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Stellar HostProfile

HD 17156

G0 V • 78.09 pc

Records

13

literature rows

Planets

1

system count

References

14

distinct source labels

HD: HD 17156HIP: HIP 13192TIC: TIC 302773669

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: Fischer et al. 2007 • System source: TICv8

Temperature

6079 K

5925 to 6100

11 values • 7 distinct

Mass

1.20 Msun

1.10 to 1.41

10 values • 9 distinct

Radius

1.47 Rsun

1.24 to 1.58

12 values • 10 distinct

Age

5.70 Gyr

2.80 to 5.70

7 values • 6 distinct

Luminosity

0.41 log(Lsun)

0.39 to 0.44

6 values • 6 distinct

Distance

78.09 pc

single adopted value

13 values • 1 distinct

Spectral Type

G0 V

Multiple classifications reported

G5 (2), G0 V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.47 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 17156

1.47 R☉

System Layout

Known planets

1 planets linked to this host

HD 17156 b

Radial Velocity

◌

Discovery

2007

Period

21.22 days

Radius

12.26 R⊕

Mass

1036.1 M⊕

Eq. Temp

888 K

HD 17156 and Its Jupiter-Like Planet

HD 17156 is a G0 V star 255 light-years away. That spectral type marks it as a main-sequence dwarf of the same temperature class as the Sun. It is 5.7 billion years old, with a mass of 1.2 solar masses larger than the Sun's and a radius of 1.47 solar radii also larger than the Sun's. Its temperature of 6080 K is hotter than the Sun's. One planet orbits this host.

HD 17156 b is a Jupiter-like planet found in 2007 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. It has a mass of 1040 Earth masses, roughly 3.26 times Jupiter's mass, and a radius of 12.3 Earth radii. Both its mass and radius estimates are larger than Earth's. Its orbital period is 21.2 days. Its mean density is 3.1 g/cm³, 0.562 times Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

13

Stellar refs

13

System refs

1

Distancestable

13 values • 1 distinct

Parallaxstable

13 values • 1 distinct

Temperaturedisputed

11 values • 7 distinct

Massdisputed

10 values • 9 distinct

Radiusdisputed

12 values • 10 distinct

Agedisputed

7 values • 6 distinct

Luminositydisputed

6 values • 6 distinct

Surface Gravitydisputed

8 values • 8 distinct

Metallicitydisputed

8 values • 6 distinct

Spectral Typedisputed

3 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
60401.411.55———78.09Stassun et al. 2017TICv8
61001.241.442.800.41—78.09Barbieri et al. 2009TICv8
5925—1.58—0.44—78.09Gaia DR2TICv8
60791.201.475.700.41G0 V78.09Fischer et al. 2007TICv8
59691.101.55—0.44—78.09TICv8TICv8
—————G578.09Cannon & Pickering 1918TICv8
60791.301.492.80——78.09Southworth 2011TICv8
60791.271.503.37——78.09Bonomo et al. 2017TICv8
60461.281.523.300.44—78.09Kane et al. 2023TICv8
—1.271.513.38——78.09Nutzman et al. 2011TICv8
60841.191.24———78.09Mortier et al. 2013TICv8
59691.231.473.460.39G578.09Ment et al. 2018TICv8
5925—1.55———78.09ExoFOPTICv8