Rough Ways Made Smooth: A series of familiar essays on scientific subjectsProctor, Richard A. (Richard Anthony)
Science
Rough Ways Made Smooth: A series of familiar essays on scientific subjects
Proctor, Richard A. (Richard Anthony)
Science
I would, in conclusion, invite those who have the requisite leisure to
a careful study of the distribution of various orders of lunar marking.
It would be well if the moon's surface were isographically charted,
and the distribution of the seas, mountain ranges, and craters of
different dimensions and character, of rills, radiating streaks, bright
and dark regions, and so on, carefully compared _inter se_, with the
object of determining whether the different parts of the moon's surface
were probably brought to their present condition during earlier or
later periods, and of interpreting also the significance of the moon's
characteristic peculiarities. In this department of astronomy, as in
some others, the effectiveness of well-devised processes of charting
has been hitherto overlooked.
FOOTNOTES:
[Footnote 8: It would still be somewhat denser, because under the
circumstances it would be somewhat cooler.]
[Footnote 9: It is thus, and not by the effects due to increasing
pressure (effects which probably do not increase beyond a certain
point), that we are to explain the fact that the earth's density as a
whole is about twice the mean density of the matters which form its
solid surface. It may be that this consideration, supported by the
results of recent experimental researches, may give a significance
hitherto not noted to the relatively small mean density of the moon.]
[Footnote 10: I have occasion to make some remarks at this stage
to avoid possible and (my experience has shown me) not altogether
improbable misconception, or even misrepresentation. The theory
enunciated above will be regarded by some, who may have read a certain
review of my Treatise on the Moon, as totally different from what I
have advocated in that work, and, furthermore, as a theory which I
have borrowed from the aforesaid review. I should not be particularly
concerned if I had occasion to modify views I had formerly expressed,
since I apprehend that every active student of science should hope,
rather than dread, that as his work proceeds he would form new
opinions. But I must point out that earlier in my book I had advocated
the theory urged above. After describing the radiations from Tycho
and other craters, I proceed as follows in chapter iv.--'It appears
to me impossible to refer these phenomena to any general cause but
the reaction of the moon's interior overcoming the tension of the
crust, and to this degree Nasmyth's theory seems correct; but it
appears manifest, also, that the crust cannot have been fractured
in the ordinary sense of the word. Since, however, it results from
Mallet's investigations that the tension of the crust is called into
play in the earlier stages of contraction, and its power to resist
contraction in the later stages,--in other words, since the crust at
first contracts faster than the nucleus, and afterwards not so fast as
the nucleus,--we may assume that the radiating systems were formed in
so early an era that the crust was plastic.
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