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Stellar HostProfile

WASP-171

G0 • 757.8 pc

Records

4

literature rows

Planets

1

system count

References

5

distinct source labels

TIC: TIC 162922904

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: Nielsen et al. 2019 • System source: TICv8

Temperature

5965 K

5846 to 6090

4 values • 3 distinct

Mass

1.17 Msun

1.14 to 1.17

2 values • 2 distinct

Radius

1.64 Rsun

1.64 to 2.11

4 values • 4 distinct

Age

5.91 Gyr

single adopted value

1 values • 1 distinct

Distance

757.8 pc

single adopted value

4 values • 1 distinct

Spectral Type

G0

Consistent across records

G0 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.64 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

WASP-171

1.64 R☉

System Layout

Known planets

1 planets linked to this host

WASP-171 b

Transit

◌

Discovery

2019

Period

3.82 days

Radius

10.98 R⊕

Mass

344.5 M⊕

Eq. Temp

1642 K

WASP-171 and Its Jupiter-Like Planet

WASP-171 is a G0 star 2470 light-years away, with a mass of 1.17 solar masses, a radius of 1.64 solar radii, and a temperature of 5970 K. Its age is 5.91 billion years. The star's reported mass estimate is larger than the Sun's, its reported radius estimate is larger than the Sun's, and its reported temperature is hotter than the Sun's. One planet orbits this host.

That planet is WASP-171 b, a Jupiter-like world discovered by transit in 2019. It completes an orbit every 3.82 days and has a mass of 345 Earth masses and a radius of 11 Earth radii. Both its reported radius estimate and its reported mass estimate are larger than Earth's, and its mean density is 1.43 g/cm³, 0.26 times Earth's. As a size class, Jupiter-like means its radius exceeds 4 times Earth's radius. During a transit, the planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods such as this one.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

4

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

4 values • 4 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 3 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5846—2.11—0.67—757.8Gaia DR2TICv8
60901.142.03—0.71—757.8TICv8TICv8
6090—2.03———757.8ExoFOPTICv8
59651.171.645.91—G0757.8Nielsen et al. 2019TICv8