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Stellar HostProfile

HD 148164

F8 • 77.20 pc

Records

5

literature rows

Planets

2

system count

References

6

distinct source labels

HIP: HIP 80484HD: HD 148164TIC: TIC 323319664

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: Ment et al. 2018 • System source: TICv8

Temperature

6032 K

6022 to 6032

3 values • 2 distinct

Mass

1.21 Msun

1.12 to 1.21

2 values • 2 distinct

Radius

1.34 Rsun

1.34 to 1.47

3 values • 3 distinct

Age

2.41 Gyr

single adopted value

1 values • 1 distinct

Luminosity

0.33 log(Lsun)

0.33 to 0.41

3 values • 3 distinct

Distance

77.20 pc

single adopted value

5 values • 1 distinct

Spectral Type

F8

Consistent across records

F8 (2)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.34 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 148164

1.34 R☉

System Layout

Known planets

2 planets linked to this host

HD 148164 b

Radial Velocity

◌

Discovery

2018

Period

328.6 days

Radius

—

Mass

390.9 M⊕

Eq. Temp

—

HD 148164 c

Radial Velocity

◌

Discovery

2018

Period

5062 days

Radius

—

Mass

1640.0 M⊕

Eq. Temp

—

HD 148164: A Distant Star With Two Known Worlds

HD 148164 is a star 252 light-years away with two known planets. Its spectral type is F8, placing it among the hotter, more massive stars than the Sun. The star is 2.41 billion years old, contains 1.21 solar masses, spans 1.34 solar radii, and has a temperature of 6030 K. Its radius and temperature both exceed the Sun's.

Both planets were discovered in 2018 using the radial velocity method, which detects the gravitational wobble a planet induces in its star's motion. HD 148164 b has a minimum mass of 391 Earth masses and an orbital period of 329 days. HD 148164 c has a minimum mass of 1640 Earth masses and an orbital period of 5060 days. The minimum mass of each planet is larger than Earth's, and the minimum mass of HD 148164 c is roughly 5.16 times Jupiter's mass. Among the listed planets, HD 148164 b has the shortest year by reported estimates, while HD 148164 c has the longest; b also has the smallest minimum mass and c the largest.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

5

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

3 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

3 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitystable

1 values • 1 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

2 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
60321.121.46—0.41—77.20TICv8TICv8
6022—1.47—0.41—77.20Gaia DR2TICv8
60321.211.342.410.33F877.20Ment et al. 2018TICv8
——————77.20Nordstrom et al. 2004TICv8
—————F877.20Cannon & Pickering 1918TICv8