Mass
0.57 Msun
0.31 to 0.63
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Stellar HostProfile
OGLE-2012-BLG-0950L
M V • 2600 pc
Records
12
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: Koshimoto et al. 2017 • System source: Koshimoto et al. 2017
Distance
2600 pc
2400 to 4200
Spectral Type
M V
Consistent across records
Planets
1
Stable across source rows
System Layout
Known planets
1 planets linked to this host
OGLE-2012-BLG-0950L b
Microlensing
◌
Discovery
2016
Period
—
Radius
—
Mass
35 M⊕
Eq. Temp
—
The Distant Microlensing System OGLE-2012-BLG-0950L
OGLE-2012-BLG-0950L is a star located 8480 light-years away. It is an M V star, a small, cool red dwarf, with a reported mass of 0.57 solar masses, smaller than the Sun's. One planet is known to orbit it.
That planet, OGLE-2012-BLG-0950L b, was discovered in 2016 by microlensing. It has a reported mass of 35 Earth masses, larger than Earth's, and no orbital period is reported for it.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
1
System refs
1
Distancedisputed
Massdisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | 0.55 | — | — | — | — | 3400 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.57 | — | — | — | M V | 2600 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.63 | — | — | — | — | 3200 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.55 | — | — | — | — | 3400 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.63 | — | — | — | — | 3200 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.33 | — | — | — | — | 3600 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.38 | — | — | — | — | 4200 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.31 | — | — | — | — | 3400 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.47 | — | — | — | — | 2600 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.54 | — | — | — | — | 2400 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.38 | — | — | — | — | 4200 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |
| — | 0.50 | — | — | — | — | 2900 | Koshimoto et al. 2017 | Koshimoto et al. 2017 |