Discovery Method
Microlensing
Consistent across records
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ExoplanetDetail
KMT-2018-BLG-1990L b
Host star KMT-2018-BLG-1990L
Records
11
archive rows
Discovery
2019
Microlensing
Radius
—
default parameter set
Mass
111 M⊕
default parameter set
KMT-2018-BLG-1990L
temperature unconstrained
Canonical Summary
Adopted planet values from the default parameter set
Values come from the archive's default parameter set. Missing values stay missing. Ranges and counts describe all source rows.
Selected source: Ryu et al. 2019
Host Star
KMT-2018-BLG-1990L
Stable across source rows
Discovery Year
2019
Stable across source rows
Semi-Major Axis
0.76 au
0.66 to 1.52
Mass
111 Mearth
101 to 293
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Refs
1
Methods
1
Discoverystable
Facilitystable
Massdisputed
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 180 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 101 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 206 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 103 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 180 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 126 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 293 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 111 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 189 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 192 Mearth | — | Ryu et al. 2019 |
| 2019 | Microlensing | KMTNet | 1.6 m wide-field telescope | — | — | 106 Mearth | — | Ryu et al. 2019 |