Temperature
6001 K
5767 to 6482
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Stellar HostProfile
Kepler-392
Unclassified star • 681.4 pc
Records
25
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 158796434
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: Morton et al. 2016 • System source: TICv8
Mass
1.07 Msun
0.87 to 1.23
Radius
1.14 Rsun
1.06 to 1.46
Age
4.37 Gyr
2.97 to 10.72
Distance
681.4 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.14 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-392
1.14 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-392 b
Transit
◌
Discovery
2014
Period
5.34 days
Radius
1 R⊕
Mass
—
Eq. Temp
—
Kepler-392 c
Transit
◌
Discovery
2014
Period
10.42 days
Radius
1.10 R⊕
Mass
—
Eq. Temp
—
Kepler-392 and Its Two Earth-Like Planets
Kepler-392 is a star located 2220 light-years away. It is 4.37 billion years old, with a mass of 1.07 solar masses, a radius of 1.14 solar radii, and a temperature of 6000 K, making it larger, more massive, and hotter than the Sun. Two planets are known to orbit this host.
Both planets were discovered by the transit method in 2014 and are classified as Earth-like. Kepler-392 b has an orbital period of 5.34 days and a radius of 1 Earth radii, making it the shortest-period and smallest-radius planet among the two. Kepler-392 c orbits every 10.4 days with a radius of 1.1 Earth radii, giving it the longest period and largest radius of the pair.
Provenance
Underlying measurements and references
Evidence Summary
Rows
25
Stellar refs
15
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed