Temperature
5846 K
5483.7 to 5846
G V • 400.3 pc
Records
4
literature rows
Planets
1
system count
References
5
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: Brahm et al. 2016 • System source: TICv8
Temperature
5846 K
5483.7 to 5846
Mass
1.13 Msun
1.05 to 1.13
Radius
1.09 Rsun
1.09 to 1.41
Age
2.10 Gyr
single adopted value
Luminosity
0.09 log(Lsun)
0.09 to 0.26
Distance
400.3 pc
single adopted value
Spectral Type
G V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 1.09 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HATS-17
1.09 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2016
Period
16.25 days
Radius
8.71 R⊕
Mass
425.3 M⊕
Eq. Temp
814 K
HATS-17 is a Sun-like star located 1310 light-years away. Its spectral type of G V identifies it as a G-type main-sequence dwarf. The star is estimated to be 2.1 billion years old, with a mass of 1.13 solar masses and a radius of 1.09 solar radii, both larger than the Sun's corresponding values. Its temperature is 5850 K. One planet orbits this star.
That planet is HATS-17 b, a Jupiter-like world discovered by the transit method in 2016. It has a mass of 425 Earth masses, roughly 1.34 times Jupiter's mass, and a radius of 8.71 Earth radii. Both its mass and radius are larger than Earth's. It completes an orbit every 16.3 days. Its mean density is 3.55 g/cm³, which is 0.644 times Earth's.
Provenance
Evidence Summary
Rows
4
Stellar refs
4
System refs
1