Temperature
5403 K
4939 to 5403
Unclassified star • 486.1 pc
Records
21
literature rows
Planets
2
system count
References
15
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
5403 K
4939 to 5403
Mass
0.89 Msun
0.76 to 0.89
Radius
0.86 Rsun
0.74 to 1.11
Age
4.57 Gyr
1.74 to 13.90
Distance
486.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.86 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-949
0.86 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2016
Period
8.69 days
Radius
2.91 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2023
Period
21.00 days
Radius
2.97 R⊕
Mass
—
Eq. Temp
582 K
Kepler-949 is a star located 1590 light-years away. Its reported mass of 0.89 solar masses and radius of 0.86 solar radii are both smaller than the Sun's, and its temperature of 5400 K is cooler than the Sun's reported temperature. The star is also estimated to be 4.57 billion years old. Two planets are known to orbit this host: Kepler-949 b and Kepler-949 c.
Both planets are Neptune-like and were found by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. Kepler-949 b was discovered in 2016, and Kepler-949 c in 2023.
Kepler-949 b has an orbital period of 8.69 days, the shortest year among the listed planets, and a radius of 2.91 Earth radii, the smallest radius among the listed planets. Its radius is larger than Earth's. Kepler-949 c has an orbital period of 21 days, the longest year among the listed planets, and a radius of 2.97 Earth radii, the largest among the listed planets; its radius is likewise larger than Earth's.
Provenance
Evidence Summary
Rows
21
Stellar refs
14
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5403 | 0.89 | 0.86 | 4.57 | — | — | 486.1 | Morton et al. 2016 | TICv8 |
| 5145 | 0.76 | 0.79 | 13.90 | — | — | 486.1 | Q1-Q8 KOI Table | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q12 KOI Table | TICv8 |
| 5130 | — | 0.75 | — | — | — | 486.1 | Berger et al. 2018 | TICv8 |
| 5130 | 0.82 | 0.74 | 1.74 | — | — | 486.1 | Fulton & Petigura 2018 | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q16 KOI Table | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q16 KOI Table | TICv8 |
| 5145 | 0.76 | 0.79 | 13.90 | — | — | 486.1 | Q1-Q8 KOI Table | TICv8 |
| 5088.2 | 0.85 | 0.77 | — | -0.44 | — | 486.1 | TICv8 | TICv8 |
| 5052 | — | 0.87 | — | — | — | 486.1 | Q1-Q6 KOI Table | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5052 | — | 1.11 | — | — | — | 486.1 | Latham et al. 2005 | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 486.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5211 | 0.82 | 0.90 | — | — | — | 486.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5052 | 0.82 | 0.87 | — | — | — | 486.1 | Batalha et al. 2013 | TICv8 |
| 5052 | — | 0.87 | — | — | — | 486.1 | Q1-Q6 KOI Table | TICv8 |
| — | — | — | — | — | — | 486.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4939 | — | 0.77 | — | -0.50 | — | 486.1 | Gaia DR2 | TICv8 |