Mass
0.69 Msun
single adopted value
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Stellar HostProfile
OGLE-2018-BLG-1126L
Unclassified star โข 5690 pc
Records
3
literature rows
Planets
1
system count
References
2
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Gould et al. 2022 โข System source: Gould et al. 2022
Distance
5690 pc
5690 to 5700
Planets
1
Stable across source rows
System Layout
Known planets
1 planets linked to this host
OGLE-2018-BLG-1126L b
Microlensing
โ
Discovery
2022
Period
โ
Radius
โ
Mass
17.80 Mโ
Eq. Temp
โ
OGLE-2018-BLG-1126L: A Microlensing Host and Its Single Planet
OGLE-2018-BLG-1126L is a star 18600 light-years away with 0.69 solar masses, and one planet is known to orbit it. That planet, OGLE-2018-BLG-1126L b, was discovered in 2022 by microlensing. Microlensing is a method that detects a planet when its gravity briefly brightens a background star.
OGLE-2018-BLG-1126L b has a mass of 17.8 Earth masses. This reported mass estimate is larger than Earth's. No orbital period is reported for OGLE-2018-BLG-1126L b.
Provenance
Underlying measurements and references
Evidence Summary
Rows
3
Stellar refs
1
System refs
1
Distancedisputed
Massstable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | 0.69 | โ | โ | โ | โ | 5700 | Gould et al. 2022 | Gould et al. 2022 |
| โ | 0.69 | โ | โ | โ | โ | 5690 | Gould et al. 2022 | Gould et al. 2022 |
| โ | 0.69 | โ | โ | โ | โ | 5700 | Gould et al. 2022 | Gould et al. 2022 |