โ†Back to Stellar Hosts
Stellar HostProfile

OGLE-2012-BLG-0950L

M V โ€ข 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: Koshimoto et al. 2017 โ€ข System source: Koshimoto et al. 2017

Mass

0.57 Msun

0.31 to 0.63

12 values โ€ข 9 distinct

Distance

2600 pc

2400 to 4200

12 values โ€ข 7 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

โ—Œ

Discovery

2016

Period

โ€”

Radius

โ€”

Mass

35 MโŠ•

Eq. Temp

โ€”

The Distant Microlensing System OGLE-2012-BLG-0950L

OGLE-2012-BLG-0950L is a star located 8480 light-years away. It is an M V star, a small, cool red dwarf, with a reported mass of 0.57 solar masses, smaller than the Sun's. One planet is known to orbit it.

That planet, OGLE-2012-BLG-0950L b, was discovered in 2016 by microlensing. It has a reported mass of 35 Earth masses, larger than Earth's, and no orbital period is reported for it.

Provenance

Underlying measurements and references

Download JSONDownload CSV

Evidence Summary

Rows

12

Stellar refs

1

System refs

1

Distancedisputed

12 values โ€ข 7 distinct

Massdisputed

12 values โ€ข 9 distinct

Spectral Typestable

1 values โ€ข 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
โ€”0.55โ€”โ€”โ€”โ€”3400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.57โ€”โ€”โ€”M V2600Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.63โ€”โ€”โ€”โ€”3200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.55โ€”โ€”โ€”โ€”3400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.63โ€”โ€”โ€”โ€”3200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.33โ€”โ€”โ€”โ€”3600Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.38โ€”โ€”โ€”โ€”4200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.31โ€”โ€”โ€”โ€”3400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.47โ€”โ€”โ€”โ€”2600Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.54โ€”โ€”โ€”โ€”2400Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.38โ€”โ€”โ€”โ€”4200Koshimoto et al. 2017Koshimoto et al. 2017
โ€”0.50โ€”โ€”โ€”โ€”2900Koshimoto et al. 2017Koshimoto et al. 2017