phosphorus-based life
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The electron configuration of a phosphorus atom
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Extraterrestrial life based on the element phosphorus,
instead of carbon, has been suggested as
a remote possibility. However, although phosphorus can be conceived of as
a potential biochemical building block, with phosphine (PH3)
as a compatible solvent, a major stumbling
is the poor variety of phosphorus hydrides.
At best, it seems that phosphorus might be able to form chains with other
elements such as carbon, silicon,
or nitrogen. A phosphorus
bottleneck?
Phosphorus is critical to terrestrial life: phosphorus and phosphates
are key parts of the double-helix "backbone" of DNA
and the energy transport molecule ATP. However,
the abundance of phosphorus in animals is about 17,000 greater than that
in the Sun (and, therefore, the solar nebula),
and two orders of magnitude greater than other major biogenic elements,
such as carbon, nitrogen, and oxygen. Put another way, life-as-we-know-it
needs a lot of phosphorus compared to the solar abundance (and, by extension,
the cosmic abundance), and the lithosphere
of Earth has managed to concentrate the phosphorus to a much greater extent
than other biogenic elements. This suggests a possible bottleneck in biotic
chemistry.
Phosphorus is manufactured only in moderately massive stars (greater than
about 15 solar masses, by neon and carbon fusion), and its presence in interstellar
molecule species appears to be quite sensitive to dust
grain mantle chemistry and fragility. It is conceivable then that planetary
systems could exist that have low phosphorus contents and are then perhaps
less suitable for Earth-type biochemistry. It is also conceivable that that
processes that have resulted in the Earth concentrating phosphorus to a
high degree are not ubiquitous in terrestrial worlds. Furthermore, much
of the phosphorus in the terrestrial lithosphere is in the form of phosphates
(particularly the apatite minerals), which
are not particularly soluble and require further processing in order to
be available to organisms. Thus, the abundance of phosphorus in solution
(or easily soluble form) is significantly lower than is suggested by the
pure value in the lithosphere. In addition, if much of the initial prebiotic
chemistry of a planet takes place in interstellar space and the circumstellar
environment of a protostar, then the animal/solar concentration may be a
better indicator of the degree to which phosphorus must be harvested in
order for the eventual success of entire biospheres. Reference
Scharf, Caleb A. Extrasolar Planets and Astrobiology,
Sausalito, Calif.: University Science Books (2009), pp. 441-2.
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