Time evolution of the gas disc and planetary envelopes after the tidal disruption of a Jupiter-like planet. (a) Azimuthally averaged surface density at four times; dashed lines mark the closer and farther VEPs. (b) Disc surface density evolution for the 10 M_⊕ case; circles indicate the closer VEP. (c): Accretion rates (top) and envelope masses (bottom) for VEPs at both orbits. M_atm, ⊕ indicates the atmospheric mass of Earth.