Abstract. In the last few decades and in the near future
CO2-induced ocean acidification is potentially a big threat to marine
calcite-shelled animals (e.g. brachiopods, bivalves, corals and gastropods).
Despite the great number of studies focusing on the effects of acidification
on shell growth, metabolism, shell dissolution and shell repair, the
consequences for biomineral formation remain poorly understood. Only a few
studies have addressed the impact of ocean acidification on shell
microstructure and geochemistry. In this study, a detailed microstructure and
stable isotope geochemistry investigation was performed on nine adult
brachiopod specimens of Magellania venosa (Dixon, 1789). These were
grown in the natural environment as well as in controlled culturing
experiments under different pH conditions (ranging from 7.35 to 8.15±0.05)
over different time intervals (214 to 335 days). Details of shell
microstructural features, such as thickness of the primary layer, density and
size of endopunctae and morphology of the basic structural unit of the
secondary layer were analysed using scanning electron microscopy. Stable
isotope compositions (δ13C and δ18O) were
tested from the secondary shell layer along shell ontogenetic increments in
both dorsal and ventral valves. Based on our comprehensive dataset, we
observed that, under low-pH conditions, M. venosa produced a more
organic-rich shell with higher density of and larger endopunctae, and smaller
secondary layer fibres. Also, increasingly negative δ13C and
δ18O values are recorded by the shell produced during
culturing and are related to the CO2 source in the culture set-up.
Both the microstructural changes and the stable isotope results are similar
to observations on brachiopods from the fossil record and strongly support
the value of brachiopods as robust archives of proxies for studying ocean
acidification events in the geologic past.