Elucidating
the details of the formation, stability, interactions,
and reactivity of biomolecular systems under extreme environmental
conditions, including high salt concentrations in brines and high
osmotic and high hydrostatic pressures, is of fundamental biological,
astrobiological, and biotechnological importance. Bacteria and archaea
are able to survive in the deep ocean or subsurface of Earth, where
pressures of up to 1 kbar are reached. The deep subsurface of Mars
may host high concentrations of ions in brines, such as perchlorates,
but we know little about how these conditions and the resulting osmotic
stress conditions would affect the habitability of such environments
for cellular life. We discuss the combined effects of osmotic (salts,
organic cosolvents) and hydrostatic pressures on the structure, stability,
and reactivity of biomolecular systems, including membranes, proteins,
and nucleic acids. To this end, a variety of biophysical techniques
have been applied, including calorimetry, UV/vis, FTIR and fluorescence
spectroscopy, and neutron and X-ray scattering, in conjunction with
high pressure techniques. Knowledge of these effects is essential
to our understanding of life exposed to such harsh conditions, and
of the physical limits of life in general. Finally, we discuss strategies
that not only help us understand the adaptive mechanisms of organisms
that thrive in such harsh geological settings but could also have
important ramifications in biotechnological and pharmaceutical applications.