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Stellar HostProfile

HD 85390

K0 • 33.52 pc

Records

11

literature rows

Planets

1

system count

References

12

distinct source labels

HIP: HIP 48235TIC: TIC 446137194HD: HD 85390

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

5175 K

5152.5 to 5186

6 values • 4 distinct

Mass

0.76 Msun

0.54 to 0.87

5 values • 4 distinct

Radius

0.82 Rsun

0.80 to 0.83

3 values • 3 distinct

Age

7.20 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-0.37 log(Lsun)

-0.37 to -0.36

4 values • 4 distinct

Distance

33.52 pc

single adopted value

11 values • 1 distinct

Spectral Type

K0

Multiple classifications reported

K0 (1), K1 V (1), K1.5 V (1)

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

HD 85390 b

Radial Velocity

Discovery

2009

Period

788 days

Radius

Mass

42 M⊕

Eq. Temp

Provenance

Underlying measurements and references

Evidence Summary

Rows

11

Stellar refs

11

System refs

1

Distancestable

11 values • 1 distinct

Parallaxstable

11 values • 1 distinct

Temperaturedisputed

6 values • 4 distinct

Massdisputed

5 values • 4 distinct

Radiusdisputed

3 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

5 values • 3 distinct

Metallicitydisputed

4 values • 3 distinct

Spectral Typedisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
51860.76-0.3733.52Sousa et al. 2008TICv8
K1.5 V33.52Gray et al. 2006TICv8
33.52Nordstrom et al. 2004TICv8
51860.7633.52Wittenmyer et al. 2019TICv8
51860.767.20-0.3733.52Mordasini et al. 2011TICv8
5152.50.83-0.3633.52Gaia DR2TICv8
33.52Henry et al. 1996TICv8
K1 V33.52Michigan Catalog, Vol. 2TICv8
K033.52Cannon & Pickering 1918TICv8
5160.60.870.82-0.3733.52TICv8TICv8
51640.540.8033.52Stassun et al. 2017TICv8