Science in Short ChaptersWilliams, W. Mattieu (William Mattieu)
Science
Science in Short Chapters
Williams, W. Mattieu (William Mattieu)
Science
According to this, the Earth, if it has cooled as the Moon is supposed
to have done, should have displayed corresponding irregularities,
and generally, the magnitude of mountains of solidified planets and
satellites should be on a scale proportionate to their whole mass.
In comparing the mountains of the Moon and _Mercury_ with those of
the Earth, a large error is commonly made by taking the customary
measurements of terrestrial mountain-heights from the sea-level. As
those portions of the Earth which rise above the waters are but its
upper mountain slopes, and the ocean bottom forms its lower plains
and valleys, we must add the greatest ocean depths to our customary
measurements, in order to state the full height of what remains of the
original mountains of the Earth. As all the stratified rocks have been
formed by the wearing down of the original upper slopes and summits, we
cannot expect to be able to recognize the original skeleton form of our
water-washed globe.
If my calculation of the atmosphere of _Mercury_ is correct, viz.,
that its pressure is equal to about one seventh of the Earth’s, or
4¼ inches of mercury, there can be no liquid water on that planet,
excepting perhaps over a small amount of circumpolar area, and during
the extremes of its aphelion winter. Thus the irregularities of the
terminator, indicating mountain elevations calculated to reach to
1/253 of the diameter of the planet, are quite in accordance with the
above-stated theoretical consideration.
There is one peculiar feature presented by the cones of the cooling
cinder which is especially interesting. The flow of fused cinder
from the little crater is at first copious and continuous; then it
diminishes and becomes alternating, by a rising and falling of the
fused mass within the cone. Ultimately the flow ceases, and then the
inner liquid sinks, more or less, below the level of the orifice. In
some cases, where much gas is evolved, this sinking is so considerable
as to leave the cone as a mere hollow shell; the inner liquid having
settled down and solidified with a flat or slightly rounded surface, at
about the level of the base of the cone, or even lower. These hollow
cones were remarkably displayed in some of the cinder of the Henderson
iron, and their formation was obviously promoted by the abundant
evolution of gas.
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