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We all know water. It has three different states: as a
liquid we may drink or swim in, as ice on which we may
skate in the winter, and as a vapour that takes the form of
clouds in the air. Our own bodies contain a lot of water - about two
thirds of our weight - and we could not live without it. The water molecule consists of an oxygen molecule (O) that is bound
to two hydrogen atoms (H) and the chemical formula is accordingly:
H2O. Many chemical substances - but far from all -
dissolve in water. What are then the outstanding properties of this polar solvent
which are so precious for life? The first one is the range of temperatures in which water is
maintained in a liquid state. Water evaporates at 100 °C and
freezes at 0 °C at normal pressure conditions. This range can be
further increased by addition of salts into the solution or at high
pressure as at the bottom of the ocean. There has been speculation about the possibility of other solvents
being used to sustain life, such as ammonia or methane, but in both
cases the range in which the solvent is liquid is smaller and the
temperatures are far below 0 °C, which would seriously affect the
kinetics of the biological reactions.
Another important property is the different density of the
liquid and solid state, which allows ice to float on liquid
water. Both properties, which are a consequence of the atomic
structure of the water molecule, are fundamental for the existence of
liquid water over an important range of temperatures. Polarity is also an important property of water, because it
allows it to interact with non-polar molecules, like fatty acids,
generating membranes, a basic cellular structure required for
compartmentalisation. The utilization of non-polar solvents, like
methane or ethane, would require the use of polar substances for the
formation of membranes, with physico-chemical properties quite
different from the unified version of our Earth reference systems. In relation to metabolism, water is interesting because it
dissociates and produces protons (i.e. hydrogen nuclei, H+),
which are very important for the control of acidity (pH) and for
energy storage. Moreover, its redox potential (a chemical
property) can be used to generate reducing power for the assimilation
of carbon dioxide (CO2) during the oxygenic
photosynthesis. But life also requires other
elements to subsist.
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Life in the Universe![]()
Origins and Limits of Life
Conditions Needed for Life
Water
Other Elements
Energy
The Environment
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Last updated September 3, 2001