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Stellar HostProfile

KMT-2018-BLG-0247L

Unclassified star • 6840 pc

Records

3

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: Jung et al. 2022 • System source: Jung et al. 2022

Mass

0.27 Msun

0.27 to 0.35

3 values • 3 distinct

Distance

6840 pc

6470 to 6840

3 values • 3 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

A Microlensing Planet Around KMT-2018-BLG-0247L

KMT-2018-BLG-0247L is a star 22300 light-years away with a reported mass estimate of 0.27 solar masses, smaller than the Sun's. One planet is known to orbit it.

That planet, KMT-2018-BLG-0247L b, was discovered in 2022 by microlensing, a method that reveals a planet through the gravitational deflection of light from a background source. Its reported mass estimate is 671 Earth masses, larger than Earth's and roughly 2.11 times Jupiter's mass. No orbital period is reported for KMT-2018-BLG-0247L b.

Provenance

Underlying measurements and references

Evidence Summary

Rows

3

Stellar refs

1

System refs

1

Distancedisputed

3 values • 3 distinct

Massdisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.35————6470Jung et al. 2022Jung et al. 2022
—0.27————6840Jung et al. 2022Jung et al. 2022
—0.29————6760Jung et al. 2022Jung et al. 2022