Temperature
3369 K
3143 to 3482.1
Unclassified star • 127.2 pc
Records
21
literature rows
Planets
3
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
3369 K
3143 to 3482.1
Mass
0.43 Msun
0.15 to 0.43
Radius
0.42 Rsun
0.18 to 0.42
Age
6.61 Gyr
single adopted value
Distance
127.2 pc
single adopted value
Planets
3
Stable across source rows
Scale Comparison
Current adopted radius: 0.42 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-445
0.42 R☉
System Layout
3 planets linked to this host
Transit
Discovery
2015
Period
2.98 days
Radius
1.58 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2015
Period
4.87 days
Radius
2.51 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2015
Period
8.15 days
Radius
1.25 R⊕
Mass
—
Eq. Temp
—
Kepler-445 is an M4 star located 415 light-years away. Its spectral type indicates a small, cool red dwarf. The star has a mass of 0.43 solar masses and a radius of 0.42 solar radii, both smaller than the Sun's corresponding values. It is also cooler than the Sun, with a temperature of 3370 K, and has an age of 6.61 billion years. Three planets are known to orbit this host.
All three planets were discovered by transit in 2015, and each has a radius larger than Earth's. Kepler-445 b is a Super-Earth with a radius of 1.58 Earth radii and an orbital period of 2.98 days, the shortest year among the listed planets. Kepler-445 c is Neptune-like, with a radius of 2.51 Earth radii and a period of 4.87 days, the second-shortest year among the listed planets. It also has the largest radius among the listed planets. Kepler-445 d is Earth-like, with a radius of 1.25 Earth radii and a period of 8.15 days, the longest year among the listed planets by reported estimates. Its radius is the smallest among the listed planets.
Provenance
Evidence Summary
Rows
21
Stellar refs
13
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 127.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 3143 | 0.28 | 0.30 | — | -2.10 | — | 127.2 | TICv8 | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q12 KOI Table | TICv8 |
| 3157 | 0.15 | 0.18 | — | — | — | 127.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 3157 | 0.18 | 0.21 | — | — | M4 | 127.2 | Muirhead et al. 2015 | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q12 KOI Table | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q16 KOI Table | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 3157 | 0.16 | 0.19 | — | -2.47 | — | 127.2 | Mann et al. 2013 | TICv8 |
| 3369 | 0.43 | 0.42 | 6.61 | — | — | 127.2 | Morton et al. 2016 | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 3157 | — | 0.30 | — | — | — | 127.2 | Berger et al. 2018 | TICv8 |
| 3157 | 0.15 | 0.18 | — | — | — | 127.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 3240 | 0.21 | 0.27 | — | — | — | 127.2 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 127.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 3219 | 0.33 | 0.35 | — | -1.94 | — | 127.2 | Mann et al. 2017 | TICv8 |
| 3240 | 0.21 | 0.27 | — | — | — | 127.2 | Q1-Q8 KOI Table | TICv8 |
| 3327 | 0.17 | 0.19 | — | — | — | 127.2 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 127.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 3482.1 | — | — | — | — | — | 127.2 | Gaia DR2 | TICv8 |