Temperature
5635 K
5529.2 to 5635
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Stellar HostProfile
HD 175167
Unclassified star โข 71.09 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
HD: HD 175167HIP: HIP 93281TIC: TIC 467966544
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: TICv8 โข System source: TICv8
Mass
1 Msun
1 to 1.37
Radius
1.76 Rsun
1.75 to 1.84
Luminosity
0.45 log(Lsun)
0.45 to 0.46
Distance
71.09 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.76 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
HD 175167
1.76 Rโ
System Layout
Known planets
1 planets linked to this host
HD 175167 b
Radial Velocity
โ
Discovery
2009
Period
1175 days
Radius
โ
Mass
4703.9 Mโ
Eq. Temp
โ
HD 175167 and Its Planet
HD 175167 is a G-type star 232 light-years away. Its spectral type of G5 IV/V indicates a temperature class similar to the Sun's, and its radius of 1.76 solar radii is larger than the Sun's. The star's temperature of 5640 K is cooler than the Sun's, and its mass is 1 solar masses. One planet orbits this host.
That planet, HD 175167 b, was discovered in 2009 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 175167 b has a mass of 4700 Earth masses, larger than Earth's and roughly 14.8 times Jupiter's mass. Its orbital period is 1180 days, the time it takes to complete one orbit.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | 1 | โ | โ | โ | โ | 71.09 | Feng et al. 2022 | TICv8 |
| 5635 | 1 | 1.76 | โ | 0.45 | โ | 71.09 | TICv8 | TICv8 |
| 5635 | 1.17 | โ | โ | โ | G5 IV/V | 71.09 | Xiao et al. 2023 | TICv8 |
| 5635 | 1.17 | โ | โ | โ | โ | 71.09 | Santos et al. 2013 | TICv8 |
| โ | โ | โ | โ | โ | G5 | 71.09 | Cannon & Pickering 1918 | TICv8 |
| 5529.2 | โ | 1.84 | โ | 0.46 | โ | 71.09 | Gaia DR2 | TICv8 |
| โ | 1.10 | โ | โ | โ | G5 IV/V | 71.09 | Arriagada et al. 2010 | TICv8 |
| โ | 1.09 | โ | โ | โ | โ | 71.09 | Winn 2022 | TICv8 |
| 5635 | 1.37 | 1.75 | โ | โ | โ | 71.09 | Stassun et al. 2017 | TICv8 |
| โ | โ | โ | โ | โ | G5 IV/V | 71.09 | Michigan Catalog, Vol. 1 | TICv8 |