cape of about 0.0014 calorie[1] per square metre of the Earth's
surface per second (assuming the rise of temperature downwards,
_i.e._ the "gradient" of temperature, to be one degree centigrade
in 35 metres) the downward extension of such rocks might, _prima
facie_, be as much as 19 kilometres.

About this calculation we have to observe that we assume the
average radioactivity of the materials with which we have dealt
at the surface to extend uniformly all the way down, _i.e._ that
our experiments reveal the average radioactivity of a radioactive
crust. There is much to be said for this assumption. The rocks
which enter into the measurements come from all depths of the
crust. It is highly probable that the less silicious, _i.e._ the
more basic, rocks, mainly come from considerable depths; the more
acid or silica-rich rocks, from higher levels in the crust. The
radioactivity determined as the mean of the values for these two
classes of rock closely agrees with that found for intermediate
rocks, or rocks containing an intermediate amount of silica.
Clarke contends that this last class of material probably
represents the average composition of the Earth's crust so far as
it has been explored by us.

[1] The calorie referred to is the quantity of heat required to
heat one gram of water, _i.e._ one cubic centimetre of
water--through one degree centigrade.

126

It is therefore highly probable that the value found for the mean
radioactivity of acid and basic rocks, or that found for
intermediate rocks, truly represents the radioactive state of the
crust to a considerable depth. But it is easy to show that we
cannot with confidence speak of the thickness of this crust as
determinable by equating the heat outflow at the surface with the
heat production of this average rock.

This appears in the failure of a radioactive layer, taken at a
thickness of about 19-kilometres, to account for the deep-seated
high temperatures which we find to be indicated by volcanic
phenomena at many places on the surface. It is not hard to show
that the 19-kilometre layer would account for a temperature no
higher than about 270 deg. >C. at its base.

It is true that this will be augmented beneath the sedimentary
deposits as we shall presently see; and that it is just in
association with these deposits that deep-seated temperatures are
most in evidence at the surface; but still the result that the
maximum temperature beneath the crust in gen