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Stellar HostProfile

OGLE-2019-BLG-0468L

G • 4400 pc

Records

4

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

Mass

0.92 Msun

single adopted value

2 values • 1 distinct

Distance

4400 pc

single adopted value

2 values • 1 distinct

Spectral Type

G

Consistent across records

G (4)

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

Two Microlensing Planets Around a Sun-Like Star

OGLE-2019-BLG-0468L is a G-type star with a mass of 0.92 solar masses, located 14400 light-years away. Two planets are known to orbit it, both discovered in 2022 by microlensing.

The inner-listed planet, OGLE-2019-BLG-0468L b, has a reported mass estimate of 1090 Earth masses, roughly 3.43 times Jupiter's mass. Its companion, OGLE-2019-BLG-0468L c, has a reported mass estimate of 3250 Earth masses, roughly 10.2 times Jupiter's mass. Both figures exceed Earth's mass, and among the listed planets b has the smallest reported mass while c has the largest. No orbital period is reported for either OGLE-2019-BLG-0468L b or OGLE-2019-BLG-0468L c.

Provenance

Underlying measurements and references

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Evidence Summary

Rows

4

Stellar refs

1

System refs

1

Distancestable

2 values • 1 distinct

Massstable

2 values • 1 distinct

Spectral Typestable

4 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.92———G4400Han et al. 2022Han et al. 2022
—0.92———G4400Han et al. 2022Han et al. 2022
—————G—Han et al. 2022Han et al. 2022
—————G—Han et al. 2022Han et al. 2022