Development of AMS allowed targeting oxalate minerals – whewellite and wedellite as a dating material for rock art. Further studies have confirmed that carbon in oxalates is not derived from the substrate on which they grow but most probably originate from bacteria and other microbiota residing on rock surfaces utilising atmospheric source. The other rock surface objects which potentially carry oxalates are the remnants of mud dauber nests. Oxalates could form post-construction from bacterial activity utilising favourable conditions in the nest stump. One more recognised source of oxalates associated with rock art is the use of plans sap as a binder for mineral pigments. In all instances oxalates on the rock surface exist in a mixture with other materials which could be carbon bearing contaminants. Hence the study of a bulk sample ends in radiocarbon concentrations of an average of all carbon compounds with unknown source and relationship with the inferred art. Therefore, chemical pretreatmed methods were developed to isolate and target a specific compound, in our case calcium oxalate. We present data of exploiting such compound-specific dating approach on mineral skins, pigments and other rock surface deposits from Northern Australian and African rock art sites. The presence of whewellite was investigated with X-ray diffraction, scanning electron microscopy and infrared spectroscopy methods. Selectiveness of the method and further studies are discussed.

Oxalate minerals for rock art dating: study continues / Vladimir A. Levchenko, Tristen Jones, Penelope King, Alan Williams, Damien G. Finch, Elena Pecchioni, Orlando Vaselli. - CD-ROM. - (2018), pp. 55-55. (Intervento presentato al convegno 20th International Rock Art Congress IFRAO 2018 Valcamonica Darfo Boario Terme (Bs) Italy).

Oxalate minerals for rock art dating: study continues

Elena Pecchioni
Membro del Collaboration Group
;
Orlando Vaselli
Membro del Collaboration Group
2018

Abstract

Development of AMS allowed targeting oxalate minerals – whewellite and wedellite as a dating material for rock art. Further studies have confirmed that carbon in oxalates is not derived from the substrate on which they grow but most probably originate from bacteria and other microbiota residing on rock surfaces utilising atmospheric source. The other rock surface objects which potentially carry oxalates are the remnants of mud dauber nests. Oxalates could form post-construction from bacterial activity utilising favourable conditions in the nest stump. One more recognised source of oxalates associated with rock art is the use of plans sap as a binder for mineral pigments. In all instances oxalates on the rock surface exist in a mixture with other materials which could be carbon bearing contaminants. Hence the study of a bulk sample ends in radiocarbon concentrations of an average of all carbon compounds with unknown source and relationship with the inferred art. Therefore, chemical pretreatmed methods were developed to isolate and target a specific compound, in our case calcium oxalate. We present data of exploiting such compound-specific dating approach on mineral skins, pigments and other rock surface deposits from Northern Australian and African rock art sites. The presence of whewellite was investigated with X-ray diffraction, scanning electron microscopy and infrared spectroscopy methods. Selectiveness of the method and further studies are discussed.
2018
20th International Rock Art Congress IFRAO 2018 "Standing on the shoulders of giants"
20th International Rock Art Congress IFRAO 2018 Valcamonica Darfo Boario Terme (Bs) Italy
Vladimir A. Levchenko, Tristen Jones, Penelope King, Alan Williams, Damien G. Finch, Elena Pecchioni, Orlando Vaselli
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1133861
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