14 Undergraduate Research II (Posters)

Monday, 19 April 2021
3:15 PM - 5:05 PM
Missouri Geological Survey Room


BULK SEDIMENTARY ORGANIC CARBON CHEMOSTRATIGRAPHY OF DINOSAUR-BEARING STRATA IN THE YUCCA FORMATION OF WEST TEXAS

Paper number: 14-4
Program: Theme Sessions
Time: 3:45 PM – 3:55 PM


Authors


Abstract

The Yucca Formation of West Texas sparse but important dinosaur fossils. The exact age of these Cretaceous dinosaur-bearing units are not well constrained. To that end, two stratigraphic sections were collected to construct C-isotope chemostratigraphic profiles using bulk sedimentary organic carbon. Bulk samples were decarbonated with 0.5M hydrochloric acid, rinsed, dried and weighed into tin capsules. One of the sections included a partial skeleton of a small ornithopod dinosaurs (“Yucca Dino Section”). The other section was collected near the Indio Mountains Field Station (“IMFS section”). Samples were combusted on a Costech 4010 Elemental analyzer attached to a Thermofinnigan MAT 253 isotope ratio mass spectrometer. Of the 10 samples ran from the “Yucca Dino Section”, the average δ13C was found to be -25.68‰ vs VPDB. For the “IMFS section”, 8 samples were analyzed averaging -25.18‰ vs VPDB. Overall, the isotopes values at the “Yucca Dino Section” show a gradual increase in isotope values, however it is unclear whether this is a result of changes in the c-cycle or related to depositional environment. The “IMFS section” showed little variation. Results were compared with marine organic C isotope chemostratigraphic records known to be Early Cretaceous and the positive trend may correlate with positive trends that occur in the Aptian and early Albian, but more data is needed . Future work should include analysis of longer stratigraphic sections.

Geological Society of America Abstracts with Programs. Vol. 53, No. 3

doi: 10.1130/abs/2021NC-362884

© Copyright 2021 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.