Temperature
5700 K
5610 to 5742
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Stellar HostProfile
HD 86728
G1V โข 14.92 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
HD: HD 86728HIP: HIP 49081TIC: TIC 172954294
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
0.96 Msun
0.96 to 1.03
Radius
1.06 Rsun
1.06 to 1.24
Age
9.52 Gyr
single adopted value
Luminosity
0.17 log(Lsun)
0.14 to 0.17
Distance
14.92 pc
single adopted value
Spectral Type
G1V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.06 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
HD 86728
1.06 Rโ
System Layout
Known planets
1 planets linked to this host
HD 86728 b
Radial Velocity
โ
Discovery
2025
Period
31.15 days
Radius
โ
Mass
9.43 Mโ
Eq. Temp
โ
HD 86728 b: A Nearby Sun-Like Star and Its Single Planet
HD 86728 is a G1V star located 48.7 light-years away, with a spectral type indicating a Sun-like, main-sequence dwarf. It has one known planet. The star's reported mass estimate is 0.96 solar masses, smaller than the Sun's, while its reported radius estimate is 1.06 solar radii, larger than the Sun's. Its reported temperature is 5700 K, cooler than the Sun, and its age is 9.52 billion years.
The one known planet is HD 86728 b, discovered in 2025 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. Its minimum mass is 9.43 Earth masses, larger than Earth's, and it completes one orbit in 31.2 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitystable
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | 0.96 | 1.06 | 9.52 | โ | โ | 14.92 | Takeda et al. 2007 | TICv8 |
| โ | โ | โ | โ | โ | โ | 14.92 | Valenti & Fischer 2005 | TICv8 |
| โ | โ | โ | โ | โ | โ | 14.92 | Nidever et al. 2002 | TICv8 |
| 5700 | 0.96 | 1.06 | 9.52 | 0.17 | G1V | 14.92 | Turnbull 2015 | TICv8 |
| โ | โ | โ | โ | โ | G5 | 14.92 | Cannon & Pickering 1918 | TICv8 |
| 5742 | 1.03 | 1.18 | โ | 0.14 | โ | 14.92 | TICv8 | TICv8 |
| 5610 | 0.97 | 1.24 | โ | 0.14 | โ | 14.92 | Gupta et al. 2025 | TICv8 |
| โ | โ | โ | โ | โ | โ | 14.92 | Nordstrom et al. 2004 | TICv8 |
| โ | โ | โ | โ | โ | โ | 14.92 | Wright et al. 2004 | TICv8 |
| โ | โ | โ | โ | โ | G4 V | 14.92 | Gray et al. 2003 | TICv8 |
| โ | โ | โ | โ | โ | โ | 14.92 | Duncan et al. 1991 | TICv8 |