A shallow mud volcano in the sedimentary basin off the Island of Elba
Authors: Sciarra Alessandra , Saroni Anna , Grassa Fausto , Ivaldi Roberta , Demarte Maurizio , Lott Christian , Weber Miriam , Eich Andi , Cimenti Ettore , Mazzarini Francesco , Coltorti Massimo 
Published: March 2020

&lt;p&gt;The Island of Elba, located in the westernmost portion of the northern Cenozoic Apennine belt, is formed by metamorphic and non-metamorphic units derived from oceanic (i.e. Ligurian Domain) and continental (i.e. the Tuscan Domain) domains stacked toward NE during the Miocene.&lt;/p&gt;&lt;p&gt;Offshore, west of the Island of Elba, magnetic and gravimetric data suggest the occurrence of N-S trending ridges that, for the very high magnetic susceptibility, have been interpreted as serpentinites, associated with other ophiolitic rocks. Moving towards south in Tuscan domain, along N-S fault, there is clear evidence of off-shore gas seepage (mainly CH&lt;sub&gt;4&lt;/sub&gt;), which can be related to recent extensional activity.&lt;/p&gt;&lt;p&gt;In this contest, a cold methane seep was discovered in the sedimentary basin off Elba Island, characterized by typical mud volcanoes conditions. Generally, mud volcanoes are the shallow expression of subsurface processes characterized by movements of large masses of sediments and &amp;#239;&amp;#172;&amp;#130;uids. A marine mud volcanoes is a window into different depth levels of the submerged geosphere where hydrogen sulfide, methane and other hydrocarbon-rich fluid seepage occurs caused by tectonic activity. Indeed, vertical migration of geogas, especially CH&lt;sub&gt;4&lt;/sub&gt; from the reservoir strata to the sea floor occurs along focused, permeable migration pathways, often created by faults and fractures.&lt;/p&gt;&lt;p&gt;The sampled gas chemistry is typical of mud volcanoes, with methane as the prevalent gas component (&gt;95 vol%) and minor gases that include carbon dioxide, nitrogen and trace amounts of helium. The combined stable C and H isotope composition of CH&lt;sub&gt;4&lt;/sub&gt; (&amp;#948;&lt;sup&gt;13&lt;/sup&gt;C and &amp;#948;&lt;sup&gt;2&lt;/sup&gt;H) highlights a thermogenic origin of &amp;#239;&amp;#172;&amp;#130;uids discharged from mud volcano, contrary to likely abiotic origin gas found in the Pomonte seep and linked to serpentinized ultrama&amp;#239;&amp;#172;&amp;#129;c rock systems.&lt;/p&gt;&lt;p&gt;The samples collected on this mud volcano are extremely depleted in &lt;sup&gt;3&lt;/sup&gt;He and their &lt;sup&gt;3&lt;/sup&gt;He/&lt;sup&gt;4&lt;/sup&gt;He ratios are typical for a geological setting in which radiogenic crustal helium is strongly predominant. On the contrary, the Pomonte ophiolitic gas seeps show a mantle-derived &lt;sup&gt;3&lt;/sup&gt;He-rich component estimated in the range between 10 and 15%.&lt;/p&gt;&lt;p&gt;Petrological data highlight the presence of siltites and marly mudstones characterized by different origin than those found on neighboring islets (shallow marine organogenic limestones); therefore, the possibility that the fragments of rock blocks, found in the mud volcano area, derive form erosional processes of the islet is discarded. The conical shapes highlighted by the multibeam echosounder are very similar to the typical backscatter signature of other mud volcanoes, thus confirming the possibilities of classify this site as mud volcano. Indeed, already during the scuba diving survey that allowed sampling gas and sediment, it was clearly observed and documented as a mud volcano.&lt;/p&gt;