Temperature
6120 K
5806 to 6250
Unclassified star • 1549.1 pc
Records
22
literature rows
Planets
2
system count
References
16
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
6120 K
5806 to 6250
Mass
1.16 Msun
1.07 to 1.20
Radius
1.23 Rsun
0.99 to 1.46
Age
3.09 Gyr
0.50 to 5.25
Distance
1549.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.23 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-182
1.23 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
9.83 days
Radius
2.58 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
20.68 days
Radius
3.43 R⊕
Mass
—
Eq. Temp
—
Kepler-182 is a star located 5050 light-years away. It is 3.09 billion years old, with a mass of 1.16 solar masses, a radius of 1.23 solar radii, and a temperature of 6120 K. Its reported mass, radius, and temperature estimates are all larger or hotter than the Sun's. Two planets orbit this host.
Both planets were found 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. Kepler-182 b is Neptune-like, which places it in a size class reaching 4 times Earth's radius. It completes an orbit, or year, in 9.83 days and has a radius of 2.58 Earth radii, larger than Earth's. Among the listed planets, it has the shortest year and the smallest radius by reported estimates. Kepler-182 c is also Neptune-like, with an orbital period of 20.7 days and a radius of 3.43 Earth radii, also larger than Earth's. Among the listed planets, it has the longest year and the largest radius by reported estimates.
Provenance
Evidence Summary
Rows
22
Stellar refs
15
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5989 | — | 0.99 | — | — | — | 1549.1 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1549.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6250 | — | 1.15 | — | — | — | 1549.1 | Rowe et al. 2014 | TICv8 |
| 6246 | 1.18 | 1.09 | — | — | — | 1549.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6215 | 1.20 | 1.15 | — | — | — | 1549.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6188 | 1.10 | 1.01 | 0.50 | — | — | 1549.1 | Q1-Q8 KOI Table | TICv8 |
| 6215 | 1.20 | 1.15 | — | — | — | 1549.1 | Q1-Q16 KOI Table | TICv8 |
| 5989 | — | 1.05 | — | — | — | 1549.1 | Q1-Q6 KOI Table | TICv8 |
| 6215 | 1.20 | 1.15 | — | — | — | 1549.1 | Q1-Q16 KOI Table | TICv8 |
| 6188 | 1.10 | 1.01 | 0.50 | — | — | 1549.1 | Q1-Q8 KOI Table | TICv8 |
| 6120 | 1.16 | 1.23 | 3.09 | — | — | 1549.1 | Morton et al. 2016 | TICv8 |
| 5806 | — | 1.46 | — | 0.34 | — | 1549.1 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 1549.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6246 | 1.18 | 1.09 | — | — | — | 1549.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5883.2 | 1.07 | 1.43 | — | 0.34 | — | 1549.1 | TICv8 | TICv8 |
| 6215 | 1.20 | 1.15 | — | — | — | 1549.1 | Q1-Q12 KOI Table | TICv8 |
| 5989 | 1.14 | 1.05 | — | — | — | 1549.1 | Batalha et al. 2013 | TICv8 |
| 6215 | 1.20 | 1.15 | — | — | — | 1549.1 | Q1-Q12 KOI Table | TICv8 |
| 5960 | — | 1.38 | — | — | — | 1549.1 | Berger et al. 2018 | TICv8 |
| 5989 | — | 1.05 | — | — | — | 1549.1 | Q1-Q6 KOI Table | TICv8 |
| 6215 | 1.20 | 1.15 | — | — | — | 1549.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5960 | 1.11 | 1.33 | 5.25 | — | — | 1549.1 | Fulton & Petigura 2018 | TICv8 |