Mass
0.39 Msun
0.39 to 0.40
Unclassified star โข 6380 pc
Records
2
literature rows
Planets
2
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: Suzuki et al. 2018 โข System source: Suzuki et al. 2018
Mass
0.39 Msun
0.39 to 0.40
Distance
6380 pc
6380 to 6400
Planets
2
Stable across source rows
System Layout
2 planets linked to this host
Microlensing
Discovery
2018
Period
โ
Radius
โ
Mass
55.30 Mโ
Eq. Temp
โ
Microlensing
Discovery
2018
Period
โ
Radius
โ
Mass
83.70 Mโ
Eq. Temp
โ
OGLE-2014-BLG-1722L is a star 20800 light-years away with two known planets. Its reported mass estimate is 0.39 solar masses, smaller than the Sun's.
Both planets were discovered in 2018 by microlensing, a method that reveals a planet through the way its gravity bends light from a background source. The first, OGLE-2014-BLG-1722L b, has a reported mass estimate of 55.3 Earth masses, larger than Earth's, and among the listed planets it has the smallest reported mass. No orbital period is reported for it. The second, OGLE-2014-BLG-1722L c, has a reported mass estimate of 83.7 Earth masses, larger than Earth's, and among the listed planets it has the largest reported mass. No orbital period is reported for it either.
Provenance
Evidence Summary
Rows
2
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 | 0.40 | โ | โ | โ | โ | 6400 | Suzuki et al. 2018 | Suzuki et al. 2018 |
| โ | 0.39 | โ | โ | โ | โ | 6380 | Suzuki et al. 2018 | Suzuki et al. 2018 |