Temperature
5326 K
5312.3 to 5654
Unclassified star • 812.5 pc
Records
18
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: Fulton & Petigura 2018 • System source: TICv8
Temperature
5326 K
5312.3 to 5654
Mass
0.86 Msun
0.86 to 0.96
Radius
0.77 Rsun
0.71 to 0.88
Age
1.35 Gyr
0.40 to 1.35
Distance
812.5 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.77 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-404
0.77 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2014
Period
11.83 days
Radius
1.27 R⊕
Mass
—
Eq. Temp
—
Transit
Discovery
2014
Period
14.75 days
Radius
1.72 R⊕
Mass
—
Eq. Temp
—
Kepler-404 is a star located 2650 light-years away, and two planets have been found in orbit around it. The host star is estimated to be 1.35 billion years old, with a mass of 0.86 solar masses and a radius of 0.771 solar radii. Its reported temperature is 5330 K. The star's reported mass estimate is smaller than the Sun's, its reported radius estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's.
Both planets were discovered by transit, the method in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness; repeated dips help establish orbital periods. Kepler-404 b is classified as Earth-like and has a radius of 1.27 Earth radii. It completes an orbit in 11.8 days, and among the listed planets it has the shortest year by reported estimates. Kepler-404 c is classified as a Super-Earth and has a radius of 1.72 Earth radii. Its orbital period is 14.8 days, and among the listed planets it has the longest year by reported estimates. Among the listed planets, Kepler-404 b has the smallest radius by reported estimates, while Kepler-404 c has the largest radius by reported estimates. Both were discovered in 2014.
Provenance
Evidence Summary
Rows
18
Stellar refs
12
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 812.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5653 | 0.95 | 0.86 | — | — | — | 812.5 | Q1-Q12 KOI Table | TICv8 |
| 5406 | — | 0.71 | — | — | — | 812.5 | Latham et al. 2005 | TICv8 |
| 5653 | 0.95 | 0.86 | — | — | — | 812.5 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5312.3 | — | 0.79 | — | -0.34 | — | 812.5 | Gaia DR2 | TICv8 |
| 5653 | 0.95 | 0.86 | — | — | — | 812.5 | Q1-Q16 KOI Table | TICv8 |
| 5653 | 0.95 | 0.86 | — | — | — | 812.5 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 812.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5326 | 0.86 | 0.77 | 1.35 | — | — | 812.5 | Fulton & Petigura 2018 | TICv8 |
| 5653 | 0.95 | 0.86 | — | — | — | 812.5 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 812.5 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5653 | 0.95 | 0.86 | — | — | — | 812.5 | Q1-Q16 KOI Table | TICv8 |
| 5654 | — | 0.88 | — | — | — | 812.5 | Rowe et al. 2014 | TICv8 |
| 5639 | 0.96 | 0.86 | — | — | — | 812.5 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5326 | — | 0.79 | — | — | — | 812.5 | Berger et al. 2018 | TICv8 |
| 5342 | 0.92 | 0.79 | — | -0.34 | — | 812.5 | TICv8 | TICv8 |
| 5612 | 0.93 | 0.82 | 0.40 | — | — | 812.5 | Q1-Q8 KOI Table | TICv8 |
| 5612 | 0.93 | 0.82 | 0.40 | — | — | 812.5 | Q1-Q8 KOI Table | TICv8 |