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Stellar HostProfile

HD 33844

K0 III • 105.8 pc

Records

8

literature rows

Planets

2

system count

References

9

distinct source labels

TIC: TIC 169534187HIP: HIP 24275HD: HD 33844

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

4888.1 K

4861 to 4925

5 values • 4 distinct

Mass

1.67 Msun

1.47 to 1.84

4 values • 4 distinct

Radius

5.39 Rsun

5.29 to 5.51

6 values • 5 distinct

Age

2.15 Gyr

1.88 to 2.42

2 values • 2 distinct

Luminosity

1.17 log(Lsun)

1.15 to 1.18

4 values • 4 distinct

Distance

105.8 pc

single adopted value

8 values • 1 distinct

Spectral Type

K0 III

Multiple classifications reported

K0 III (3), G5 (1)

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

HD 33844 b

Radial Velocity

Discovery

2015

Period

551.7 days

Radius

Mass

1497.0 M⊕

Eq. Temp

HD 33844 c

Radial Velocity

Discovery

2015

Period

916 days

Radius

Mass

556.2 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 • 4 distinct

Radiusdisputed

6 values • 5 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

4 values • 2 distinct

Metallicitydisputed

3 values • 2 distinct

Spectral Typedisputed

4 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
4888.15.381.17105.8Gaia DR2TICv8
49091.555.392.421.17K0 III105.8Jenkins et al. 2025TICv8
G5105.8Cannon & Pickering 1918TICv8
49255.37105.8TICv8TICv8
K0 III105.8Michigan Catalog, Vol. 4TICv8
1.475.511.18105.8Lin et al. 2024TICv8
48611.785.291.881.15K0 III105.8Wittenmyer et al. 2016TICv8
48611.845.39105.8Stassun et al. 2017TICv8