Back to Stellar Hosts
Stellar HostProfile

WASP-96

G8 • 352.5 pc

Records

8

literature rows

Planets

1

system count

References

9

distinct source labels

TIC: TIC 160148385

Approximate color

from effective temperature

Canonical Summary

Adopted host values from all rows

Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.

Temperature

5540 K

5476 to 5678

7 values • 6 distinct

Mass

1.03 Msun

0.98 to 1.06

5 values • 4 distinct

Radius

1.07 Rsun

1.05 to 1.15

7 values • 5 distinct

Age

7.30 Gyr

5.20 to 9.40

4 values • 4 distinct

Luminosity

0.03 log(Lsun)

2.17e-3 to 0.03

3 values • 3 distinct

Distance

352.5 pc

single adopted value

8 values • 1 distinct

Spectral Type

G8

Consistent across records

G8 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.07 R☉ • circles scaled linearly by radius

Sun

1.0 R☉ baseline

WASP-96

1.07 R☉

System Layout

Known planets

1 planets linked to this host

WASP-96 b

Transit

Discovery

2014

Period

3.43 days

Radius

13.45 R⊕

Mass

152.6 M⊕

Eq. Temp

1285 K

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values • 1 distinct

Parallaxstable

8 values • 1 distinct

Temperaturedisputed

7 values • 6 distinct

Massdisputed

5 values • 4 distinct

Radiusdisputed

7 values • 5 distinct

Agedisputed

4 values • 4 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

5 values • 5 distinct

Metallicitydisputed

5 values • 4 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
54761.150.03352.5Gaia DR2TICv8
56781.031.055.20352.5McGruder et al. 2023TICv8
55001.061.059.40352.5Bonomo et al. 2017TICv8
55871.021.076.602.17e-3352.5Wang et al. 2026TICv8
55600.981.120.03352.5TICv8TICv8
55401.12352.5ExoFOPTICv8
352.5Nikolov et al. 2022TICv8
55401.061.058G8352.5Hellier et al. 2014TICv8