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Stellar HostProfile

OGLE-2015-BLG-0966L

Unclassified star โ€ข 2500 pc

Records

16

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: Street et al. 2016 โ€ข System source: Street et al. 2016

Mass

0.38 Msun

single adopted value

16 values โ€ข 1 distinct

Distance

2500 pc

2500 to 3300

16 values โ€ข 2 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

โ—Œ

Discovery

2016

Period

โ€”

Radius

โ€”

Mass

21 MโŠ•

Eq. Temp

โ€”

A Microlensed Planet Around OGLE-2015-BLG-0966L

OGLE-2015-BLG-0966L is a star 8150 light-years away with a reported mass estimate of 0.38 solar masses, smaller than the Sun's. One planet is known to orbit this star.

That planet, OGLE-2015-BLG-0966L b, was discovered in 2016 by microlensing, a method that reveals a planet through the gravitational deflection of a background star's light. Its reported mass estimate is 21 Earth masses, larger than Earth's. No orbital period is reported for OGLE-2015-BLG-0966L b.

Provenance

Underlying measurements and references

Evidence Summary

Rows

16

Stellar refs

1

System refs

1

Distancedisputed

16 values โ€ข 2 distinct

Massstable

16 values โ€ข 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”3300Street et al. 2016Street et al. 2016
โ€”0.38โ€”โ€”โ€”โ€”2500Street et al. 2016Street et al. 2016