century, but during the 1950s examples of shallow-water
evaporites began to emerge, interpreted as having been
deposited in restricted marginal-marine estuaries or
basins. Marginal-marine evaporite deposition was further
stimulated with the documentation in the 1960s of
supratidal (“sabkha”) evaporite deposition along the Arabian margin of the Persian Gulf. With no modern analogs
for the thick, extensive evaporite sequences of the Phanerozoic, the Holocene occurrences of marginal-marine
sabkha evaporates have been used to explain ancient evaporite deposits. The application of the “sabkha model” was
accelerated with the recovery of upper Miocene
(Messinian) anhydrite and halite from the floor of the
Mediterranean Sea on Legs 13 and 42A of the Deep Sea
Drilling Project (DSDP). The implication was that these
evaporates were deposited in shallow subaqueous to subaerial environments and that the Mediterranean must have
dried up and refilled several times with a huge waterfall at
the Strait of Gibraltar. This has been called the deep-basin,
desiccation hypothesis, and the event has been called the
“Messinian Salinity Crisis.” Supratidal evaporite deposition in general and the Messinian Salinity Crisis in particular have dominated the evaporite literature in the decades
since the 1960s.
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