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<article language="en">
	<journal>
		<journal_title>Earth System Dynamics Discussions</journal_title>
		<journal_url>www.earth-syst-dynam-discuss.net</journal_url>
		<eissn>2190-4995</eissn>
		<volume_number>1</volume_number>
		<issue_number>1</issue_number>
		<publication_year>2010</publication_year>
	</journal>
	<doi>10.5194/esdd-1-191-2010</doi>
	<article_url>http://www.earth-syst-dynam-discuss.net/1/191/2010/</article_url>
	<abstract_html>http://www.earth-syst-dynam-discuss.net/1/191/2010/esdd-1-191-2010.html</abstract_html>
	<fulltext_pdf>http://www.earth-syst-dynam-discuss.net/1/191/2010/esdd-1-191-2010.pdf</fulltext_pdf>
	<start_page>191</start_page>
	<end_page>246</end_page>
	<publication_date>2010-09-17</publication_date>
	<article_title content_type="html">Assessing life&apos;s effects on the interior dynamics of planet Earth using non-equilibrium thermodynamics</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>J. G. Dyke</name>
			<email>jdyke@bgc-jena.mpg.de</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>F. Gans</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>A. Kleidon</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max Planck Institut fÃ¼r Biogeochemie, Jena, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">Vernadsky described life as &lt;i&gt;the&lt;/i&gt; geologic force, while Lovelock noted
the role of life in driving the Earth&apos;s atmospheric composition to a unique
state of thermodynamic disequilibrium. Here, we use these notions in
conjunction with thermodynamics to quantify biotic activity as a driving
force for geologic processes. Specifically, we explore the hypothesis that
biologically-mediated processes operating on the surface of the Earth, such
as the biotic enhancement of weathering of continental crust, affect interior
processes such as mantle convection and have therefore shaped the evolution
of the whole Earth system beyond its surface and atmosphere. We set up three
simple models of mantle convection, oceanic crust recycling and continental
crust recycling. We describe these models in terms of non-equilibrium
thermodynamics in which the generation and dissipation of gradients is
central to driving their dynamics and that such dynamics can be affected by
their boundary conditions. We use these models to quantify the maximum power
that is involved in these processes. The assumption that these processes,
given a set of boundary conditions, operate at maximum levels of generation
and dissipation of free energy lead to reasonable predictions of core
temperature, seafloor spreading rates, and continental crust thickness. With
a set of sensitivity simulations we then show how these models interact
through the boundary conditions at the mantle-crust and oceanic-continental
crust interfaces. These simulations hence support our hypothesis that the
depletion of continental crust at the land surface can affect rates of
oceanic crust recycling and mantle convection deep within the Earth&apos;s
interior. We situate this hypothesis within a broader assessment of
surface-interior interactions by setting up a work budget of the Earth&apos;s
interior to compare the maximum power estimates that drive interior processes
to the power that is associated with biotic activity. We estimate that the
maximum power involved in mantle convection is 12 TW, oceanic crust cycling
is 28 TW, and continental uplift is less than 1 TW. By directly utilizing the
low entropy nature of solar radiation, photosynthesis generates 215 TW of
chemical free energy. This high power associated with life results from the
fact that photochemistry is not limited by the low energy that is available
from the heating gradients that drive geophysical processes in the interior.
We conclude that by utilizing only a small fraction of the generated free
chemical energy for geochemical transformations at the surface, life has the
potential to substantially affect interior processes, and so the whole Earth
system. Consequently, when understanding Earth system processes we may need
to adopt a dynamical model schema in which previously fixed boundary
conditions become components of a co-evolutionary system.</abstract>
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</article>

