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South
flank of the prehistoric and strongly terraced complex cone of
Monte Troina near the town of Pedara, with the snow-covered main
edifice of Mount Etna in the background, 12 May 1996. Monte Troina
consists of several nested cones, the southernmost of which, seen
in this photograph, is open to the south and actually contains
a small, horseshoe-shaped nested cone whose rim forms the sharp
rim in the left portion of the image |
Mamma
Etna's countless children
Monte Troina
SE flank, 15.060314° E, 37.611419° N
Summit elevation: 632 m (SW crater rim)
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Lying
immediately to the south of the center of the town of Pedara, Monte Troina
is a complex of three coalesced cones lying along a NNW-SSE-trending eruptive
fissure with a minimum length of 700 m. The age of Monte Troina is certainly
prehistoric, and it appears more strongly modified by agricultural activity
than most other flank cones in the area. It is possible that further small
edifices produced by the same eruption lie on the northern extension of
the aforementioned fissure, beneath the historical center of Pedara.
The cone complex of Monte Troina has three major craters, the southernmost
of which is open to the south and appears to contain, on its southern
side, a small nested cone which is also open to the south; the shallow
central crater has a prominent breach on its southeast side, while the
equally shallow northernmost crater is inclined toward north. A sanctuary,
unfortunately almost entirely constructed of concrete and thus aesthetically
, lies on the northern rim of the northern crater. On the northern side,
near the town of Pedara, the height of Monte Troina is only about 20 meters,
but its summit stands nearly 100 m above the south base of the cone complex.
At the south base of Monte Troina lies a peculiar, broad and irregularly
shaped depression which might be a collapsed effusive vent or an explosion
crater. An investigation of the deposits on the rims of the southern crater
failed to reveal any lithic material that would have been ejected from
a nearby explosion crater, so that an origin by collapse of the depression
at the south base is more likely.
I first climbed Monte Troina on 5 March 2004, when most of the photographs
shown on this page were taken. Access to this complex of pyroclastic cones
is relatively easy; a small footpath leads to the summit area immediately
to the east of the concrete sanctuary on the northern side of the complex.
Small tracks go across all of the summit area, whose vegetation is relatively
sparse, and a visit to this area offers fine panoramic views over nearly
all of the numerous pyroclastic cones on the southern and southeastern
flank of Etna, and invites the visitor to marvel at the dense urbanization
of the area.
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Left:
difficult to recognize in photograph, but this view shows the nested
"inner" southern crater, whose southward opening is seen
as a kind of trench in the center of the image; rim of the "outer"
southern crater is seen in center-left background
Center: looking straight down through the open south side of the
"inner" southern crater, onto the floor of a large depression
that lies at the south base of Monte Troina - possibly a collapsed
effusive vent
Right: a more complete view of the depression at the south base
of Monte Troina. The small dark cone of Monte
Trigona can be seen in the distance, surrounded by buildings.
Photos taken 5 March 2004 |
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