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Stellar HostProfile

HD 4203

Unclassified star • 81.38 pc

Records

16

literature rows

Planets

2

system count

References

17

distinct source labels

TIC: TIC 434225151HIP: HIP 3502HD: HD 4203

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 • System source: TICv8

Temperature

5644 K

5502 to 5728

9 values • 9 distinct

Mass

1.15 Msun

0.93 to 1.25

10 values • 7 distinct

Radius

1.33 Rsun

1.20 to 1.55

6 values • 6 distinct

Age

5 Gyr

5 to 8.52

2 values • 2 distinct

Luminosity

0.21 log(Lsun)

0.21 to 0.30

3 values • 3 distinct

Distance

81.38 pc

single adopted value

16 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.33 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 4203

1.33 R☉

System Layout

Known planets

2 planets linked to this host

HD 4203 b

Radial Velocity

◌

Discovery

2001

Period

431.9 days

Radius

—

Mass

708.8 M⊕

Eq. Temp

—

HD 4203 c

Radial Velocity

◌

Discovery

2014

Period

6700 days

Radius

—

Mass

689.7 M⊕

Eq. Temp

—

HD 4203 and Its Two Known Planets

HD 4203 is a G5 star situated 265 light-years away. The star is estimated to be 5 billion years old and contains 1.15 solar masses of material, with a radius of 1.33 solar radii and a temperature of 5640 K. Its mass and radius are both larger than the Sun's, while its temperature is cooler. Two planets are known to orbit this host, both discovered by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion.

HD 4203 b was discovered in 2001. It has a minimum mass of 709 Earth masses - roughly 2.23 times Jupiter's mass - and an orbital period of 432 days, the shortest year among the listed planets.

HD 4203 c was discovered in 2014. Its minimum mass is 690 Earth masses, or roughly 2.17 times Jupiter's mass, and it takes 6700 days to complete one orbit, the longest year among the listed planets. It also has the smallest minimum mass of the pair, while HD 4203 b has the largest. Both minimum masses are lower bounds on the planets' true masses, and both are larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

16

Stellar refs

16

System refs

1

Distancestable

16 values • 1 distinct

Parallaxstable

16 values • 1 distinct

Temperaturedisputed

9 values • 9 distinct

Massdisputed

10 values • 7 distinct

Radiusdisputed

6 values • 6 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

9 values • 7 distinct

Metallicitydisputed

9 values • 7 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
55961.251.42———81.38Stassun et al. 2017TICv8
—1.131.208.52——81.38Takeda et al. 2007TICv8
56361.06————81.38Santos et al. 2004TICv8
—1.06————81.38Vogt et al. 2002TICv8
56500.93————81.38Santos et al. 2003TICv8
56441.151.3350.21—81.38Ghezzi et al. 2010TICv8
55820.991.50—0.29—81.38TICv8TICv8
—1.13————81.38Bryan et al. 2016TICv8
5502—1.55—0.30—81.38Gaia DR2TICv8
—————G581.38Cannon & Pickering 1918TICv8
——————81.38Wright et al. 2004TICv8
——————81.38Valenti & Fischer 2005TICv8
5625.11.141.50———81.38Rosenthal et al. 2021TICv8
——————81.38Nidever et al. 2002TICv8
5728—————81.38Suárez-Andrés et al. 2016TICv8
57021.13————81.38Butler et al. 2006TICv8