Canonical parameters adopted in this work for the systems Kepler-1625 and Kepler-1708. We consider the planets and satellites in circular and coplanar orbits, except when stated differently.
| System . | M⋆ . | R⋆ . | Mp . | Rp . | ap . | Ms . | Rs . | as . |
|---|---|---|---|---|---|---|---|---|
| . | M⊙ . | R⊙ . | MJ . | RJ . | ua . | M⊕ . | R⊕ . | Rp . |
| Kepler-1625 | 1.079 | 1.793 | 3.0 | 1.18 | 0.87 | 17.15 | 3.865 | 40.0 |
| Kepler-1708 | 1.1 | 1.1 | 0.81 | 0.89 | 1.64 | 5.0 | 2.61 | 11.7 |
| System . | M⋆ . | R⋆ . | Mp . | Rp . | ap . | Ms . | Rs . | as . |
|---|---|---|---|---|---|---|---|---|
| . | M⊙ . | R⊙ . | MJ . | RJ . | ua . | M⊕ . | R⊕ . | Rp . |
| Kepler-1625 | 1.079 | 1.793 | 3.0 | 1.18 | 0.87 | 17.15 | 3.865 | 40.0 |
| Kepler-1708 | 1.1 | 1.1 | 0.81 | 0.89 | 1.64 | 5.0 | 2.61 | 11.7 |
Canonical parameters adopted in this work for the systems Kepler-1625 and Kepler-1708. We consider the planets and satellites in circular and coplanar orbits, except when stated differently.
| System . | M⋆ . | R⋆ . | Mp . | Rp . | ap . | Ms . | Rs . | as . |
|---|---|---|---|---|---|---|---|---|
| . | M⊙ . | R⊙ . | MJ . | RJ . | ua . | M⊕ . | R⊕ . | Rp . |
| Kepler-1625 | 1.079 | 1.793 | 3.0 | 1.18 | 0.87 | 17.15 | 3.865 | 40.0 |
| Kepler-1708 | 1.1 | 1.1 | 0.81 | 0.89 | 1.64 | 5.0 | 2.61 | 11.7 |
| System . | M⋆ . | R⋆ . | Mp . | Rp . | ap . | Ms . | Rs . | as . |
|---|---|---|---|---|---|---|---|---|
| . | M⊙ . | R⊙ . | MJ . | RJ . | ua . | M⊕ . | R⊕ . | Rp . |
| Kepler-1625 | 1.079 | 1.793 | 3.0 | 1.18 | 0.87 | 17.15 | 3.865 | 40.0 |
| Kepler-1708 | 1.1 | 1.1 | 0.81 | 0.89 | 1.64 | 5.0 | 2.61 | 11.7 |
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