  The peeling behaviour of the Weyl tensor near null infinity is determined for
an asymptotically flat higher dimensional spacetime. The result is
qualitatively different from the peeling property in 4d. To leading order, the
Weyl tensor is type N. The first subleading term is type II. The next term is
algebraically general in 6 or more dimensions but in 5 dimensions another type
N term appears before the algebraically general term. The Bondi energy flux is
written in terms of "Newman-Penrose" Weyl components.
