Temperature
5767 K
5767 to 5808
G2V โข 23.30 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Temperature
5767 K
5767 to 5808
Mass
0.98 Msun
0.98 to 1.04
Radius
1.17 Rsun
1.17 to 1.21
Age
9.68 Gyr
single adopted value
Luminosity
0.15 log(Lsun)
0.15 to 0.15
Distance
23.30 pc
single adopted value
Spectral Type
G2V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.17 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
HD 168009
1.17 Rโ
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2021
Period
15.15 days
Radius
โ
Mass
9.53 Mโ
Eq. Temp
โ
HD 168009 is a G2V star, a Sun-like main-sequence dwarf, located 76 light-years away. The star's reported mass estimate is smaller than the Sun's, at 0.98 solar masses, while its reported radius estimate is larger than the Sun's, at 1.17 solar radii. Its temperature is 5770 K, and its age is 9.68 billion years. One planet is known to orbit this host.
That planet, HD 168009 b, was discovered in 2021 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 168009 b has a minimum mass of 9.53 Earth masses, a lower bound on its true mass, and that minimum mass is larger than Earth's. The planet completes one orbit every 15.1 days.
The star's reported radius estimate is larger than the Sun's, and its reported mass estimate is smaller than the Sun's.
Provenance
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5767 | 0.98 | 1.17 | 9.68 | 0.15 | G2V | 23.30 | Turnbull 2015 | TICv8 |
| โ | โ | โ | โ | โ | โ | 23.30 | Valenti & Fischer 2005 | TICv8 |
| โ | 0.98 | 1.17 | 9.68 | โ | โ | 23.30 | Takeda et al. 2007 | TICv8 |
| โ | โ | โ | โ | โ | โ | 23.30 | Nordstrom et al. 2004 | TICv8 |
| โ | โ | โ | โ | โ | โ | 23.30 | Wright et al. 2004 | TICv8 |
| โ | โ | โ | โ | โ | โ | 23.30 | Duncan et al. 1991 | TICv8 |
| 5778.3 | 0.99 | 1.21 | โ | โ | โ | 23.30 | Rosenthal et al. 2021 | TICv8 |
| 5808 | 1.04 | 1.17 | โ | 0.15 | โ | 23.30 | TICv8 | TICv8 |
| โ | โ | โ | โ | โ | G0 | 23.30 | Cannon & Pickering 1918 | TICv8 |
| โ | โ | โ | โ | โ | โ | 23.30 | Nidever et al. 2002 | TICv8 |
| โ | โ | โ | โ | โ | G1 V | 23.30 | Gray et al. 2003 | TICv8 |