  We revisit the limits on $R$-parity violation in the minimal supersymmetric
standard model. In particular, we focus on the high-scale supersymmetry
scenario in which all the sparticles are in excess of the inflationary scale of
approximately $10^{13}$ GeV, and thus no sparticles ever come into thermal
equilibrium. In this case the cosmological limits, stemming from the
preservation of the baryon asymmetry that have been previously applied for weak
scale supersymmetry, are now relaxed. We argue that even when sparticles are
never in equilibrium, $R$-parity violation is still constrained via higher
dimensional operators by neutrino and nucleon experiments and/or insisting on
the preservation of a non-zero $B-L$ asymmetry.
