Stable initial conditions for the system Kepler-1708 for the cases with and without the star. The results are presented as a function of the mass of the co-orbital companion (M2).
| M2 . | θ without the star . | θ with the star . |
|---|---|---|
| M⊕ . | (deg) . | (deg) . |
| 0.107 | 51−79 | 50−79 |
| 0.5 | 51−80 | 51−80 |
| 1.0 | 58−68 | 59−68 |
| 1.5 | − | − |
| 2.0 | − | − |
| 2.5 | 59−60 | 59−60 |
| 3.0 | − | − |
| 3.5 | − | − |
| 4.0 | 55−64 | 56−64 |
| 4.5 | 55−63 | 55−63 |
| 5.0 | 53, 56−64 | 53, 56−64 |
| M2 . | θ without the star . | θ with the star . |
|---|---|---|
| M⊕ . | (deg) . | (deg) . |
| 0.107 | 51−79 | 50−79 |
| 0.5 | 51−80 | 51−80 |
| 1.0 | 58−68 | 59−68 |
| 1.5 | − | − |
| 2.0 | − | − |
| 2.5 | 59−60 | 59−60 |
| 3.0 | − | − |
| 3.5 | − | − |
| 4.0 | 55−64 | 56−64 |
| 4.5 | 55−63 | 55−63 |
| 5.0 | 53, 56−64 | 53, 56−64 |
Stable initial conditions for the system Kepler-1708 for the cases with and without the star. The results are presented as a function of the mass of the co-orbital companion (M2).
| M2 . | θ without the star . | θ with the star . |
|---|---|---|
| M⊕ . | (deg) . | (deg) . |
| 0.107 | 51−79 | 50−79 |
| 0.5 | 51−80 | 51−80 |
| 1.0 | 58−68 | 59−68 |
| 1.5 | − | − |
| 2.0 | − | − |
| 2.5 | 59−60 | 59−60 |
| 3.0 | − | − |
| 3.5 | − | − |
| 4.0 | 55−64 | 56−64 |
| 4.5 | 55−63 | 55−63 |
| 5.0 | 53, 56−64 | 53, 56−64 |
| M2 . | θ without the star . | θ with the star . |
|---|---|---|
| M⊕ . | (deg) . | (deg) . |
| 0.107 | 51−79 | 50−79 |
| 0.5 | 51−80 | 51−80 |
| 1.0 | 58−68 | 59−68 |
| 1.5 | − | − |
| 2.0 | − | − |
| 2.5 | 59−60 | 59−60 |
| 3.0 | − | − |
| 3.5 | − | − |
| 4.0 | 55−64 | 56−64 |
| 4.5 | 55−63 | 55−63 |
| 5.0 | 53, 56−64 | 53, 56−64 |
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.
