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The second most important constituent of the biosphere is ~U8#Iq1
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liquid water. This can only exist in a very narrow range of temperatures, iy
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since water freezes at 0°C and boils at 100°C. This is *D<S \6=
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only a tiny range compared with the low temperatures of some zx(j6
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other planets and the hot interior of the earth, let the temperature __1__ ,-CDF)~G=3
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of the sun. by controlpanel LO.4sO
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As we know, life would only be possible on the face of a __2__ }(E6:h;}~
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planet had temperatures somewhere within this range. __3__ /N%f78
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The earth’s supply of water probably remains quite fairly constant __4__ 9 b]U&A$
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in quantity. A certain number of hydrogen atoms, which U_}$QW0'
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are one of the main constituents of water, are lost by escaping sQJM 4'8f
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from the atmosphere to out space, but they are probably just __5__ TP{a*ke^5,
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about to be replaced by new water rising away from the depths of the __6__ I J4"X#Q/
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earth during volcanic action. The total quantity of water is not Ysr{1! K
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known, and it is about enough to cover the surface of the globe __7__ +ypG<VBx%
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to a depth of about two and three-quarter kms. Most of it—97% ~|uCZ.;o
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is in the form of the salt waters of the oceans. The rest is p,tB
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fresh, but three quarter of this is in the form of ice at the Poles __8__ +W;B8^imG
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and on mountains, and cannot be used by living systems when __9__ )D[ypuM&
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melted. Of the remaining fraction, which is somewhat fewer __10__ ;~1r{kXxA"
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than 1%of the whole, there is 10-20 times as much stored as underground 5z]dA~;*2
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water as is actually on the surface. There is also a minor,