Temperature
5654 K
5552 to 5654
Unclassified star • 241.9 pc
Records
19
literature rows
Planets
2
system count
References
13
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
5654 K
5552 to 5654
Mass
1.02 Msun
0.91 to 1.02
Radius
1.51 Rsun
1.42 to 1.51
Age
9.77 Gyr
9.77 to 12.10
Distance
241.9 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 1.51 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-449
1.51 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2015
Period
12.58 days
Radius
2.06 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2015
Period
33.67 days
Radius
2.76 R⊕
Mass
—
Eq. Temp
—
Kepler-449 is a star 789 light-years away. Its reported mass is 1.02 solar masses, its radius is 1.51 solar radii, its temperature is 5650 K, and its age is 9.77 billion years. The star’s reported radius estimate is larger than the Sun’s, and its reported temperature is cooler than the Sun’s. Two planets are known around this host.
Kepler-449 b and Kepler-449 c were both discovered in 2015 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-449 b is classified as a Super-Earth and has an orbital period of 12.6 days and a radius of 2.06 Earth radii. Kepler-449 c is classified as Neptune-like and has an orbital period of 33.7 days and a radius of 2.76 Earth radii. Both planets’ reported radius estimates are larger than Earth’s. Among the listed planets, Kepler-449 b has the shortest year and the smallest radius by reported estimates, while Kepler-449 c has the longest year and the largest radius by reported estimates.
Provenance
Evidence Summary
Rows
19
Stellar refs
12
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5552 | 0.95 | 1.46 | 12.10 | — | — | 241.9 | Q1-Q8 KOI Table | TICv8 |
| 5588 | 0.97 | 1.47 | — | — | — | 241.9 | Q1-Q16 KOI Table | TICv8 |
| 5552 | — | 1.46 | — | — | — | 241.9 | Q1-Q6 KOI Table | TICv8 |
| 5590.5 | — | — | — | — | — | 241.9 | Gaia DR2 | TICv8 |
| 5588 | 0.97 | 1.47 | — | — | — | 241.9 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 241.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5552 | — | 1.46 | — | — | — | 241.9 | Q1-Q6 KOI Table | TICv8 |
| 5588 | 0.97 | 1.47 | — | — | — | 241.9 | Q1-Q12 KOI Table | TICv8 |
| 5649.2 | — | — | — | — | — | 241.9 | TICv8 | TICv8 |
| 5654 | 1.02 | 1.51 | 9.77 | — | — | 241.9 | Morton et al. 2016 | TICv8 |
| 5552 | — | 1.46 | — | — | — | 241.9 | Batalha et al. 2013 | TICv8 |
| — | 0.97 | 1.47 | — | — | — | 241.9 | Huber et al. 2013 | TICv8 |
| 5552 | 0.95 | 1.46 | 12.10 | — | — | 241.9 | Q1-Q8 KOI Table | TICv8 |
| 5587 | 0.91 | 1.42 | — | — | — | 241.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 241.9 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5588 | 0.97 | 1.47 | — | — | — | 241.9 | Q1-Q12 KOI Table | TICv8 |
| 5587 | 0.91 | 1.42 | — | — | — | 241.9 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5588 | 0.97 | 1.47 | — | — | — | 241.9 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5588 | 0.97 | 1.47 | — | — | — | 241.9 | Q1-Q17 DR24 KOI Table | TICv8 |