Temperature
5833 K
5449 to 6105
Unclassified star • 1144.9 pc
Records
32
literature rows
Planets
3
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
5833 K
5449 to 6105
Mass
1.02 Msun
0.84 to 1.10
Radius
1.03 Rsun
0.87 to 1.05
Age
3.80 Gyr
0.40 to 7.41
Distance
1144.9 pc
single adopted value
Planets
3
Stable across source rows
Scale Comparison
Current adopted radius: 1.03 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-276
1.03 R☉
System Layout
3 planets linked to this host
Transit
Discovery
2014
Period
14.13 days
Radius
2.87 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2013
Period
31.88 days
Radius
2.90 R⊕
Mass
16.60 M⊕
Eq. Temp
—
Transit
Discovery
2013
Period
48.65 days
Radius
2.80 R⊕
Mass
16.30 M⊕
Eq. Temp
—
Kepler-276 is a star located 3730 light-years away, and it hosts three known planets. The star itself is 3.8 billion years old and has a mass of 1.02 solar masses and a radius of 1.03 solar radii, with a temperature of 5830 K.
All three planets are Neptune-like in size classification and were found by the transit method. Kepler-276 b was discovered in 2014 and has a radius of 2.87 Earth radii and an orbital period of 14.1 days. Kepler-276 c was discovered in 2013 and has a mass of 16.6 Earth masses, a radius of 2.9 Earth radii, and an orbital period of 31.9 days. Kepler-276 d was also discovered in 2013 and has a mass of 16.3 Earth masses, a radius of 2.8 Earth radii, and an orbital period of 48.6 days.
Among the listed planets, Kepler-276 b has the shortest year, at 14.1 days, followed by Kepler-276 c with the second-shortest year, at 31.9 days. Kepler-276 d has the longest year, at 48.6 days. In radius, Kepler-276 c is the largest, at 2.9 Earth radii, while Kepler-276 d is the smallest, at 2.8 Earth radii, and Kepler-276 b is second-smallest, at 2.87 Earth radii. The masses of Kepler-276 c and Kepler-276 d are both larger than Earth's, and the radii of all three planets are larger than Earth's. Kepler-276 c has a mean density of 3.75 g/cm³, 0.681 times Earth's, while Kepler-276 d has a mean density of 4.09 g/cm³, 0.743 times Earth's.
Provenance
Evidence Summary
Rows
32
Stellar refs
18
System refs
1