We give an explicit expression for gravitational energy, written solely in
terms of physical spacetime geometry, which (in suitable limits) agrees wit
h the total Arnowitt-Deser-Misner and Trautman-Bondi-Sachs energies for asy
mptotically flat spacetimes and with the Abbott-Deser energy for asymptotic
ally anti-de Sitter spacetimes. Our expression is a boundary value of the s
tandard gravitational Hamiltonian. Moreover, although it stands alone as su
ch, we derive the expression by picking the zero-point of energy via a "lig
ht-cone reference.'' [S0556-2821(99)07420-2].