Temperature
5079 K
4982.8 to 5079
Unclassified star • 283.3 pc
Records
5
literature rows
Planets
1
system count
References
6
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
5079 K
4982.8 to 5079
Mass
0.85 Msun
0.85 to 0.91
Radius
0.75 Rsun
0.75 to 0.76
Luminosity
-0.47 log(Lsun)
-0.50 to -0.47
Distance
283.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.75 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
EPIC 212499991
0.75 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2019
Period
34.88 days
Radius
1.60 R⊕
Mass
—
Eq. Temp
—
EPIC 212499991 is a star 924 light-years away with one known planet. The star's reported mass estimate is 0.85 solar masses and its reported radius estimate is 0.752 solar radii, both smaller than the Sun's. Its temperature of 5080 K is cooler than the Sun's. The planet EPIC 212499991 b is classified as a Super-Earth, a size class reaching 2.5 times Earth's radius. The planet's reported radius estimate is 1.6 Earth radii, larger than Earth's, and it orbits every 34.9 days. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods. EPIC 212499991 b was discovered by transit in 2019.
Provenance
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4982.8 | — | 0.76 | — | -0.50 | — | 283.3 | Gaia DR2 | TICv8 |
| 5079 | 0.85 | 0.75 | — | -0.47 | — | 283.3 | TICv8 | TICv8 |
| — | 0.91 | — | — | — | — | 283.3 | Heller et al. 2019 | TICv8 |
| — | — | — | — | — | — | 283.3 | Pope et al. 2016 | TICv8 |
| — | — | 0.76 | — | — | — | 283.3 | Kruse et al. 2019 | TICv8 |