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Earth Science Frontiers, Vol. 17, Special Issue, Aug. 2010 ISSN 1005-2321<br />

Epioceanic Depositional Sett<strong>in</strong>g <strong>and</strong> Skeletals from a Cephalopod<br />

Limestone (Betic Cordillera, SE Spa<strong>in</strong>): A Geochemical Approach<br />

R. Coimbra, F. Olóriz<br />

Departamento de Estratigrafía y Paleontología, Facultad de Ciencias, Universidad de Granada, Campus Universiario de Fuentenueva,<br />

Granada18002, Spa<strong>in</strong> (E-mail: foloriz@ugr.es)<br />

Geochemical data from four different types of<br />

carbonate materials are presented: micrite matrix from<br />

two sections (Cardador <strong>and</strong> Alamedilla), carbonate<br />

cements, neomorphic ammonite shells <strong>and</strong> belemnite<br />

rostra.<br />

Analysed materials belong to Lower Tithonian<br />

deposits, Semiforme/Verruciferum Zone, registered as<br />

Ammonitico Rosso facies <strong>in</strong> an epioceanic high<br />

(Cardador section), <strong>and</strong> a coeval cephalopod limestone<br />

deposited closer to the mid-Subbetic volcanic ridge<br />

(Alamedilla section).<br />

The Cardador section shows more <strong>and</strong> less<br />

calcareous, red-to-grey AR horizons with variable<br />

nodularity. Wackstones dom<strong>in</strong>ate conta<strong>in</strong><strong>in</strong>g radiolaria,<br />

calcisphaeres, calcareous d<strong>in</strong>oflagellates, plantik cri-<br />

noids (Saccocoma), unidentifiable benthic forams,<br />

ostracods, cephalopods (rare ammonitella or embrionic<br />

shell of ammonoids; aptychi), <strong>and</strong> fragments of<br />

juvenile <strong>and</strong> adult ammonite carcasses along with<br />

broken mollusks, ech<strong>in</strong>oderms (plates <strong>and</strong> sp<strong>in</strong>es),<br />

sponge spicules <strong>and</strong> pelagic bivalves, among others;<br />

packstone horizons ma<strong>in</strong>ly composed by filaments also<br />

occur.<br />

The Alamedilla section shows reddish-brownish-<br />

to-pale-grey limestone <strong>and</strong> marls. Limestones are<br />

locally rich <strong>in</strong> ammonites (cephalopod limestones)<br />

which preserve neomorphic shells <strong>and</strong> with<strong>in</strong>-bed<br />

orientation related to shell size, although horizontal<br />

settl<strong>in</strong>g is dom<strong>in</strong>ant. Wackstones dom<strong>in</strong>ate conta<strong>in</strong><strong>in</strong>g<br />

rare radiolaria, common to abundant calcareous d<strong>in</strong>o-<br />

flagellates, lesser amount of plantik cr<strong>in</strong>oids (Sacco-<br />

coma), benthic forams (most probably Lenticul<strong>in</strong>a),<br />

ostracods, cephalopods (common ammonitella or em-<br />

brionic shell of ammonoids), <strong>and</strong> fragments of juvenile<br />

<strong>and</strong> adult ammonite carcasses <strong>and</strong> rare aptychi, along<br />

with broken mollusks, lesser amount of small gastro-<br />

pods, rare brachiopods <strong>and</strong> ech<strong>in</strong>oderms (plates), <strong>and</strong><br />

variable amount of filaments (pelagic bivalves).<br />

H<strong>and</strong> specimens were collected under precise<br />

stratigraphic control <strong>and</strong> two slabs were produced for<br />

each sample: one for th<strong>in</strong> section preparation (micro-<br />

facies <strong>and</strong> cathodolum<strong>in</strong>escence) <strong>and</strong> the other for<br />

geochemical studies. Cathodolum<strong>in</strong>escence <strong>in</strong>spection<br />

was carried out <strong>in</strong> order to access the degree of<br />

diagenetic impr<strong>in</strong>t. Stable isotope analysis (carbon <strong>and</strong><br />

oxygen) was preformed on a total of seventy six h<strong>and</strong><br />

drilled bulk carbonate powder samples. Aliquots<br />

produced with the same powder sub-samples measured<br />

for isotope composition were analysed for their Ca, Mg,<br />

Mn, Fe <strong>and</strong> Sr elemental concentrations us<strong>in</strong>g <strong>in</strong>du-<br />

ctively coupled plasma-atomic emission spectrometry<br />

(ICP-AES).<br />

Cathodolum<strong>in</strong>escence imag<strong>in</strong>g of matrix micrite<br />

presents dist<strong>in</strong>ct degrees of lum<strong>in</strong>escence (Fig.1 B, F):<br />

brighter for micrite matrix from the Alamedilla section,<br />

attributed to an environmental enrichment <strong>in</strong> Mn 2+ , <strong>in</strong><br />

agreement with elemental data. A latter carbonate<br />

cement phase is identified as secondary blocky calcite<br />

(Fig.1 F) with alternat<strong>in</strong>g pattern between <strong>in</strong>tr<strong>in</strong>sic <strong>and</strong><br />

yellow lum<strong>in</strong>escence (zonation), provid<strong>in</strong>g evidence<br />

for shallow mar<strong>in</strong>e burial (Bruckschen <strong>and</strong> Richter,<br />

1994). Skeletal material shows overall <strong>in</strong>tr<strong>in</strong>sic dark<br />

lum<strong>in</strong>escence (Fig.1 B, D), suggest<strong>in</strong>g a fair presser-<br />

vation of both neomorphic ammonite shells <strong>and</strong> belem-<br />

nite rostra.<br />

Carbon isotope values for matrix micrite from the<br />

studied section at Cardador <strong>and</strong> the rock block from<br />

Alamedilla section, neomorphic ammonite shells <strong>and</strong><br />

secondary blocky calcite plot with<strong>in</strong> the same range of<br />

values, from 1.5‰ to 2.1‰. The obta<strong>in</strong>ed values are<br />

comparable to published data from other former<br />

Tethyan marg<strong>in</strong> locations (Jenkyns, 1996; Weissert <strong>and</strong><br />

Mohr, 1996; Bartol<strong>in</strong>i et al., 1999) that reflect Upper<br />

<strong>Jurassic</strong> seawater carbon isotope composition. Belem-<br />

nite rostra carbon isotope values differ from this trend,<br />

show<strong>in</strong>g δ 13 C values depleted as much as 3.8‰ relative<br />

to the encas<strong>in</strong>g matrix micrite (Alamedilla section). A<br />

likely lighter carbon source is metabolic carbon, that<br />

fails to be <strong>in</strong> equilibrium with seawater carbon due to<br />

the <strong>in</strong>ternal position of belemnite rostra (Price <strong>and</strong> Page,<br />

2008; Price et al., 2009).<br />

Oxygen isotope composition presents a higher<br />

variability. Matrix micrite from the Cardador section<br />

<strong>and</strong> neomorphic ammonite shells are the least depleted<br />

materials, rang<strong>in</strong>g from 0.1‰ to 0.9‰, followed by<br />

matrix micrite from Alamedilla <strong>and</strong> encased belemnite<br />

rostra. As most depleted, carbonate cements range from<br />

-2.7‰ to -0.3‰. Oxygen isotope composition is here<br />

considered to reflect mar<strong>in</strong>e bottom water paleo-<br />

temperature, except for carbonate cements, that <strong>in</strong>dicate<br />

higher temperature of circulat<strong>in</strong>g fluids dur<strong>in</strong>g mar<strong>in</strong>e<br />

burial diagenesis, supported by the observed zonation<br />

under cathodolum<strong>in</strong>escence.<br />

Elemental composition revealed an exceptional<br />

Mn enrichment on micrite matrix from Alamedilla (up<br />

to 4000 ppm), only present at the Cardador section on<br />

297

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