132 Planetary Geology (Posters)
Wednesday, 7 November 2001
1:30 PM - 5:30 PM
AN EXTRATERRESTRIAL COMPONENT AT THE PERMO-TRIASSIC BOUNDARY? CLUES FROM SIDEROPHILE ELEMENT ABUNDANCES
Paper number: 132-5
Program: Technical Sessions
Time: 1:30 PM – 5:30 PM
Authors
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Heinz HuberUniv of Vienna, Vienna, N/A
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Mark SephtonOpen Univ, Milton Keynes, N/A
Abstract
For the iridium analyses we used multiparameter gamma-gamma coincidence spectrometry, which allows the non-destructive determination of very low Ir concentrations (in the sub-ppb range). For the Gartnerkofel P-Tr boundary samples, we found Ir values of 65 - 155 ppt. These values are above background and confirm the anomalies found before; further analyses are in progress. The Val Badia section, which had not been analyzed for Ir contents before, gave even more encouraging results. The background samples have 21 - 65 ppt Ir, but one sample, coinciding exactly with a positive d13C (carbonate) peak, and an even more distinct d13C (alkanes peak), has 242 ppt Ir. A second (close) sample, also coinciding with a (less pronounced) d13C (alkanes peak) has 120 ppt Ir. These observations do not prove the extraterrestrial nature of the Ir, but it was possible to confirm the presence of an Ir anomaly. We are currently measuring the Os-isotopic composition and the platinum-group element abundances in the samples to obtain further clues regarding the origin of the siderophile element anomaly.