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Stellar HostProfile

MOA-2008-BLG-379L

K • 3300 pc

Records

2

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: Suzuki et al. 2014 • System source: Suzuki et al. 2014

Mass

0.56 Msun

single adopted value

2 values • 1 distinct

Distance

3300 pc

single adopted value

2 values • 1 distinct

Spectral Type

K

Consistent across records

K (1)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

MOA-2008-BLG-379L b: A Microlensing Discovery

MOA-2008-BLG-379L is a K-type star with a reported mass estimate of 0.56 solar masses, smaller than the Sun's. It lies 10800 light-years away and hosts one known planet, found by microlensing in 2013.

That planet, MOA-2008-BLG-379L b, has a reported mass estimate of 1300 Earth masses, larger than Earth's and roughly 4.09 times Jupiter's mass. No orbital period is reported for MOA-2008-BLG-379L b.

Provenance

Underlying measurements and references

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Evidence Summary

Rows

2

Stellar refs

1

System refs

1

Distancestable

2 values • 1 distinct

Massstable

2 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.56———K3300Suzuki et al. 2014Suzuki et al. 2014
—0.56————3300Suzuki et al. 2014Suzuki et al. 2014