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Stellar HostProfile

HD 37605

K0 • 46.79 pc

Records

9

literature rows

Planets

2

system count

References

10

distinct source labels

TIC: TIC 144730053HD: HD 37605HIP: HIP 26664

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

5340 K

5304 to 5475

7 values • 6 distinct

Mass

0.97 Msun

0.68 to 1

6 values • 4 distinct

Radius

0.93 Rsun

0.86 to 0.99

6 values • 6 distinct

Age

5.65 Gyr

1 to 7

3 values • 3 distinct

Luminosity

-0.22 log(Lsun)

-0.24 to -0.15

5 values • 5 distinct

Distance

46.79 pc

single adopted value

9 values • 1 distinct

Spectral Type

K0

Multiple classifications reported

K0 (2), K0 V (1)

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

HD 37605 c

Radial Velocity

Discovery

2012

Period

2720 days

Radius

Mass

1013.9 M⊕

Eq. Temp

HD 37605 b

Radial Velocity

Discovery

2004

Period

54.21 days

Radius

Mass

Eq. Temp

Provenance

Underlying measurements and references

Evidence Summary

Rows

9

Stellar refs

9

System refs

1

Distancestable

9 values • 1 distinct

Parallaxstable

9 values • 1 distinct

Temperaturedisputed

7 values • 6 distinct

Massdisputed

6 values • 4 distinct

Radiusdisputed

6 values • 6 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

5 values • 5 distinct

Surface Gravitydisputed

5 values • 5 distinct

Metallicitydisputed

6 values • 6 distinct

Spectral Typedisputed

3 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
146.79Bryan et al. 2016TICv8
53290.920.98-0.1546.79TICv8TICv8
53290.940.915.65-0.22K046.79Ment et al. 2018TICv8
K046.79Cannon & Pickering 1918TICv8
544810.907-0.23K0 V46.79Wang et al. 2012TICv8
540510.861-0.2446.79Ghezzi et al. 2010TICv8
547546.79Cochran et al. 2004TICv8
53040.99-0.1546.79Gaia DR2TICv8
53400.680.9546.79Stassun et al. 2017TICv8