Temperature
6217 K
6217 to 6443
Unclassified star • 383.8 pc
Records
7
literature rows
Planets
1
system count
References
8
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: TICv8 • System source: TICv8
Temperature
6217 K
6217 to 6443
Mass
1.20 Msun
1.10 to 1.20
Radius
1.27 Rsun
0.76 to 1.27
Luminosity
0.34 log(Lsun)
0.31 to 0.34
Distance
383.8 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.27 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
WASP-31
1.27 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2010
Period
3.41 days
Radius
17.36 R⊕
Mass
151.9 M⊕
Eq. Temp
—
WASP-31 is a star 1250 light-years away with a mass of 1.2 solar masses and a radius of 1.27 solar radii. Its temperature is 6220 K. One planet orbits this host.
That planet, WASP-31 b, was discovered by transit in 2010 and is classified as Jupiter-like. It has a mass of 152 Earth masses, a radius of 17.4 Earth radii, and an orbital period of 3.41 days.
The star's reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's. WASP-31 b's reported radius and mass estimates are larger than Earth's.
Provenance
Evidence Summary
Rows
7
Stellar refs
7
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6300 | 1.16 | 1.24 | — | — | — | 383.8 | Brown et al. 2012 | TICv8 |
| 6443 | 1.10 | 0.76 | — | — | — | 383.8 | Mortier et al. 2013 | TICv8 |
| 6217 | 1.20 | 1.27 | — | 0.34 | — | 383.8 | TICv8 | TICv8 |
| 6302 | 1.16 | 1.25 | — | — | — | 383.8 | Anderson et al. 2011 | TICv8 |
| 6335.5 | — | 1.19 | — | 0.31 | — | 383.8 | Gaia DR2 | TICv8 |
| 6302 | — | 1.27 | — | — | — | 383.8 | ExoFOP | TICv8 |
| 6300 | 1.17 | 1.25 | 1 | — | — | 383.8 | Bonomo et al. 2017 | TICv8 |