Mass
0.41 Msun
0.41 to 0.48
Unclassified star โข 7790 pc
Records
4
literature rows
Planets
1
system count
References
2
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: Shin et al. 2022 โข System source: Shin et al. 2022
Mass
0.41 Msun
0.41 to 0.48
Distance
7790 pc
7790 to 8120
Planets
1
Stable across source rows
System Layout
1 planets linked to this host
Microlensing
Discovery
2022
Period
โ
Radius
โ
Mass
225.7 Mโ
Eq. Temp
โ
OGLE-2016-BLG-1093L is a star 25400 light-years away with a reported mass estimate of 0.41 solar masses, smaller than the Sun's. One planet is known to orbit it.
That planet, OGLE-2016-BLG-1093L b, was discovered in 2022 by microlensing, a method that reveals a planet through the gravitational influence it and its host exert on light from a more distant background source. The planet's reported mass estimate is 226 Earth masses, larger than Earth's. No orbital period is reported for OGLE-2016-BLG-1093L b.
Provenance
Evidence Summary
Rows
4
Stellar refs
1
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | 0.46 | โ | โ | โ | โ | 8120 | Shin et al. 2022 | Shin et al. 2022 |
| โ | 0.48 | โ | โ | โ | โ | 8060 | Shin et al. 2022 | Shin et al. 2022 |
| โ | 0.45 | โ | โ | โ | โ | 7930 | Shin et al. 2022 | Shin et al. 2022 |
| โ | 0.41 | โ | โ | โ | โ | 7790 | Shin et al. 2022 | Shin et al. 2022 |