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Stellar HostProfile

WASP-56

G6 • 321.1 pc

Records

7

literature rows

Planets

1

system count

References

8

distinct source labels

TIC: TIC 347329162

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: Faedi et al. 2013 • System source: TICv8

Temperature

5600 K

5476 to 5797

7 values • 3 distinct

Mass

1.02 Msun

0.71 to 1.11

5 values • 5 distinct

Radius

1.11 Rsun

0.96 to 1.25

7 values • 6 distinct

Age

6.20 Gyr

single adopted value

2 values • 1 distinct

Distance

321.1 pc

single adopted value

7 values • 1 distinct

Spectral Type

G6

Consistent across records

G6 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.11 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

WASP-56

1.11 R☉

System Layout

Known planets

1 planets linked to this host

WASP-56 b

Transit

◌

Discovery

2012

Period

4.62 days

Radius

10.54 R⊕

Mass

143.0 M⊕

Eq. Temp

—

WASP-56 b: A Jupiter-Like World Orbiting a Sun-Like Star

WASP-56 is a star located 1,050 light-years away, and one planet orbits it. The host star has a spectral type of G6, meaning it is a G-type star cooler than the Sun. It is estimated to be 6.2 billion years old, with a mass of 1.02 solar masses, a radius of 1.11 solar radii, and a temperature of 5600 K. Its radius is larger than the Sun's, and its temperature is cooler than the Sun's.

The planet WASP-56 b was discovered in 2012 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. It is classified as Jupiter-like, a size class for planets exceeding 4 times Earth's radius. WASP-56 b has a mass of 143 Earth masses and a radius of 10.5 Earth radii, both larger than Earth's, and its mean density is 0.674 g/cm³, 0.122 times Earth's. It completes one orbit in 4.62 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

7

Stellar refs

7

System refs

1

Distancestable

7 values • 1 distinct

Parallaxstable

7 values • 1 distinct

Temperaturedisputed

7 values • 3 distinct

Massdisputed

5 values • 5 distinct

Radiusdisputed

7 values • 6 distinct

Agestable

2 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

5 values • 4 distinct

Metallicitydisputed

5 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
56001.021.116.20—G6321.1Faedi et al. 2013TICv8
57971.041.11—0.10—321.1TICv8TICv8
57971.111.06———321.1Mortier et al. 2013TICv8
5476—1.25—0.10—321.1Gaia DR2TICv8
56001.111.116.20——321.1Bonomo et al. 2017TICv8
56000.710.96———321.1Stassun et al. 2017TICv8
5797—1.11———321.1ExoFOPTICv8