Discovery Method
Transit
Consistent across records
Host star Kepler-584 • 4.21 R⊕ • 35.18 d orbit
Records
10
archive rows
Discovery
2016
Transit
Radius
4.21 R⊕
default parameter set
Mass
—
default parameter set
Kepler-584
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: Morton et al. 2016
Host Star
Kepler-584
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2016
Stable across source rows
Orbital Period
35.18 day
35.18 to 35.18
Radius
4.21 Rearth
4 to 5.37
Scale Comparison
Current adopted radius: 4.21 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
Kepler-584 b
4.21 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 |
|---|---|---|---|---|---|---|---|---|
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | — | — | — | Holczer et al. 2016 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | 4.02 Rearth | — | 656 K | Q1-Q16 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | 4.02 Rearth | — | 656 K | Q1-Q17 DR24 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | 4.17 Rearth | — | 664 K | Q1-Q17 DR25 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | 4.02 Rearth | — | 656 K | Q1-Q12 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | — | 5.37 Rearth | — | — | Berger et al. 2018 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | 4 Rearth | — | 647 K | Q1-Q8 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | — | — | — | Q1-Q17 DR25 Supplemental KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | 4.21 Rearth | — | — | Morton et al. 2016 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 35.18 day | — | — | — | Gajdoš et al. 2019 |