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Stellar HostProfile

HD 43197

G8 V • 62.41 pc

Records

6

literature rows

Planets

2

system count

References

7

distinct source labels

HD: HD 43197HIP: HIP 29550TIC: TIC 37660988

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: Naef et al. 2010 • System source: TICv8

Temperature

5508 K

5476.8 to 5508

3 values • 3 distinct

Mass

0.96 Msun

single adopted value

3 values • 1 distinct

Radius

1 Rsun

1 to 1.07

3 values • 3 distinct

Luminosity

-0.14 log(Lsun)

-0.14 to -0.03

3 values • 3 distinct

Distance

62.41 pc

single adopted value

6 values • 1 distinct

Spectral Type

G8 V

Multiple classifications reported

G5 (1), G8 V (1), G8/K0 IV/V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 43197

1 R☉

System Layout

Known planets

2 planets linked to this host

HD 43197 b

Radial Velocity

◌

Discovery

2010

Period

308.9 days

Radius

—

Mass

175.8 M⊕

Eq. Temp

—

HD 43197 c

Radial Velocity

◌

Discovery

2022

Period

9296.0 days

Radius

—

Mass

2500.7 M⊕

Eq. Temp

—

HD 43197 and Its Two Known Planets

HD 43197 is a G8 V star 204 light-years away. Its temperature is 5510 K, and its reported temperature is cooler than the Sun's. The star's mass estimate is 0.96 solar masses, smaller than the Sun's, and its radius is 1 solar radii.

Two planets are known to orbit HD 43197. HD 43197 b was discovered in 2010 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. It has a minimum mass of 176 Earth masses, larger than Earth's, and an orbital period of 309 days, the shortest year among the listed planets. HD 43197 c was discovered in 2022, also by radial velocity. Its mass estimate is 2500 Earth masses, larger than Earth's and roughly 7.87 times Jupiter's mass. Its orbital period is 9300 days, the longest year among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

6

Stellar refs

6

System refs

1

Distancestable

6 values • 1 distinct

Parallaxstable

6 values • 1 distinct

Temperaturedisputed

3 values • 3 distinct

Massstable

3 values • 1 distinct

Radiusdisputed

3 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typedisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5478.60.961.07—-0.04—62.41TICv8TICv8
—0.96————62.41Feng et al. 2022TICv8
55080.961—-0.14G8 V62.41Naef et al. 2010TICv8
—————G562.41Cannon & Pickering 1918TICv8
—————G8/K0 IV/V62.41Michigan Catalog, Vol. 3TICv8
5476.8—1.07—-0.03—62.41Gaia DR2TICv8