  We discuss some implications of recent progress in understanding the black
hole information paradox for complementarity in de Sitter space. Extending
recent work by two of the authors, we describe a bulk procedure that allows
information expelled through the cosmological horizon to be received by an
antipodal observer. Generically, this information transfer takes a scrambling
time $t = H^{-1}\log(S_{\rm dS})$. We emphasize that this procedure relies
crucially on selection of the Bunch-Davies vacuum state, interpreted as the
thermofield double state that maximally entangles two antipodal static patches.
The procedure also requires the presence of an (entangled) energy reservoir,
created by the collection of Hawking modes from the cosmological horizon. We
show how this procedure avoids a cloning paradox and comment on its
implications.
