PALAIOS
HOME HELP FEEDBACK SUBSCRIPTIONS ARCHIVE SEARCH TABLE OF CONTENTS
 QUICK SEARCH:   [advanced]


     


PALAIOS; June 2009; v. 24; no. 6; p. 377-386; DOI: 10.2110/palo.2008.p08-101r
© 2009 SEPM Society for Sedimentary Geology
This Article
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Citing Articles
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by WIERZBOWSKI, H.
Right arrow Articles by JOACHIMSKI, M. M.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

RESEARCH ARTICLES

STABLE ISOTOPES, ELEMENTAL DISTRIBUTION, AND GROWTH RINGS OF BELEMNOPSID BELEMNITE ROSTRA: PROXIES FOR BELEMNITE LIFE HABITAT

HUBERT WIERZBOWSKI*,1 and MICHAEL M. JOACHIMSKI2

1 Institute of Geological Sciences, Polish Academy of Sciences, ul. Twarda 51/55, 00-818 Warsaw, Poland
2 GeoCenter Northern Bavaria, University of Erlangen-Nuremberg, Schlossgarten 5, 91054 Erlangen, Germany hwierzbo{at}twarda.pan.pl

Stables isotopes and elemental composition of two well-preserved belemnite rostra (Hibolithes beyrichi and H. hastatus) from the Bathonian of central Poland were studied. Average temperatures calculated from the oxygen isotope ratios of Hibolithes beyrichi and H. hastatus are 10°C and 6°C, respectively. The absence of high-amplitude variations in high-resolution temperature profiles suggests these belemnites lived in deeper waters. This interpretation is compatible with a nektobenthic habitat of belemnopsid belemnites. Carbon isotope ratios of the rostra are assumed to be affected by vital fractionation with prominent fluctuations in the {delta}13C records resulting from changes in the metabolic activity. Observed variations in Mg:Ca ratios of the rostra (from 5 mmolFormulamol–1 to 28 mmolFormulamol–1) are predominantly a primary signal. Temperature dependence of the Mg:Ca ratio is inferred for H. beyrichi on the basis of a correlation with {delta}18O values; however, no such correlation is observed for H. hastatus. No significant correlation is observed between Sr:Ca ratios and {delta}18O values in either taxon. Sulphur contents in the rostra vary from 630 ppm to 4400 ppm and are interpreted to be largely coprecipitated with belemnite calcite. Extreme compositions of sulphur are interpreted to result from the incorporation of diagenetic sulphur during early marine diagenesis, which is also characterized in these rostra by high Mg:Ca and Sr:Ca ratios and low {delta}13C values. A total number of growth rings in the rostrum of H. beyrichi is calculated at around 600, thus, an expected life span of H. beyrichi is considered to be ~1.5 years assuming daily precipitation of growth bands.







HOME HELP FEEDBACK SUBSCRIPTIONS ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2009 by the SEPM Society for Sedimentary Geology.