  We discuss the definition of conserved quantities in asymptotically locally
de Sitter spacetimes. One may define an analogue of holographic charges at
future and past infinity and at other Cauchy surfaces $I_t$ as integrals over
the intersection of timelike surfaces $C$ and the Cauchy surface $I_t$. In
general, the charges $Q^t$ defined on the Cauchy surface $I_t$ depend on $C$,
but if gravitational flux is absent the charges are independent of $C$. On the
other hand, if there is a net gravitational flux entering or leaving the
spacetime region bounded by $C_1, C_2$ and two Cauchy surfaces then $\Delta
Q^t(C_1, C_2) = Q^t(C_1)-Q^t(C_2)$ changes by the same amount.
