Temperature
5745 K
5745 to 5790
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Stellar HostProfile
HD 164595
G2V โข 28.25 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
HIP: HIP 88194HD: HD 164595TIC: TIC 158917706
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 โข System source: TICv8
Mass
0.97 Msun
0.97 to 1.03
Radius
1.04 Rsun
1.02 to 1.04
Age
7.12 Gyr
single adopted value
Luminosity
0.04 log(Lsun)
0.02 to 0.04
Distance
28.25 pc
single adopted value
Spectral Type
G2V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.04 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
HD 164595
1.04 Rโ
System Layout
Known planets
1 planets linked to this host
HD 164595 b
Radial Velocity
โ
Discovery
2015
Period
40 days
Radius
โ
Mass
16.14 Mโ
Eq. Temp
โ
HD 164595 and Its Planet
HD 164595 is a G2V star located 92.2 light-years away, with one known planet in orbit. The star has an age of 7.12 billion years, a mass of 0.97 solar masses, a radius of 1.04 solar radii, and a temperature of 5750 K. Its reported mass estimate is smaller than the Sun's, while its reported radius estimate is larger than the Sun's; its reported temperature is cooler than the Sun's.
The sole listed planet is HD 164595 b, discovered in 2015 by the radial velocity method. This technique measures the wobble a planet's gravity induces in its star's motion, and repeated wobbles reveal the planet and its orbital period. HD 164595 b has a minimum mass of 16.1 Earth masses, a lower bound on its true mass, which is larger than Earth's. It completes one orbit in 40 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
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 | โ | โ | โ | โ | โ | 28.25 | Nordstrom et al. 2004 | TICv8 |
| โ | โ | โ | โ | โ | โ | 28.25 | Nidever et al. 2002 | TICv8 |
| โ | โ | โ | โ | โ | G5 | 28.25 | Cannon & Pickering 1918 | TICv8 |
| โ | 0.97 | 1.04 | 7.12 | โ | โ | 28.25 | Takeda et al. 2007 | TICv8 |
| 5751 | 1.03 | 1.03 | โ | 0.02 | โ | 28.25 | TICv8 | TICv8 |
| โ | โ | โ | โ | โ | โ | 28.25 | Wright et al. 2004 | TICv8 |
| 5790 | 0.99 | โ | โ | โ | G2 V | 28.25 | Courcol et al. 2015 | TICv8 |
| 5762 | โ | 1.02 | โ | 0.02 | โ | 28.25 | Gaia DR2 | TICv8 |
| 5745 | 0.97 | 1.04 | 7.12 | 0.04 | G2V | 28.25 | Turnbull 2015 | TICv8 |
| โ | โ | โ | โ | โ | โ | 28.25 | Valenti & Fischer 2005 | TICv8 |