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Stellar HostProfile

MOA-2019-BLG-008L

Unclassified star • 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: Bachelet et al. 2022 • System source: Bachelet et al. 2022

Mass

0.50 Msun

0.50 to 1.10

12 values • 6 distinct

Distance

2600 pc

2200 to 3500

12 values • 8 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

MOA-2019-BLG-008L b: A Microlensing Discovery

MOA-2019-BLG-008L is a star 8480 light-years from Earth with a reported mass estimate of 0.5 solar masses, smaller than the Sun's. One planet is known to orbit it.

That planet, MOA-2019-BLG-008L b, was discovered by microlensing in 2022. Its reported mass estimate is 5720 Earth masses, larger than Earth's and roughly 18 times Jupiter's mass. No orbital period is reported for MOA-2019-BLG-008L b.

Provenance

Underlying measurements and references

Evidence Summary

Rows

12

Stellar refs

1

System refs

1

Distancedisputed

12 values • 8 distinct

Massdisputed

12 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.60————2200Bachelet et al. 2022Bachelet et al. 2022
—0.60————2300Bachelet et al. 2022Bachelet et al. 2022
—0.50————2600Bachelet et al. 2022Bachelet et al. 2022
—1.10————3200Bachelet et al. 2022Bachelet et al. 2022
—1.10————3500Bachelet et al. 2022Bachelet et al. 2022
—0.80————2600Bachelet et al. 2022Bachelet et al. 2022
—0.80————2400Bachelet et al. 2022Bachelet et al. 2022
—0.70————2600Bachelet et al. 2022Bachelet et al. 2022
—0.60————2600Bachelet et al. 2022Bachelet et al. 2022
—0.90————2700Bachelet et al. 2022Bachelet et al. 2022
—0.90————2800Bachelet et al. 2022Bachelet et al. 2022
—0.60————2600Bachelet et al. 2022Bachelet et al. 2022