Geological and geochemical data from the proposed Sirente crater field: New age dating and evidence for heating of target Item Type Article; text Authors Ormö, Jens; Koeberl, Christian; Rossi, Angelo Pio; Komatsu, Goro Citation Ormö, J., Koeberl, C., Rossi, A. P., & Komatsu, G. (2006). Geological and geochemical data from the proposed Sirente crater field: New age dating and evidence for heating of target. Meteoritics & Planetary Science, 41(9), 1331-1345. DOI 10.1111/j.1945-5100.2006.tb00525.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 27/09/2021 20:14:45 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656183 Meteoritics & Planetary Science 41, Nr 9, 1331–1345 (2006) Abstract available online at http://meteoritics.org Geological and geochemical data from the proposed Sirente crater field: New age dating and evidence for heating of target Jens ORMÖ1*, Christian KOEBERL2, Angelo Pio ROSSI3, 4, and Goro KOMATSU3 1Centro de Astrobiología (CSIC/INTA), Instituto Nacional de Técnica Aeroespacial, Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain 2Department of Geological Sciences, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria 3International Research School of Planetary Sciences, Universita d’Annunzio, Viale Pindaro 42, 65127 Pescara, Italy 4ESA Research and Scientific Support Department, Keplerlaan 1, Postbus 299, ESTEC/SCI-SB, 2200 AG Noordwijk, The Netherlands *Corresponding author. E-mail:
[email protected] (Received 23 February 2006; revision accepted 05 July 2006) Abstract–The proposed Sirente crater field consists of a slightly oblong main structure (main crater) 120 m in width and about 30 smaller structures (satellite craters), all in unconsolidated but stiff carbonate mud.