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ExoplanetDetail

NGTS-4 b

Host star NGTS-4 • 3.18 R⊕ • 1.34 d orbit

Records

4

archive rows

Discovery

2019

Transit

Radius

3.18 R⊕

default parameter set

Mass

20.60 M⊕

default parameter set

NGTS-4

1650 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: West et al. 2019

Host Star

NGTS-4

Stable across source rows

NGTS-4

Discovery Method

Transit

Consistent across records

Transit (4)

Discovery Year

2019

Stable across source rows

2019

Orbital Period

1.34 day

1.34 to 1.34

4 values • 4 distinct

Semi-Major Axis

0.02 au

single adopted value

1 values • 1 distinct

Radius

3.18 Rearth

3.03 to 3.19

3 values • 3 distinct

Mass

20.60 Mearth

single adopted value

1 values • 1 distinct

Density

3.45 g/cm**3

single adopted value

1 values • 1 distinct

Equilibrium Temperature

1650 K

1391.9 to 1650

2 values • 2 distinct

Scale Comparison

Radius against familiar reference worlds

Current adopted radius: 3.18 R⊕ • circles scaled linearly by radius

Earth

1.0 R⊕ baseline

NGTS-4 b

3.18 R⊕

Jupiter

11.2 R⊕ reference

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Refs

4

Methods

1

Discoverystable

4 values • 1 distinct

Facilitystable

4 values • 1 distinct

Periodstable

4 values • 1 distinct

Radiusdisputed

3 values • 3 distinct

Massstable

1 values • 1 distinct

Eq. Tempdisputed

2 values • 2 distinct

YearMethodFacilityTelescopePeriodRadiusMassEq. TempReference
2019TransitNext-Generation Transit Survey (NGTS)20 cm NGTS telescope1.34 day3.18 Rearth20.60 Mearth1650 KWest et al. 2019
2019TransitNext-Generation Transit Survey (NGTS)20 cm NGTS telescope1.34 day3.03 Rearth—1391.9 KExoFOP
2019TransitNext-Generation Transit Survey (NGTS)20 cm NGTS telescope1.34 day———Patel & Espinoza 2022
2019TransitNext-Generation Transit Survey (NGTS)20 cm NGTS telescope1.34 day3.19 Rearth——Lafarga et al. 2026