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Stellar HostProfile

HD 47186

Unclassified star โ€ข 37.46 pc

Records

10

literature rows

Planets

2

system count

References

11

distinct source labels

HIP: HIP 31540HD: HD 47186TIC: TIC 101145648

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: Ghezzi et al. 2010 โ€ข System source: TICv8

Temperature

5640 K

5640 to 5685

5 values โ€ข 5 distinct

Mass

1 Msun

0.96 to 1

4 values โ€ข 3 distinct

Radius

1.13 Rsun

1.08 to 1.13

4 values โ€ข 4 distinct

Age

6.50 Gyr

single adopted value

1 values โ€ข 1 distinct

Luminosity

0.07 log(Lsun)

0.03 to 0.07

4 values โ€ข 4 distinct

Distance

37.46 pc

single adopted value

10 values โ€ข 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.13 Rโ˜‰ (circles scaled linearly by radius)

Sun

1.0 Rโ˜‰ baseline

HD 47186

1.13 Rโ˜‰

System Layout

Known planets

2 planets linked to this host

HD 47186 b

Radial Velocity

โ—Œ

Discovery

2008

Period

4.08 days

Radius

โ€”

Mass

22.25 MโŠ•

Eq. Temp

โ€”

HD 47186 c

Radial Velocity

โ—Œ

Discovery

2008

Period

1353.6 days

Radius

โ€”

Mass

111.4 MโŠ•

Eq. Temp

โ€”

HD 47186 and Its Two Known Planets

HD 47186 is a G5 V star 122 light-years away, with two planets reported to orbit it. The Sun-like star has a mass of 1 solar masses and a radius of 1.13 solar radii, larger than the Sun's. Its temperature is 5640 K, cooler than the Sun's, and its age is 6.5 billion years.

Both planets were found in 2008 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. HD 47186 b has a minimum mass of 22.2 Earth masses and an orbital period of 4.08 days. HD 47186 c has a minimum mass of 111 Earth masses and an orbital period of 1350 days. A minimum mass is a lower bound on a planet's true mass. Each planet's minimum mass is larger than Earth's. Among the listed planets, HD 47186 b has the shortest year by reported estimates, and HD 47186 c has the longest year by reported estimates. HD 47186 b also has the smallest minimum mass among the listed planets, while HD 47186 c has the largest.

Provenance

Underlying measurements and references

Evidence Summary

Rows

10

Stellar refs

10

System refs

1

Distancestable

10 values โ€ข 1 distinct

Parallaxstable

10 values โ€ข 1 distinct

Temperaturedisputed

5 values โ€ข 5 distinct

Massdisputed

4 values โ€ข 3 distinct

Radiusdisputed

4 values โ€ข 4 distinct

Agestable

1 values โ€ข 1 distinct

Luminositydisputed

4 values โ€ข 4 distinct

Surface Gravitydisputed

4 values โ€ข 3 distinct

Metallicitydisputed

4 values โ€ข 4 distinct

Spectral Typedisputed

3 values โ€ข 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
56750.99โ€”โ€”0.03โ€”37.46Sousa et al. 2008TICv8
564011.136.500.07โ€”37.46Ghezzi et al. 2010TICv8
564111.10โ€”0.04โ€”37.46TICv8TICv8
5685โ€”1.08โ€”0.04โ€”37.46Gaia DR2TICv8
โ€”โ€”โ€”โ€”โ€”G5 V37.46Michigan Catalog, Vol. 3TICv8
โ€”โ€”โ€”โ€”โ€”G537.46Cannon & Pickering 1918TICv8
โ€”โ€”โ€”โ€”โ€”G6 V37.46Gray et al. 2006TICv8
โ€”โ€”โ€”โ€”โ€”โ€”37.46Nordstrom et al. 2004TICv8
โ€”โ€”โ€”โ€”โ€”โ€”37.46Bouchy et al. 2009TICv8
56570.961.08โ€”โ€”โ€”37.46Stassun et al. 2017TICv8