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The morphological rarity of the Apuan Alps has always
been an attraction for naturalists-travellers, or at least, it has been so
since the 16th century, when a scientific investigation on the mountain
range was carried out to understand its nature and find natural products
useful for economy. |
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Antonio
Vallisneri
(1714):
on the origin of
springs, based on an exploration in the Apuan Alps and Apennines |
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In 1833, for the first time the Apuan Alps are shown in a geological
cross-section in a work by Paolo Savi (1798-1871) who gives a ‘Plutonic’
interpretation of the mountain range. According to him, it was raised by the
intrusion of a deep magma body and became a remnant of an ancient orographic
ridge – called “metalliferous chain” – originally situated in the area from
La Spezia to Mt. Argentario. |
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Modern geology began with a systematic survey of the Apuan Alps completed between 1879 and 1890 by Bernardino Lotti (1847-1933) and Domenico Zaccagna (1851-1940). The two engineers of the Geological Royal Committee belonged to the ‘autochthonist’ school of thought assigning the Apuan rocks to a single stratigraphic sequence excluding any possibility of nappe overlapping. Therefore, they proposed a folding tectonics characterized by regular folds with double vergence without dealing with the existence of faults.
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The scientific commitment was matched with the institutional interest of the
Geological Committee, which aimed at providing the Apuan marble mining industry with an
useful instrument in a historic moment of remarkable spreading of quarrying
activities beyond the traditional basins of Carrara, Massa and the area of
Versilia.
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Domenico Zaccagna (1880-1886): Mt. Sagro's geological map - scale 1:25.000 |
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For the very first time in
the history of the Apuan Alps and Apennines the allochthonous origin of nappes was recognized, though it had already been
proposed by Lugeon and Argand for the Pennine Alps (1905) on the basis of
the overthrusting of two equivalent stratigraphic sequences. In the
following two decades the geological studies, especially by experts from the
central European school and culture, enabled the identification of a
‘tectonic window’ in the central part of the Apuan range. In particular, in
1926, Norbert Tillman (1883-1947) described the Apuan Alps as a complex
structure of folded sedimentary sequences which are overturned, faulted and
tectonically overlapped. After the Second World War the main subject of
geological studies was the gravitational sliding of nappes, which led Carlo
Migliorini (1891-1953) to formulate the theory of ‘composite wedges’ (1948),
according to which nappes may gradually slip for hundreds of kilometres
through different and subsequent phases thanks to a limited number of
inclined surfaces. The interpretation was then retrieved and developed by
Giovanni Merla (1906-1983) and Livio Trevisan (1909-1996), who, shortly
afterwards, described a gravitational sliding of nappes progressively moving
from the Tyrrhenian to the Adriatic area thanks to the upthrust of
subsequent tectonic ‘ridges’ or ‘wrinkles’. In the same period, Felice
Ippolito (1915-1997) carried out geological-petrographic studies on the
Apuan Alps and Pisani Mountains assigning the Apuan rocks to three
superposed sequences. The ‘Autochthonous’ sequence is the deepest one and is
overthrusted by an equivalent lithological sequence, called ‘Tuscan Nappe’
which is in turn topped by the ‘Ligurian Unit’. |
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Piero Elter (1974): Northern Apennines diagram block |
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