A theory of gravity localizes quantum ? ?information differently from nongravitational quantum field ? ?theories. This effect, called the holography of information, arises ? ?as a consequence of the gravitational constraints. A precise version ? ?of this property can be established using an asymptotic analysis ? ?while making only weak assumptions about the ultraviolet completion ? ?of the low-energy theory. For simple lowenergy states, this property ? ?can also be studied in perturbation theory. I will describe how ? ?holography of information is manifested in asymptotically anti-de ? ?Sitter space, asymptotically flat space, and asymptotically de ? ?Sitter space. I will also discuss implications for evaporating ? ?black-holes and show how accounting for this feature of gravity ? ?leads to a resolution of several puzzles. ?