Temperature
6138 K
5925.5 to 6461
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Stellar HostProfile
Kepler-1395
Unclassified star • 492.9 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
TIC: TIC 63204326
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
1.17 Msun
1.13 to 1.40
Radius
1.23 Rsun
1.19 to 1.99
Age
2.88 Gyr
2.60 to 2.88
Distance
492.9 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.23 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
Kepler-1395
1.23 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1395 b
Transit
◌
Discovery
2016
Period
3.78 days
Radius
0.80 R⊕
Mass
—
Eq. Temp
—
Kepler-1395 b: A Sub-Earth in a Distant System
Kepler-1395 is a star located 1610 light-years away, and one planet has been found orbiting it. The host star is estimated to be 2.88 billion years old, with a mass of 1.17 solar masses and a radius of 1.23 solar radii. Its temperature is 6140 K, and its reported mass, radius, and temperature are all larger or hotter than the Sun's.
The system's only known planet, Kepler-1395 b, was discovered in 2016 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-1395 b is classified as a Sub-Earth, meaning its radius is smaller than Earth's. Its radius is 0.8 Earth radii, and its reported radius estimate is smaller than Earth's. The planet completes an orbit in 3.78 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6017 | 1.13 | 1.21 | — | — | — | 492.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6200 | — | 1.85 | — | — | — | 492.9 | Latham et al. 2005 | TICv8 |
| 6461 | 1.30 | 1.95 | — | — | — | 492.9 | Q1-Q16 KOI Table | TICv8 |
| 6138 | 1.17 | 1.23 | 2.88 | — | — | 492.9 | Morton et al. 2016 | TICv8 |
| 6069 | 1.15 | 1.19 | 2.69 | — | — | 492.9 | Fulton & Petigura 2018 | TICv8 |
| 6071.9 | 1.13 | 1.24 | — | 0.28 | — | 492.9 | TICv8 | TICv8 |
| 6461 | 1.30 | 1.95 | — | — | — | 492.9 | Q1-Q12 KOI Table | TICv8 |
| 6461 | 1.30 | 1.95 | — | — | — | 492.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 492.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6069 | — | 1.21 | — | — | — | 492.9 | Berger et al. 2018 | TICv8 |
| 6458 | 1.40 | 1.99 | 2.60 | — | — | 492.9 | Q1-Q8 KOI Table | TICv8 |
| 5925.5 | — | 1.27 | — | 0.25 | — | 492.9 | Gaia DR2 | TICv8 |