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Stellar HostProfile

OGLE-2012-BLG-0724L

M V • 6700 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: Hirao et al. 2016 • System source: Hirao et al. 2016

Mass

0.29 Msun

single adopted value

2 values • 1 distinct

Distance

6700 pc

single adopted value

2 values • 1 distinct

Spectral Type

M V

Consistent across records

M V (1)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

OGLE-2012-BLG-0724L b: A Microlensing World in the Galactic Distance

OGLE-2012-BLG-0724L is a host star 21900 light-years away with one known planet. The star is an M V spectral type, a small, cool red dwarf with a mass of 0.29 solar masses, which is smaller than the Sun's mass.

The planet OGLE-2012-BLG-0724L b was discovered in 2016 by microlensing and has a reported mass of 150 Earth masses, larger than Earth's mass. No orbital period is reported for OGLE-2012-BLG-0724L 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
—0.29———M V6700Hirao et al. 2016Hirao et al. 2016
—0.29————6700Hirao et al. 2016Hirao et al. 2016