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Stellar HostProfile

HD 164604

K3.5 V • 39.36 pc

Records

10

literature rows

Planets

2

system count

References

11

distinct source labels

TIC: TIC 406317882HIP: HIP 88414HD: HD 164604

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: Xiao et al. 2026 • System source: TICv8

Temperature

4663 K

4663 to 4806.8

5 values • 3 distinct

Mass

0.77 Msun

0.77 to 0.80

5 values • 3 distinct

Radius

0.78 Rsun

0.72 to 0.78

3 values • 3 distinct

Age

1.60 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-0.59 log(Lsun)

-0.61 to -0.59

3 values • 3 distinct

Distance

39.36 pc

single adopted value

10 values • 1 distinct

Spectral Type

K3.5 V

Multiple classifications reported

K3.5 V (2), K0 (1), K1/3 (1), K2 V (1), K3.5 V (k) (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.78 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 164604

0.78 R☉

System Layout

Known planets

2 planets linked to this host

HD 164604 b

Radial Velocity

◌

Discovery

2009

Period

653.9 days

Radius

—

Mass

4195.3 M⊕

Eq. Temp

—

HD 164604 c

Radial Velocity

◌

Discovery

2026

Period

5387 days

Radius

—

Mass

3019.4 M⊕

Eq. Temp

—

HD 164604 and Its Two Known Planets

HD 164604 is a K3.5 V star located 128 light-years away. Its spectral type marks it as a main-sequence dwarf, and it is the only star in its system. The star is 1.6 billion years old and has a mass of 0.77 solar masses, a radius of 0.78 solar radii, and a temperature of 4660 K. Its reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's. Two planets are known to orbit this host.

HD 164604 b was discovered in 2009 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. It has a mass of 4200 Earth masses and an orbital period of 654 days. Its reported mass estimate is larger than Earth's and roughly 13.2 times Jupiter's mass. Among the listed planets, it has the shortest year by reported estimates and the largest reported mass.

HD 164604 c was discovered in 2026, also by radial velocity. It has a mass of 3020 Earth masses and an orbital period of 5390 days. Its reported mass estimate is larger than Earth's and roughly 9.5 times Jupiter's mass. Among the listed planets, it has the longest year by reported estimates and the smallest reported mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

10

Stellar refs

10

System refs

1

Distancestable

10 values • 1 distinct

Parallaxstable

10 values • 1 distinct

Temperaturedisputed

5 values • 3 distinct

Massdisputed

5 values • 3 distinct

Radiusdisputed

3 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

3 values • 3 distinct

Metallicitydisputed

4 values • 2 distinct

Spectral Typedisputed

6 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
46840.77————39.36Santos et al. 2013TICv8
—————K3.5 V (k)39.36Gray et al. 2006TICv8
4806.80.780.72—-0.61—39.36TICv8TICv8
——————39.36Nordstrom et al. 2004TICv8
—————K039.36Cannon & Pickering 1918TICv8
—0.80———K2 V39.36Arriagada et al. 2010TICv8
46840.77———K3.5 V39.36Feng et al. 2019TICv8
—————K1/339.36Michigan Catalog, Vol. 3TICv8
46630.770.781.60-0.59K3.5 V39.36Xiao et al. 2026TICv8
4684—0.77—-0.59—39.36Gaia DR2TICv8