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Stellar HostProfile

XEST 17-036

M4 • 158.6 pc

Records

1

literature rows

Planets

1

system count

References

2

distinct source labels

TIC: TIC 61229372

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: Walker et al. 2026 • System source: TICv8

Temperature

3551 K

single adopted value

1 values • 1 distinct

Mass

0.26 Msun

single adopted value

1 values • 1 distinct

Age

3.30e-3 Gyr

single adopted value

1 values • 1 distinct

Distance

158.6 pc

single adopted value

1 values • 1 distinct

Spectral Type

M4

Consistent across records

M4 (1)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

◌

Discovery

2026

Period

—

Radius

—

Mass

3369.0 M⊕

Eq. Temp

—

XEST 17-036 and Its Young World

XEST 17-036 is a star 517 light-years away with a spectral type of M4, placing it among the small, cool red dwarfs. Its reported mass of 0.26 solar masses is smaller than the Sun's, and its temperature of 3550 K is cooler than the Sun's. At 0.0033 billion years old, it is a very young star. One planet is known to orbit this host.

That planet, KOINTREAU-1 b, was found by imaging in 2026. Its reported mass of 3370 Earth masses is larger than Earth's and roughly 10.6 times Jupiter's mass. No orbital period is reported for KOINTREAU-1 b.

Provenance

Underlying measurements and references

Evidence Summary

Rows

1

Stellar refs

1

System refs

1

Distancestable

1 values • 1 distinct

Parallaxstable

1 values • 1 distinct

Temperaturestable

1 values • 1 distinct

Massstable

1 values • 1 distinct

Agestable

1 values • 1 distinct

Surface Gravitystable

1 values • 1 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
35510.26—3.30e-3—M4158.6Walker et al. 2026TICv8