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Stellar HostProfile

KMT-2016-BLG-1337L

M • 6920 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: Han et al. 2026 • System source: Han et al. 2026

Mass

0.54 Msun

single adopted value

2 values • 1 distinct

Distance

6920 pc

6920 to 6950

2 values • 2 distinct

Spectral Type

M

Consistent across records

M (2)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

A Microlensing Planet Around KMT-2016-BLG-1337L

KMT-2016-BLG-1337L is an M-type star, a small, cool red dwarf, located 22,600 light-years away. Its reported mass estimate is 0.54 solar masses, smaller than the Sun's. One planet is known to orbit this host.

That planet is KMT-2016-BLG-1337L b, a circumbinary planet, meaning it orbits both stars of a binary system rather than one star alone. It was discovered by microlensing in 2026 and has a reported mass estimate of 89 Earth masses, larger than Earth's. No orbital period is reported for the planet.

Provenance

Underlying measurements and references

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Evidence Summary

Rows

2

Stellar refs

1

System refs

1

Distancedisputed

2 values • 2 distinct

Massstable

2 values • 1 distinct

Spectral Typestable

2 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.54———M6920Han et al. 2026Han et al. 2026
—0.54———M6950Han et al. 2026Han et al. 2026