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ExoplanetDetail

WASP-174 b

Host star WASP-174 • 16.11 R⊕ • 4.23 d orbit

Records

5

archive rows

Discovery

2018

Transit

Radius

16.11 R⊕

default parameter set

Mass

104.9 M⊕

default parameter set

WASP-174

1528 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: Mancini et al. 2020

Host Star

WASP-174

Stable across source rows

WASP-174

Discovery Method

Transit

Consistent across records

Transit (5)

Discovery Year

2018

Stable across source rows

2018

Orbital Period

4.23 day

4.23 to 4.23

5 values • 4 distinct

Semi-Major Axis

0.06 au

0.06 to 0.06

2 values • 2 distinct

Radius

16.11 Rearth

14.57 to 19.62

3 values • 3 distinct

Mass

104.9 Mearth

104.9 to 413.2

2 values • 2 distinct

Density

0.14 g/cm**3

single adopted value

1 values • 1 distinct

Equilibrium Temperature

1528 K

1490 to 1528

3 values • 3 distinct

Scale Comparison

Radius against familiar reference worlds

Current adopted radius: 16.11 R⊕ • circles scaled linearly by radius

Earth

1.0 R⊕ baseline

WASP-174 b

16.11 R⊕

Jupiter

11.2 R⊕ reference

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Refs

5

Methods

1

Discoverystable

5 values • 1 distinct

Facilitystable

5 values • 1 distinct

Periodstable

5 values • 1 distinct

Radiusdisputed

3 values • 3 distinct

Massdisputed

2 values • 2 distinct

Eq. Tempdisputed

3 values • 3 distinct

YearMethodFacilityTelescopePeriodRadiusMassEq. TempReference
2018TransitSuperWASP-SouthCanon 200mm f/1.8L4.23 day19.62 Rearth—1491 KExoFOP
2018TransitSuperWASP-SouthCanon 200mm f/1.8L4.23 day16.11 Rearth104.9 Mearth1528 KMancini et al. 2020
2018TransitSuperWASP-SouthCanon 200mm f/1.8L4.23 day———Kokori et al. 2023
2018TransitSuperWASP-SouthCanon 200mm f/1.8L4.23 day———Ivshina & Winn 2022
2018TransitSuperWASP-SouthCanon 200mm f/1.8L4.23 day14.57 Rearth413.2 Mearth1490 KTemple et al. 2018