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Stellar HostProfile

KMT-2024-BLG-0404L

M • 7210 pc

Records

1

literature rows

Planets

2

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. 2025 • System source: Han et al. 2025

Mass

0.09 Msun

single adopted value

1 values • 1 distinct

Distance

7210 pc

single adopted value

1 values • 1 distinct

Spectral Type

M

Consistent across records

M (1)

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

Two Microlensing Planets Around a Distant Red Dwarf

KMT-2024-BLG-0404L is an M-type star, a small, cool red dwarf with a reported mass estimate of 0.09 solar masses, smaller than the Sun's. It lies 23500 light-years away and hosts two known planets, both discovered by microlensing in 2025.

The larger of the two is KMT-2024-BLG-0404L b, whose reported mass estimate is 8660 Earth masses, larger than Earth's and roughly 27.2 times Jupiter's mass. Among the listed planets, it has the largest reported mass. No orbital period is reported for it.

Its companion is KMT-2024-BLG-0404L c, with a reported mass estimate of 17.3 Earth masses, larger than Earth's and the smallest reported mass among the listed planets. No orbital period is reported for it either.

Provenance

Underlying measurements and references

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Evidence Summary

Rows

1

Stellar refs

1

System refs

1

Distancestable

1 values • 1 distinct

Massstable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.09———M7210Han et al. 2025Han et al. 2025