Evolution of TOI-1130’s orbital parameters reported in Table 3 for 30 yr. Top panels: evolution of the planetary semi-major axes, orbital eccentricities, and inclinations of TOI-1130b (left) and TOI-1130c (right). Lower panels: evolution of the resonant angles Θ₁ and Θ₂, and the period ratio of TOI-1130 b and TOI-1130 c. The color shade represents the probability of the quantity having a certain value at a given time, with a darker shade indicating a higher probability. These probabilities were calculated based on the 600 dynamical simulations discussed in the text.