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Stellar HostProfile

OGLE-2014-BLG-1722L

Unclassified star โ€ข 6380 pc

Records

2

literature rows

Planets

2

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: Suzuki et al. 2018 โ€ข System source: Suzuki et al. 2018

Mass

0.39 Msun

0.39 to 0.40

2 values โ€ข 2 distinct

Distance

6380 pc

6380 to 6400

2 values โ€ข 2 distinct

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

โ—Œ

Discovery

2018

Period

โ€”

Radius

โ€”

Mass

55.30 MโŠ•

Eq. Temp

โ€”

โ—Œ

Discovery

2018

Period

โ€”

Radius

โ€”

Mass

83.70 MโŠ•

Eq. Temp

โ€”

OGLE-2014-BLG-1722L and Its Two Planets

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

Underlying measurements and references

Evidence Summary

Rows

2

Stellar refs

1

System refs

1

Distancedisputed

2 values โ€ข 2 distinct

Massdisputed

2 values โ€ข 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
โ€”0.40โ€”โ€”โ€”โ€”6400Suzuki et al. 2018Suzuki et al. 2018
โ€”0.39โ€”โ€”โ€”โ€”6380Suzuki et al. 2018Suzuki et al. 2018