 R⊕ baseline

WASP-62 b

15.06 R⊕

Jupiter

11.2 R⊕ reference

Provenance

Underlying measurements and references

Evidence Summary

Rows

12

Refs

12

Methods

1

Discoverystable

12 values • 1 distinct

Facilitystable

12 values • 1 distinct

Periodstable

12 values • 1 distinct

Radiusdisputed

5 values • 4 distinct

Massdisputed

4 values • 4 distinct

Eq. Tempdisputed

2 values • 2 distinct

YearMethodFacilityTelescopePeriodRadiusMassEq. TempReference
2012TransitSuperWASPCanon 200mm f/1.8L4.41 day14.80 Rearth165.3 MearthStassun et al. 2017
2012TransitSuperWASPCanon 200mm f/1.8L4.41 dayMaciejewski 2020
2012TransitSuperWASPCanon 200mm f/1.8L4.41 dayKokori et al. 2022
2012TransitSuperWASPCanon 200mm f/1.8L4.41 dayIvshina & Winn 2022
2012TransitSuperWASPCanon 200mm f/1.8L4.41 daySkaf et al. 2020
2012TransitSuperWASPCanon 200mm f/1.8L4.41 dayKokori et al. 2023
2012TransitSuperWASPCanon 200mm f/1.8L4.41 dayPatel & Espinoza 2022
2012TransitSuperWASPCanon 200mm f/1.8L4.41 dayGarhart et al. 2020
2012TransitSuperWASPCanon 200mm f/1.8L4.41 day15.58 Rearth180.5 MearthBonomo et al. 2017
2012TransitSuperWASPCanon 200mm f/1.8L4.41 day15.06 Rearth1819.1 KExoFOP
2012TransitSuperWASPCanon 200mm f/1.8L4.41 day15.58 Rearth181.2 MearthHellier et al. 2012
2012TransitSuperWASPCanon 200mm f/1.8L4.41 day15.02 Rearth184.3 Mearth1475.3 KBrown et al. 2017