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Stellar HostProfile

HD 36384

M0 III • 209.3 pc

Records

2

literature rows

Planets

1

system count

References

3

distinct source labels

HD: HD 36384HIP: HIP 26638TIC: TIC 418343111

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: Lee et al. 2023 • System source: TICv8

Temperature

3940 K

3940 to 3989

2 values • 2 distinct

Mass

1.14 Msun

single adopted value

1 values • 1 distinct

Radius

38.40 Rsun

38.40 to 43.57

2 values • 2 distinct

Age

0.11 Gyr

single adopted value

1 values • 1 distinct

Luminosity

2.59 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

209.3 pc

single adopted value

2 values • 1 distinct

Spectral Type

M0 III

Consistent across records

M0 III (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 38.40 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 36384

38.40 R☉

System Layout

Known planets

1 planets linked to this host

HD 36384 b

Radial Velocity

◌

Discovery

2023

Period

490 days

Radius

—

Mass

2097.7 M⊕

Eq. Temp

—

HD 36384 b: A Massive World Orbiting a Red Giant

HD 36384 is a single star located 683 light-years away, and its only known planet is HD 36384 b. The host is classified as an M0 III star, placing it among the cooler, redder stars. Its spectral type suggests it has evolved off the main sequence into the giant stage. The star has a mass of 1.14 solar masses, a radius of 38.4 solar radii, and a temperature of 3940 K. Its radius is larger than the Sun's, while its temperature is cooler than the Sun's. The star's age is 0.113 billion years.

HD 36384 b was discovered in 2023 using the radial velocity method. The radial velocity method detects the wobble a planet's gravity induces in its star's motion, with repeated wobbles revealing the planet and its orbital period. The planet's orbital period is 490 days. HD 36384 b has a minimum mass of 2100 Earth masses, meaning its true mass is at least that value. Its minimum mass is larger than Earth's and roughly 6.6 times Jupiter's mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

2

Stellar refs

2

System refs

1

Distancestable

2 values • 1 distinct

Parallaxstable

2 values • 1 distinct

Temperaturedisputed

2 values • 2 distinct

Massstable

1 values • 1 distinct

Radiusdisputed

2 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositystable

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
39401.1438.400.112.59M0 III209.3Lee et al. 2023TICv8
3989—43.57———209.3TICv8TICv8