Temperature
4726 K
4513 to 4956.0
Unclassified star
Records
20
literature rows
Planets
2
system count
References
14
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
4726 K
4513 to 4956.0
Mass
0.75 Msun
0.67 to 0.75
Radius
0.71 Rsun
0.64 to 0.79
Age
3.63 Gyr
3.63 to 13.90
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.71 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-383
0.71 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
12.90 days
Radius
1.32 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
31.20 days
Radius
1.24 R⊕
Mass
—
Eq. Temp
—
Kepler-383 is a star with two known planets, both classified as Earth-like and both discovered in 2014 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. The star's reported mass estimate is 0.75 solar masses and its radius is 0.71 solar radii, both smaller than the Sun's. Its reported temperature is 4730 K, cooler than the Sun's, and its age is 3.63 billion years.
The two planets are Kepler-383 b and Kepler-383 c. Kepler-383 b has an orbital period of 12.9 days and a radius of 1.32 Earth radii, while Kepler-383 c has an orbital period of 31.2 days and a radius of 1.24 Earth radii. Radius here compares a planet's size with Earth's radius, not its volume. Among the listed planets, Kepler-383 b has the shortest year by reported estimates and the largest radius, while Kepler-383 c has the longest year and the smallest radius.
Provenance
Evidence Summary
Rows
20
Stellar refs
13
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4710 | 0.68 | 0.70 | — | — | — | — | Q1-Q17 DR24 KOI Table | TICv8 |
| 4534 | 0.67 | 0.64 | — | — | — | — | Batalha et al. 2013 | TICv8 |
| 4956.0 | — | — | — | — | — | — | Gaia DR2 | TICv8 |
| 4534 | — | 0.64 | — | — | — | — | Q1-Q6 KOI Table | TICv8 |
| 4710 | 0.68 | 0.70 | — | — | — | — | Q1-Q16 KOI Table | TICv8 |
| 4701 | 0.67 | 0.65 | 13.90 | — | — | — | Q1-Q8 KOI Table | TICv8 |
| 4701 | 0.67 | 0.65 | 13.90 | — | — | — | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | — | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4726 | 0.75 | 0.71 | 3.63 | — | — | — | Morton et al. 2016 | TICv8 |
| 4608.8 | — | — | — | — | — | — | TICv8 | TICv8 |
| 4710 | 0.68 | 0.70 | — | — | — | — | Q1-Q16 KOI Table | TICv8 |
| 4710 | 0.68 | 0.70 | — | — | — | — | Q1-Q17 DR24 KOI Table | TICv8 |
| 4534 | — | 0.64 | — | — | — | — | Q1-Q6 KOI Table | TICv8 |
| 4513 | 0.71 | 0.72 | — | — | — | — | Q1-Q17 DR25 KOI Table | TICv8 |
| 4534 | — | 0.79 | — | — | — | — | Latham et al. 2005 | TICv8 |
| 4710 | — | 0.67 | — | — | — | — | Rowe et al. 2014 | TICv8 |
| 4513 | 0.71 | 0.72 | — | — | — | — | Q1-Q17 DR25 KOI Table | TICv8 |
| 4710 | 0.68 | 0.70 | — | — | — | — | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | — | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4710 | 0.68 | 0.70 | — | — | — | — | Q1-Q12 KOI Table | TICv8 |