Temperature
2859 K
single adopted value
Unclassified star • 66.06 pc
Records
2
literature rows
Planets
1
system count
References
3
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
2859 K
single adopted value
Mass
0.29 Msun
0.05 to 0.29
Radius
0.32 Rsun
single adopted value
Luminosity
-2.22 log(Lsun)
-2.59 to -2.22
Distance
66.06 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.32 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
2MASS J0249-0557 A
0.32 R☉
System Layout
1 planets linked to this host
Imaging
Discovery
2018
Period
—
Radius
17.37 R⊕
Mass
3616.9 M⊕
Eq. Temp
1723 K
2MASS J0249-0557 A is an M6 V star located 215 light-years away. Its reported mass estimate is 0.295 solar masses, its reported radius estimate is 0.316 solar radii, and its reported temperature is 2860 K, all smaller or cooler than the corresponding values for the Sun. The star hosts one known planet.
That planet is 2MASS J0249-0557 c, discovered by imaging in 2018. It is a Jupiter-like planet, a class defined by a radius exceeding four times Earth's, and it is circumbinary, orbiting both stars of the binary system rather than one star alone. Its reported radius estimate is 17.4 Earth radii and its reported mass estimate is 3620 Earth masses, roughly 11.4 times Jupiter's mass. Both values exceed Earth's corresponding figures, and its mean density is 3.8 g/cm³, 0.69 times Earth's. No orbital period is reported for 2MASS J0249-0557 c.
Provenance
Evidence Summary
Rows
2
Stellar refs
2
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 2859 | 0.29 | 0.32 | — | -2.22 | — | 66.06 | TICv8 | TICv8 |
| — | 0.05 | — | 0.02 | -2.59 | M6 V | 66.06 | Dupuy et al. 2018 | TICv8 |