  We consider the issue of information recovery for an object carrying energy
and entropy into a black hole using the generalized entropy formalism, in the
context of JT gravity where the backreaction problem can be solved exactly. We
verify the main aspects of the Hayden-Preskill scenario but with some
refinements. We show that the information is encoded in the Hawking radiation
in a redundant way, as expected for a quantum error correcting code. We show
how quantum extremal surfaces associated to information recovery have the form
of a python's lunch and thereby show that the complexity of decoding is
exponential in a combination of the entropy shift of the black hole and the
entropy of the object. We also show that an infalling observer must have a
smooth experience at the horizon and we calculate their endurance proper time
inside the black hole before they are radiated out.
