Temperature
5615 K
5615 to 5732
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Stellar HostProfile
HD 117207
Unclassified star • 32.35 pc
Records
21
literature rows
Planets
1
system count
References
22
distinct source labels
HIP: HIP 65808TIC: TIC 405501056HD: HD 117207
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
Mass
1 Msun
0.96 to 1.08
Radius
1.11 Rsun
1.07 to 1.14
Age
6.50 Gyr
4.19 to 6.92
Luminosity
0.04 log(Lsun)
0.04 to 0.07
Distance
32.35 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.11 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 117207
1.11 R☉
System Layout
Known planets
1 planets linked to this host
HD 117207 b
Radial Velocity
◌
Discovery
2004
Period
2621.8 days
Radius
—
Mass
612.1 M⊕
Eq. Temp
—
HD 117207 and Its Planet
HD 117207 is a star 106 light-years from Earth with one known planet. Its spectral type, G7 IV-V, indicates a star of the same broad temperature class as the Sun, and its reported temperature of 5620 K is cooler than the Sun's. The star's reported radius of 1.11 solar radii is larger than the Sun's, while its mass is 1 solar mass and its age is 6.5 billion years.
The planet HD 117207 b was discovered in 2004 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 117207 b has a minimum mass of 612 Earth masses, a lower bound on its true mass, and is roughly 1.93 times Jupiter's mass. Its minimum mass is larger than Earth's. The planet completes an orbit every 2620 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
21
Stellar refs
21
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5724 | 1.08 | — | — | — | — | 32.35 | Butler et al. 2006 | TICv8 |
| — | — | — | — | — | — | 32.35 | Wright et al. 2004 | TICv8 |
| 5667 | 0.98 | — | — | 0.06 | — | 32.35 | Sousa et al. 2008 | TICv8 |
| 5643.5 | — | 1.13 | — | 0.07 | — | 32.35 | Gaia DR2 | TICv8 |
| 5618 | 0.99 | 1.14 | — | 0.07 | — | 32.35 | TICv8 | TICv8 |
| — | — | — | — | — | — | 32.35 | Nidever et al. 2002 | TICv8 |
| — | — | — | — | — | G5 | 32.35 | Cannon & Pickering 1918 | TICv8 |
| — | — | — | — | — | G7 IV-V | 32.35 | Gray et al. 2006 | TICv8 |
| 5649 | — | — | — | — | — | 32.35 | Suárez-Andrés et al. 2016 | TICv8 |
| 5662 | 0.96 | 1.11 | — | — | — | 32.35 | Stassun et al. 2017 | TICv8 |
| — | — | — | — | — | — | 32.35 | Valenti & Fischer 2005 | TICv8 |
| 5732 | 1.05 | 1.07 | 4.19 | — | — | 32.35 | Barbato et al. 2018 | TICv8 |
| 5634.8 | 1.02 | 1.13 | — | — | — | 32.35 | Rosenthal et al. 2021 | TICv8 |
| — | — | — | — | — | G8 IV/V | 32.35 | Michigan Catalog, Vol. 3 | TICv8 |
| 5615 | 1 | 1.11 | 6.50 | 0.04 | — | 32.35 | Ghezzi et al. 2010 | TICv8 |
| 5732 | 1.05 | — | — | — | G7 IV-V | 32.35 | Xiao et al. 2023 | TICv8 |
| 5723 | 1.04 | — | 6.92 | — | G8 IV/V | 32.35 | Marcy et al. 2005 | TICv8 |
| — | — | — | — | — | — | 32.35 | Henry et al. 1996 | TICv8 |
| — | 1.03 | 1.07 | 6.68 | — | — | 32.35 | Takeda et al. 2007 | TICv8 |
| — | — | — | — | — | — | 32.35 | Nordstrom et al. 2004 | TICv8 |
| — | 1.03 | — | — | — | — | 32.35 | Bryan et al. 2016 | TICv8 |