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Stellar HostProfile

HIP 38594

Unclassified star • 17.79 pc

Records

4

literature rows

Planets

2

system count

References

5

distinct source labels

HIP: HIP 38594TIC: TIC 128902569

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: TICv8 • System source: TICv8

Temperature

3969 K

3954 to 4086.3

3 values • 3 distinct

Mass

0.61 Msun

0.57 to 0.61

3 values • 3 distinct

Radius

0.63 Rsun

0.59 to 0.71

3 values • 3 distinct

Luminosity

-1.06 log(Lsun)

-1.06 to -0.96

3 values • 3 distinct

Distance

17.79 pc

single adopted value

4 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.63 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HIP 38594

0.63 R☉

System Layout

Known planets

2 planets linked to this host

HIP 38594 b

Radial Velocity

◌

Discovery

2020

Period

60.72 days

Radius

—

Mass

8.10 M⊕

Eq. Temp

—

HIP 38594 c

Radial Velocity

◌

Discovery

2020

Period

3477.8 days

Radius

—

Mass

48.40 M⊕

Eq. Temp

—

HIP 38594: A Nearby Red Dwarf and Its Two Known Planets

HIP 38594 is a star 58 light-years away with a spectral type of M0, placing it among the small, cool red dwarfs. Its mass is 0.609 solar masses and its radius is 0.627 solar radii, both smaller than the Sun's corresponding values, while its temperature of 3970 K is cooler than the Sun's. Two planets are known to orbit this host.

Both planets were discovered in 2020 using the radial velocity method, which detects the gravitational wobble a planet induces in its star's motion; repeated wobbles reveal the planet and its orbital period. HIP 38594 b has a minimum mass of 8.1 Earth masses and an orbital period of 60.7 days, giving it the shortest year among the listed planets. HIP 38594 c has a minimum mass of 48.4 Earth masses and an orbital period of 3480 days, the longest year among the listed planets. Of the two, HIP 38594 b has the smallest minimum mass and HIP 38594 c the largest, and both minimum masses are larger than Earth's. The companion star's properties are not represented in these figures, which describe the host alone.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

4

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

3 values • 3 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

3 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitystable

1 values • 1 distinct

Spectral Typedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
4086.3—0.59—-1.06—17.79Gaia DR2TICv8
39690.610.63—-1.06—17.79TICv8TICv8
39540.570.71—-0.96M17.79Turnbull 2015TICv8
—0.61———M017.79Feng et al. 2020TICv8