←Back to Stellar Hosts
Stellar HostProfile

TOI-6383 A

M3 • 171.3 pc

Records

3

literature rows

Planets

1

system count

References

4

distinct source labels

TIC: TIC 328513434

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: Bernabò et al. 2024 • System source: TICv8

Temperature

3444 K

3425 to 3444

3 values • 2 distinct

Mass

0.46 Msun

0.45 to 0.46

2 values • 2 distinct

Radius

0.46 Rsun

0.46 to 0.46

3 values • 3 distinct

Luminosity

-1.49 log(Lsun)

-1.59 to -1.49

2 values • 2 distinct

Distance

171.3 pc

single adopted value

3 values • 1 distinct

Spectral Type

M3

Consistent across records

M3 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.46 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-6383 A

0.46 R☉

System Layout

Known planets

1 planets linked to this host

◌

Discovery

2024

Period

1.79 days

Radius

11.29 R⊕

Mass

331 M⊕

Eq. Temp

745 K

TOI-6383 A b: A Close-Orbiting Giant Around a Cool Dwarf

TOI-6383 A is an M3 host star 559 light-years away. The star's reported mass estimate is 0.458 solar masses, its reported radius estimate is 0.457 solar radii, and its reported temperature is 3440 K. These stellar measurements describe the host star alone rather than the whole stellar system. The star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's. Its spectral type places it among the small, cool red dwarfs. One planet is known to orbit this host.

TOI-6383 A b is a Jupiter-like planet discovered by transit in 2024. Its reported radius estimate is 11.3 Earth radii, larger than Earth's, and its reported mass estimate is 331 Earth masses, also larger than Earth's. A Jupiter-like classification means its radius exceeds four times Earth's radius. Its mean density is 1.27 g/cm³, 0.23 times Earth's. It completes an orbit in 1.79 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

3

Stellar refs

3

System refs

1

Distancestable

3 values • 1 distinct

Parallaxstable

3 values • 1 distinct

Temperaturedisputed

3 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 3 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
3425—0.46———171.3ExoFOPTICv8
34440.460.46—-1.49M3171.3Bernabò et al. 2024TICv8
34250.450.46—-1.59—171.3TICv8TICv8