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ExoplanetDetail

WASP-73 b

Host star WASP-73 • 15.92 R⊕ • 4.09 d orbit

Records

8

archive rows

Discovery

2014

Transit

Radius

15.92 R⊕

default parameter set

Mass

909.0 M⊕

default parameter set

WASP-73

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

WASP-73

Stable across source rows

WASP-73

Discovery Method

Transit

Consistent across records

Transit (8)

Discovery Year

2014

Stable across source rows

2014

Orbital Period

4.09 day

4.09 to 4.09

8 values • 5 distinct

Radius

15.92 Rearth

13.00 to 15.92

4 values • 4 distinct

Mass

909.0 Mearth

597.2 to 909.0

3 values • 3 distinct

Scale Comparison

Radius against familiar reference worlds

Current adopted radius: 15.92 R⊕ • circles scaled linearly by radius

Earth

1.0 R⊕ baseline

WASP-73 b

15.92 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
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day———Patel & Espinoza 2022
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day13.00 Rearth597.2 Mearth—Bonomo et al. 2017
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day———Kokori et al. 2023
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day15.92 Rearth909.0 Mearth—Stassun et al. 2017
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day13.62 Rearth—1755.1 KExoFOP
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day13.00 Rearth597.5 Mearth1790 KDelrez et al. 2014
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day———Ivshina & Winn 2022
2014TransitSuperWASPCanon 200mm f/1.8L4.09 day———Mallonn et al. 2019