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Stellar HostProfile

HD 217107

G8IV/V • 20.06 pc

Records

25

literature rows

Planets

2

system count

References

25

distinct source labels

HD: HD 217107HIP: HIP 113421TIC: TIC 38271828

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: Turnbull 2015 • System source: TICv8

Temperature

5704 K

5575 to 5704

10 values • 9 distinct

Mass

1.11 Msun

0.98 to 1.14

13 values • 11 distinct

Radius

1.08 Rsun

1.08 to 1.22

8 values • 7 distinct

Age

5.84 Gyr

4 to 15

5 values • 4 distinct

Luminosity

0.09 log(Lsun)

0.04 to 0.10

4 values • 4 distinct

Distance

20.06 pc

single adopted value

25 values • 1 distinct

Spectral Type

G8IV/V

Multiple classifications reported

G8 IV (3), G (1), G5 (1), G8 IV-V (1), G8 IV/V (1), G8IV/V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.08 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 217107

1.08 R☉

System Layout

Known planets

2 planets linked to this host

HD 217107 b

Radial Velocity

◌

Discovery

1998

Period

7.13 days

Radius

—

Mass

459.6 M⊕

Eq. Temp

—

HD 217107 c

Radial Velocity

◌

Discovery

2005

Period

5138.7 days

Radius

—

Mass

1388.9 M⊕

Eq. Temp

—

HD 217107 and Its Two Known Planets

HD 217107 is a star located 65.4 light-years from us. It is a single star with a spectral type of G8IV/V, and its reported properties include an age of 5.84 billion years, a mass of 1.11 solar masses, a radius of 1.08 solar radii, and a temperature of 5700 K. The host star is cooler than the Sun, while its reported mass and radius estimates are both larger than the Sun's. Two planets have been found orbiting HD 217107.

HD 217107 b was discovered in 1998 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. It has a mass of 460 Earth masses and an orbital period of 7.13 days. Among the listed planets, HD 217107 b has the shortest year and the smallest reported mass. Its mass is roughly 1.45 times Jupiter's mass.

HD 217107 c was discovered in 2005, also through radial velocity measurements. It has a mass of 1390 Earth masses and an orbital period of 5140 days. Among the listed planets, HD 217107 c has the longest year and the largest reported mass, and its mass is roughly 4.37 times Jupiter's mass. Both planets' reported mass estimates are larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

25

Stellar refs

24

System refs

1

Distancestable

25 values • 1 distinct

Parallaxstable

25 values • 1 distinct

Temperaturedisputed

10 values • 9 distinct

Massdisputed

13 values • 11 distinct

Radiusdisputed

8 values • 7 distinct

Agedisputed

5 values • 4 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

9 values • 8 distinct

Metallicitydisputed

10 values • 7 distinct

Spectral Typedisputed

8 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—————G8 IV-V20.06Gray et al. 2003TICv8
56651.101.0940.04—20.06Ghezzi et al. 2010TICv8
—1.05———G8 IV20.06Vogt et al. 2005TICv8
—1.14————20.06An et al. 2025TICv8
5679—————20.06Suárez-Andrés et al. 2016TICv8
———15——20.06Sanz-Forcada et al. 2010TICv8
——————20.06Valenti & Fischer 2005TICv8
—1.041.2211.90—G20.06Giovinazzi et al. 2025TICv8
5630—1.18—0.10—20.06Gaia DR2TICv8
56461.02————20.06Santos et al. 2004TICv8
—————G520.06Cannon & Pickering 1918TICv8
—1.111.085.84——20.06Takeda et al. 2007TICv8
——————20.06Nordstrom et al. 2004TICv8
57041.111.085.840.09G8IV/V20.06Turnbull 2015TICv8
—————G8 IV/V20.06Michigan Catalog, Vol. 5TICv8
——————20.06Nidever et al. 2002TICv8
56461.02———G8 IV20.06Wittenmyer et al. 2007TICv8
—1.13————20.06An et al. 2025TICv8
5680—————20.06Maldonado et al. 2015TICv8
—1.11————20.06Bryan et al. 2016TICv8
5606.81.061.17———20.06Rosenthal et al. 2021TICv8
——————20.06Wright et al. 2004TICv8
562211.11———20.06Stassun et al. 2017TICv8
—————G8 IV20.06Baines et al. 2009TICv8
55750.981.20—0.10—20.06TICv8TICv8