Temperature
5295 K
4963 to 5295
Unclassified star • 527.3 pc
Records
36
literature rows
Planets
4
system count
References
19
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: Morton et al. 2016 • System source: TICv8
Temperature
5295 K
4963 to 5295
Mass
0.87 Msun
0.77 to 0.87
Radius
0.83 Rsun
0.79 to 0.95
Age
4.68 Gyr
2.45 to 13.70
Distance
527.3 pc
single adopted value
Planets
4
Stable across source rows
Scale Comparison
Current adopted radius: 0.83 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-176
0.83 R☉
System Layout
4 planets linked to this host
Transit
Discovery
2014
Period
5.43 days
Radius
1.43 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
12.76 days
Radius
2.60 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
25.75 days
Radius
2.51 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2016
Period
51.17 days
Radius
1.45 R⊕
Mass
—
Eq. Temp
—
Kepler-176 is a star located 1720 light-years away. It is 4.68 billion years old, with a mass of 0.87 solar masses and a radius of 0.83 solar radii. Its temperature is 5300 K, which is cooler than the Sun's. The star's reported mass estimate and radius estimate are both smaller than the Sun's. Four planets are known to orbit this host.
All four planets were found 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. Kepler-176 b was discovered in 2014. It is an Earth-like planet with a radius of 1.43 Earth radii and an orbital period of 5.43 days, giving it the shortest year among the listed planets. Kepler-176 c was also discovered in 2014 and is Neptune-like, with a radius of 2.6 Earth radii and an orbital period of 12.8 days, the second-shortest year among the listed planets. Its radius is the largest among them and is larger than Earth's.
Kepler-176 d, another 2014 discovery, is Neptune-like with a radius of 2.51 Earth radii and an orbital period of 25.8 days, the second-longest year among the listed planets. Its radius is larger than Earth's and is the second-largest among the listed planets. Kepler-176 e was discovered in 2016. It is Earth-like, with a radius of 1.45 Earth radii and an orbital period of 51.2 days, the longest year among the listed planets. Its radius is the second-smallest among the listed planets and is larger than Earth's.
Provenance
Evidence Summary
Rows
36
Stellar refs
18
System refs
1