Discovery Method
Transit
Consistent across records
Host star Kepler-444 • 0.50 R⊕ • 4.55 d orbit
Records
10
archive rows
Discovery
2015
Transit
Radius
0.50 R⊕
default parameter set
Mass
—
default parameter set
Kepler-444
temperature unconstrained
Canonical Summary
Values come from the archive's default parameter set. Missing values stay missing. Ranges and counts describe all source rows.
Selected source: Campante et al. 2015
Host Star
Kepler-444
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2015
Stable across source rows
Orbital Period
4.55 day
4.55 to 4.55
Semi-Major Axis
0.05 au
0.05 to 0.05
Radius
0.50 Rearth
0.39 to 75.16
Scale Comparison
Current adopted radius: 0.50 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
Kepler-444 c
0.50 R⊕
Jupiter
11.2 R⊕ reference
Provenance
Evidence Summary
Rows
10
Refs
10
Methods
1
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 0.39 Rearth | — | 799 K | Q1-Q17 DR24 KOI Table |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | — | — | — | Q1-Q17 DR25 Supplemental KOI Table |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | — | — | — | Holczer et al. 2016 |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 0.50 Rearth | — | — | Campante et al. 2015 |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 0.44 Rearth | — | — | Weiss et al. 2024 |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 0.39 Rearth | — | 799 K | Q1-Q12 KOI Table |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 0.65 Rearth | — | 868 K | Q1-Q17 DR25 KOI Table |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 0.39 Rearth | — | 799 K | Q1-Q16 KOI Table |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | 4.55 day | 75.16 Rearth | — | — | Morton et al. 2016 |
| 2015 | Transit | Kepler | 0.95 m Kepler Telescope | — | 0.75 Rearth | — | — | Berger et al. 2018 |