Mass
0.51 Msun
single adopted value
←Back to Stellar Hosts
Stellar HostProfile
MOA-2022-BLG-033L
F7 V • 1840 pc
Records
4
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: Han et al. 2025 • System source: Han et al. 2025
Distance
1840 pc
single adopted value
Spectral Type
F7 V
Consistent across records
Planets
1
Stable across source rows
System Layout
Known planets
1 planets linked to this host
MOA-2022-BLG-033L b
Microlensing
◌
Discovery
2025
Period
—
Radius
—
Mass
12.15 M⊕
Eq. Temp
—
MOA-2022-BLG-033L b: A Microlensing Planet Around a Distant Dwarf
MOA-2022-BLG-033L is a star 6000 light-years away with one known planet. Its spectral type, F7 V, identifies it as an F-type main-sequence dwarf. The star's reported mass estimate is 0.51 solar masses, smaller than the Sun's.
The planet MOA-2022-BLG-033L b was discovered by microlensing in 2025. Its reported mass estimate is 12.2 Earth masses, larger than Earth's. No orbital period is reported for MOA-2022-BLG-033L b.
Provenance
Underlying measurements and references
Evidence Summary
Rows
4
Stellar refs
1
System refs
1
Distancestable
Massstable
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | 0.51 | — | — | — | F7 V | 1840 | Han et al. 2025 | Han et al. 2025 |
| — | 0.51 | — | — | — | F7 V | 1840 | Han et al. 2025 | Han et al. 2025 |
| — | 0.51 | — | — | — | F7 V | 1840 | Han et al. 2025 | Han et al. 2025 |
| — | 0.51 | — | — | — | F7 V | 1840 | Han et al. 2025 | Han et al. 2025 |