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The planet we live on: The beginnings of the Earth Sciences

The planet we live on: The beginnings of the Earth Sciences

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Figure 3.26: Global temperature change over <strong>the</strong> last 450 thousand years, obtained fromduterium isotope measurements. <str<strong>on</strong>g>The</str<strong>on</strong>g> ratios <str<strong>on</strong>g>we</str<strong>on</strong>g>re measured in <strong>the</strong> EPICA and Vostockice cores and have been c<strong>on</strong>verted to ice volume estimati<strong>on</strong>s in <strong>the</strong> lo<str<strong>on</strong>g>we</str<strong>on</strong>g>r graph.space if it <str<strong>on</strong>g>we</str<strong>on</strong>g>re not for <strong>the</strong> greenhouse gases. <str<strong>on</strong>g>The</str<strong>on</strong>g>se absorb some <strong>of</strong> <strong>the</strong> outgoing infra-redradiati<strong>on</strong> causing a warming <strong>of</strong> <strong>the</strong> atmosphere and <strong>of</strong> <strong>the</strong> <strong>Earth</strong>. If it <str<strong>on</strong>g>we</str<strong>on</strong>g>re not for <strong>the</strong>warming effect <strong>of</strong> <strong>the</strong> greenhouse gases, heat from solar radiati<strong>on</strong> would be lost and <strong>the</strong><strong>Earth</strong> would be frozen and could not support life. So <strong>the</strong> atmosphere has to c<strong>on</strong>tain somegreenhouse gases for <strong>the</strong> <strong>Earth</strong> to be warm enough for life to exist.Some <strong>of</strong> <strong>the</strong> carb<strong>on</strong> dioxide in <strong>the</strong> atmosphere dissolves in rain and is carried into <strong>the</strong>sea. <str<strong>on</strong>g>The</str<strong>on</strong>g>re it is used by organisms to make calcium carb<strong>on</strong>ate shells and reefs. <str<strong>on</strong>g>The</str<strong>on</strong>g> morecarb<strong>on</strong> dioxide <strong>the</strong>re is in <strong>the</strong> atmosphere, <strong>the</strong> more becomes dissolved in <strong>the</strong> sea andis <strong>the</strong>n available to organisms. So this results in a negative feedback effect; <strong>the</strong> morecarb<strong>on</strong> dioxide <strong>the</strong>re is in <strong>the</strong> atmosphere, <strong>the</strong> more is removed, reducing <strong>the</strong> amount in<strong>the</strong> atmosphere.<str<strong>on</strong>g>The</str<strong>on</strong>g>se are two <strong>of</strong> <strong>the</strong> important feedback effects that affect <strong>the</strong> <strong>Earth</strong>, but <strong>the</strong>re are manyo<strong>the</strong>rs, some <str<strong>on</strong>g>we</str<strong>on</strong>g>ll understood and some not <str<strong>on</strong>g>we</str<strong>on</strong>g>ll understood at all. <str<strong>on</strong>g>The</str<strong>on</strong>g> overall effect <strong>of</strong><strong>the</strong>se has been <strong>the</strong> change <strong>of</strong> <strong>Earth</strong>’s temperature over geological time, as shown in Figure3.25. This shows that <strong>the</strong> <strong>Earth</strong> has had glacial periods in <strong>the</strong> past, when it was partlycovered by ice sheets, and much warmer periods, when <strong>the</strong>re <str<strong>on</strong>g>we</str<strong>on</strong>g>re no ice sheets. As <str<strong>on</strong>g>we</str<strong>on</strong>g>currently have ice sheets in polar areas, this shows that <strong>the</strong> <strong>Earth</strong> is undergoing <strong>on</strong>e <strong>of</strong><strong>the</strong> colder periods <strong>of</strong> <strong>Earth</strong>’s geological history.We can obtain informati<strong>on</strong> <strong>on</strong> how <strong>Earth</strong>’s temperature has changed in much more recentgeological time by measuring isotope ratios in cores drilled into ice sheets, as shown inFigure 3.26.This shows that even over <strong>the</strong> last few hundred thousand years, <strong>Earth</strong>’s temperature has90

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