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Stellar HostProfile

HD 202206

G6 V • 45.97 pc

Records

15

literature rows

Planets

1

system count

References

16

distinct source labels

HIP: HIP 104903TIC: TIC 24294415HD: HD 202206

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: Benedict & Harrison 2017 • System source: TICv8

Temperature

5766 K

5722 to 5776

9 values • 9 distinct

Mass

1.07 Msun

1.03 to 1.27

9 values • 8 distinct

Radius

1.04 Rsun

0.99 to 1.05

6 values • 5 distinct

Age

2.90 Gyr

1 to 5.60

4 values • 4 distinct

Distance

45.97 pc

single adopted value

15 values • 1 distinct

Spectral Type

G6 V

Multiple classifications reported

G6 V (3), G5 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.04 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 202206

1.04 R☉

System Layout

Known planets

1 planets linked to this host

HD 202206 c

Radial Velocity

◌

Discovery

2004

Period

1260 days

Radius

—

Mass

5689.2 M⊕

Eq. Temp

—

HD 202206 and Its Two Planets

HD 202206 is a Sun-like star 150 light-years away, with a spectral type of G2 V. It is 3.94 billion years old, holds 1.06 solar masses, spans 1.04 solar radii, and has a temperature of 5760 K. Its reported radius estimate is larger than the Sun's. Two planets orbit this host.

HD 202206 b was found by the radial velocity method in 2026. It has a reported mass of 6850 Earth masses, roughly 21.6 times Jupiter's mass and larger than Earth's, and an orbital period of 256 days, the shortest year among the listed planets.

HD 202206 c was also found by radial velocity, in 2004. Its reported mass is 982 Earth masses, roughly 3.09 times Jupiter's mass and larger than Earth's. Its orbital period is 1300 days, the longest year among the listed planets, and its reported mass is the smallest among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

15

Stellar refs

15

System refs

1

Distancestable

15 values • 1 distinct

Parallaxstable

15 values • 1 distinct

Temperaturedisputed

9 values • 9 distinct

Massdisputed

9 values • 8 distinct

Radiusdisputed

6 values • 5 distinct

Agedisputed

4 values • 4 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

9 values • 8 distinct

Metallicitydisputed

8 values • 6 distinct

Spectral Typedisputed

4 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
57661.071.042.90—G6 V45.97Benedict & Harrison 2017TICv8
—————G545.97Cannon & Pickering 1918TICv8
5739.11.031.05—0.03—45.97TICv8TICv8
—1.071.032.04——45.97Takeda et al. 2007TICv8
—————G6 V45.97Michigan Catalog, Vol. 4TICv8
57221.100.991-0.03—45.97Ghezzi et al. 2010TICv8
57651.15—5.60—G6 V45.97Udry et al. 2002TICv8
—1.15————45.97Gozdziewski et al. 2006TICv8
57601.271.03———45.97Stassun et al. 2017TICv8
57571.04——0.02—45.97Sousa et al. 2008TICv8
5734.5—1.05—0.03—45.97Gaia DR2TICv8
5776—————45.97Maldonado et al. 2015TICv8
57521.06————45.97Santos et al. 2004TICv8
——————45.97Correia et al. 2005TICv8
——————45.97Valenti & Fischer 2005TICv8