Discovery
Transit
Host star Kepler-553 • 11.33 R⊕ • 328.2 d orbit
Records
11
archive rows
Discovery
—
Transit
Radius
11.33 R⊕
median non-null value
Mass
2129.5 M⊕
median non-null value
Kepler-553
242 K equilibrium
Quick Summary
This first pass still reads from the currently available detail payload. Canonical adopted summaries will replace first-row values in the next backend pass.
Host Star
Kepler-553
Discovery
Transit
Year
2016
Period
328.2 day
Radius
11.58 Rearth
Mass
2129.5 Mearth
Eq. Temp
251 K
Scale Comparison
Current adopted radius: 11.33 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
Kepler-553 c
11.33 R⊕
Jupiter
11.2 R⊕ reference
Provenance
Evidence Summary
Rows
11
Refs
11
Methods
1
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 11.58 Rearth | 2129.5 Mearth | 251 K | Dalba et al. 2024 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | — | — | — | Q1-Q17 DR25 Supplemental KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 11.20 Rearth | — | — | Morton et al. 2016 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 11.83 Rearth | — | 242 K | Q1-Q12 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 11.83 Rearth | — | 242 K | Q1-Q16 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | — | — | — | Gajdoš et al. 2019 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 11.83 Rearth | — | 242 K | Q1-Q17 DR24 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 11.33 Rearth | — | — | Fulton & Petigura 2018 |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 10.99 Rearth | — | 224 K | Q1-Q17 DR25 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | 328.2 day | 10.70 Rearth | — | 228 K | Q1-Q8 KOI Table |
| 2016 | Transit | Kepler | 0.95 m Kepler Telescope | — | 11.22 Rearth | — | — | Berger et al. 2018 |