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The second most important constituent of the biosphere is [T =>QS@g
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liquid water. This can only exist in a very narrow range of temperatures, 81y<Uz 6
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since water freezes at 0°C and boils at 100°C. This is iE"]S )
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only a tiny range compared with the low temperatures of some &Hp*A^M
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other planets and the hot interior of the earth, let the temperature __1__ hO$Gx*e$
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of the sun. by controlpanel
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As we know, life would only be possible on the face of a __2__ p1d%&e
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planet had temperatures somewhere within this range. __3__ Q<AOc\oO
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The earth’s supply of water probably remains quite fairly constant __4__ #N`G2}1J
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in quantity. A certain number of hydrogen atoms, which <bhGpLh-E
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are one of the main constituents of water, are lost by escaping bR"4:b>K
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from the atmosphere to out space, but they are probably just __5__ Q`8-|(ngw
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about to be replaced by new water rising away from the depths of the __6__ V1M|p!
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earth during volcanic action. The total quantity of water is not !Ltx2CB2]
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known, and it is about enough to cover the surface of the globe __7__ SPlt=*C#_
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to a depth of about two and three-quarter kms. Most of it—97% $S<B\\
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is in the form of the salt waters of the oceans. The rest is {jYVA~.|Z
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fresh, but three quarter of this is in the form of ice at the Poles __8__ jG&HPVr
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and on mountains, and cannot be used by living systems when __9__ WxYEu+_
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melted. Of the remaining fraction, which is somewhat fewer __10__ >%`SXB&9
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than 1%of the whole, there is 10-20 times as much stored as underground (|AZO!
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water as is actually on the surface. There is also a minor,