  In light of very recent E989 experimental result, we investigate the
possibility that heavy sparticles explain the muon g-2 anomaly. We focus on the
bino-smuon loop in an effective SUSY scenario, where a light gravitino plays
the role of dark matter and other sparticles are heavy. Due to the enhancement
of left-right mixing of smuons by heavy higgsinos, the contribution of
bino-smuon loop can sizably increase the prediction of muon g-2 to the
experimental value. Under collider and vacuum stability constraints, we find
that TeV scale bino and smuon can still account for the new muon g-2 anomaly.
The implications for LHC phenomenology are also discussed.
