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The second most important constituent of the biosphere is 7fC:'1]G
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liquid water. This can only exist in a very narrow range of temperatures, Mt*V-`+\
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since water freezes at 0°C and boils at 100°C. This is ,FwJ0V
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only a tiny range compared with the low temperatures of some
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other planets and the hot interior of the earth, let the temperature __1__ :W9a t
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of the sun. by controlpanel 0$_WIk
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As we know, life would only be possible on the face of a __2__ E"7[|-`e6
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planet had temperatures somewhere within this range. __3__ F#~*j
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The earth’s supply of water probably remains quite fairly constant __4__ ;?y~ h$
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in quantity. A certain number of hydrogen atoms, which \z
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are one of the main constituents of water, are lost by escaping B
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from the atmosphere to out space, but they are probably just __5__ RIDl4c
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about to be replaced by new water rising away from the depths of the __6__ ltKMvGEF
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earth during volcanic action. The total quantity of water is not ZSr!L@S
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known, and it is about enough to cover the surface of the globe __7__ |D_4 iFC
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to a depth of about two and three-quarter kms. Most of it—97% 3#Iq5vT
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is in the form of the salt waters of the oceans. The rest is u\"/EaQ{
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fresh, but three quarter of this is in the form of ice at the Poles __8__ o' v!83$L
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and on mountains, and cannot be used by living systems when __9__ )[u'LgVN/L
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melted. Of the remaining fraction, which is somewhat fewer __10__ ;rNX
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than 1%of the whole, there is 10-20 times as much stored as underground }0f~hL24
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water as is actually on the surface. There is also a minor,