The Wonder Book of Volcanoes and EarthquakesHouston, Edwin J. (Edwin James)
Science
The Wonder Book of Volcanoes and Earthquakes
Houston, Edwin J. (Edwin James)
Earthquakes; Volcanoes
The relative positions of the other volcanic mountains of the
Mediterranean Sea; i. e., Etna, Stromboli, and the volcanoes of the
Santorin group of the Grecian Archipelago, are shown in the map, Fig.
12.
We will begin with the volcanic mountain of Etna, under which,
according to mythology, the angry gods had buried the rebellious
Typhoon.
Etna is situated on the island of Sicily, immediately southwest of
Italy. It is a much larger mountain than Vesuvius, rising, as it
does, from a circular base about eighty-seven miles around, to a
height of 10,840 feet above the level of the Mediterranean. It forms
a conspicuous object when seen either from the Mediterranean, or from
distant parts of Italy.
The height of Etna is so great that its slopes can be divided into
three distinct climatic zones or belts. The lowest of these lies
between the sea and a height of 2,500 feet. In this zone the mountain
slopes are covered with cultivated fields, olive groves, orchards,
and vineyards. The middle zone lies between 2,500 feet and 6,270
feet. This zone is covered with forests of chestnuts, oaks, beeches,
and cork trees. The third and highest zone includes the rest of the
mountain, and may be called the desert zone, since it is a sterile
region, covered with huge blocks of lava and scoriæ, and terminating,
in the higher portions, in a snow-covered plain, from which the
central cone rises.
Etna is continually sending up columns of steam and sulphur vapor.
Every now and then it starts in eruption, throwing out large
quantities of lava either from the crater on its summit, or from
some of the 200 smaller cones or craters that occupy portions of its
slopes. On account, probably, of its height the eruptions are most
frequently on the sides. Etna affords a magnificent example of a huge
volcanic pile of the Vesuvian type, which has been slowly built up
by the gradual accumulation of materials that have escaped from its
craters.
One of the most interesting features of the higher regions of Etna is
an immense chasm rent in a side of the cone near the summit, and known
as the Val del Bove. This chasm forms a vast amphitheater.
The great force that removed such an immense mass of matter from
the cone could not have been the eroding power of water, since the
materials of the cone are too porous to permit streams of any size to
rush down the slopes. The force is most probably to be found in some
explosive eruption of the mountain, when a portion of the crater was
suddenly blown off, just as was done in Vesuvius when a large part of
the old crater of Somma was blown away. What is especially interesting
about the Val del Bove is the opportunity it affords for studying the
interior structure of the mountain, for it practically enables one to
enter to almost the heart of this great volcano.
Public-domain text, read in full here on John Shaqi.
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