Back to Stellar Hosts
Stellar HostProfile

HD 102329

K0 • 217.1 pc

Records

8

literature rows

Planets

2

system count

References

9

distinct source labels

HD: HD 102329HIP: HIP 57467TIC: TIC 325254372

Approximate color

from effective temperature

Canonical Summary

Adopted host values from all rows

Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.

Temperature

4773.7 K

4745 to 4830

5 values • 4 distinct

Mass

1.62 Msun

1.30 to 3.21

4 values • 3 distinct

Radius

9.08 Rsun

6.30 to 9.82

4 values • 4 distinct

Age

1.60 Gyr

single adopted value

1 values • 1 distinct

Luminosity

1.44 log(Lsun)

1.29 to 1.59

2 values • 2 distinct

Distance

217.1 pc

single adopted value

8 values • 1 distinct

Spectral Type

K0

Multiple classifications reported

K0 (1), K0 III (1)

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

HD 102329 c

Radial Velocity

Discovery

2018

Period

1123 days

Radius

Mass

483.1 M⊕

Eq. Temp

HD 102329 b

Radial Velocity

Discovery

2011

Period

778.1 days

Radius

Mass

1875.1 M⊕

Eq. Temp

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values • 1 distinct

Parallaxstable

8 values • 1 distinct

Temperaturedisputed

5 values • 4 distinct

Massdisputed

4 values • 3 distinct

Radiusdisputed

4 values • 4 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitydisputed

3 values • 2 distinct

Spectral Typedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
47453.219.82217.1Stassun et al. 2017TICv8
K0 III217.1Michigan Catalog, Vol. 5TICv8
48301.956.301.601.29217.1Johnson et al. 2011TICv8
48139.10217.1TICv8TICv8
4773.79.071.59217.1Gaia DR2TICv8
K0217.1Cannon & Pickering 1918TICv8
47451.30217.1Mortier et al. 2013TICv8
1.30217.1Bryan et al. 2016TICv8