Temperature
3405 K
3316 to 3424
M3 V • 140.2 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: Bakos et al. 2020 • System source: TICv8
Temperature
3405 K
3316 to 3424
Mass
0.49 Msun
0.44 to 0.49
Radius
0.48 Rsun
0.45 to 0.52
Age
3.20 Gyr
single adopted value
Luminosity
-1.56 log(Lsun)
-1.62 to -1.53
Distance
140.2 pc
single adopted value
Spectral Type
M3 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.48 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HATS-71
0.48 R☉
System Layout
1 planets linked to this host
Transit
Discovery
2020
Period
3.80 days
Radius
11.48 R⊕
Mass
117.6 M⊕
Eq. Temp
586.8 K
HATS-71 is an M3 V star, a small, cool red dwarf, located 457 light-years away. One planet orbits this host. The star is estimated to be 3.2 billion years old, with a mass of 0.486 solar masses and a radius of 0.478 solar radii. Its temperature is 3410 K, cooler than the Sun's.
The planet HATS-71 b is Jupiter-like, a size class that exceeds 4 times Earth's radius. It was discovered in 2020 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. HATS-71 b has a radius of 11.5 Earth radii and a mass of 118 Earth masses, both larger than Earth's corresponding values. Its orbital period is 3.8 days. The mean density is 0.428 g/cm³, 0.0778 times Earth's.
Provenance
Evidence Summary
Rows
4
Stellar refs
4
System refs
1