Kepler-1704b
| Discovery | |
|---|---|
| Discovered by | Paul A. Dalba et al. |
| Discovery date | 2021 |
| Designations | |
| KOI-375.01 | |
| Orbital characteristics | |
| Periastron | 0.16 |
| Apoastron | 3.9 |
| 2.026+0.024 −0.031 AU | |
| Eccentricity | 0.921+0.010 −0.015 |
| 988.8811177±0.0009114 | |
| Inclination | 89.01+0.59 −0.27° |
| Physical characteristics | |
| 10.81 R🜨 | |
| Mass | 4.15 ± 0.29 MJ |
| Temperature | 253.8+3.7 −4.1 K |
Kepler-1704b is a super-Jupiter on a highly eccentric orbit around the star Kepler-1704. It has a mass of 4.51 MJ. The planet's distance from its star varies from 0.16 to 3.9 AU. It is a failed hot Jupiter, having been scattered from its birth orbit to orbit with a periastron just above the tidal circularization distance.