Ce. Sherman et al., Marine and meteoric diagenesis of Pleistocene carbonates from a nearshore submarine terrace, Oahu, Hawaii, J SED RES, 69(5), 1999, pp. 1083-1097
The nearshore slope of Oahu consists of a shallowly dipping shelf extending
from the shoreline out to the similar to -20 m contour, where there is a s
harp break in slope down to similar to -30 m, Limestones recovered in a ser
ies of short cores taken from this nearshore terrace are typical of shallow
-marine reef environments and comprise either a branching-coral or massive-
coral facies, The composition as well as shoreward zonation of facies sugge
sts that the terrace represents an in situ fossil reef complex. Th-U ages o
f in situ corals are all Pleistocene and suggest that the bulk of the featu
re formed during marine oxygen isotope stage 7. Later accretion along the s
eaward front of the terrace occurred during marine oxygen isotope substages
5a and/or 5c. Deposition during these interglacial highstands has not prev
iously been documented in the sea-level record on Oahu,
Although the diagenetic record in the cored samples is incomplete, three pe
riods of diagenesis are identified: early shallow marine, meteoric, and pos
t-meteoric shallow marine. Early shallow-marine diagenesis includes cementa
tion by aragonite and Mg calcite in an active marine phreatic zone and pred
ominantly micritization in a stagnant marine phreatic zone. Meteoric proces
ses occurred in the vadose zone and include precipitation of calcite (needl
e fibers, meniscus cements, micritic networks), neomorphism, and dissolutio
n. All limestones are now in an active marine phreatic zone. Evidence of po
st-meteoric shallow-marine diagenesis is found in last-generation Mg calcit
e cements and internal sediments occurring directly on limestone substrates
that have otherwise been stabilized to calcite. The present seafloor is un
dergoing extensive biological and physical erosion. No Holocene limestones
were recovered. Petrographic and geochemical signatures of subaerial exposu
re and meteoric diagenesis are recognized within the upper several centimet
ers of all cores. Thus, the present seafloor in the study area is a flooded
Pleistocene subaerial exposure surface.