The Trouvelot astronomical drawings manual — John Shaqi
The Trouvelot astronomical drawings manualTrouvelot, E. L. (Etienne Leopold)
Science
The Trouvelot astronomical drawings manual
Trouvelot, E. L. (Etienne Leopold)
Astronomy -- Pictorial works
Notwithstanding their many points of similarity with the volcanoes of
the Earth, the lunar craters differ from them in many particulars,
showing that volcanic forces acting on different globes may produce
widely different results. For example, the floors of terrestrial craters
are usually situated at considerable elevations above the general
surface, while those of the lunar craters are generally much depressed,
the height of their walls being only about one-half the depth of their
cavities. Again, while on the Earth the mass of the volcanic cones far
exceeds the capacity of their openings, on the Moon it is not rare to
see the capacity of the crater cavities exceeding the mass of the
surrounding walls. On the Earth, the volcanic cones and mouths are
comparatively regular and smooth, and are generally due to the
accumulation of the ashes and the debris of all kinds which are ejected
from the volcanic mouths. On the Moon, very few craters show this
character, and for the most part their walls have a very different
structure, being irregular, very rugged, and composed of a succession of
concentric ridges, rising at many points to great elevations, and
forming peaks of stupendous height. Again, many of the larger
terrestrial craters have their interior occupied by a central cone, or
several such cones, having a volcanic mouth on their summits; on the
Moon such central cones are very rare. Although many of the large lunar
craters have their interior occupied by central masses which have been
often compared to the central cones of our great volcanoes, yet these
objects have a very different character and origin. For the most part,
they are mountainous masses of different forms--having very rarely any
craters on them--and seem to have resulted from the crowding and lifting
up of the crater floor by the phenomena of subsidence, of which these
craters show abundant signs. Besides, the terrestrial craters are
characterized by large and important lava streams, while on the Moon the
traces of such phenomena are quite rare, and when they are shown, they
generally differ from those of the Earth by their numerous and
complicated ramifications, and also by the fact that many of these lava
streamlets take their origin at a considerable distance from the crater
slopes, and are grooved and depressed as if the burning liquids which
are supposed to have produced them had subsequently disappeared, by
evaporation or otherwise, leaving the furrow empty.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account