DINOSAUR TRACK AND SUBAERIAL EXPOSURE SURFACES IN THE ALBIAN GLEN ROSE FORMATION OF CENTRAL TEXAS
First, isotope data show that not all track-bearing layers are associated with a negative-upward trend in carbon and oxygen stable isotope composition (δ13C and δ18O, respectively). At Starzville, a 2 and 1 ‰ drop in δ13C and δ18O values, respectively, in the 70 cm below the track-bearing layer results from the subaerial exposure of the track layer deposited in a shallow marine environment and altered by meteoric fluids; this is confirmed by the strongly negative δ13C and δ18O values measured in the marly infill of burrows from the track layer. Such a trend is not seen at other study locations: at Blanco River, a 1.5 ‰ decrease in δ18O values and no significant change in δ13C values is recorded from the start of the measured section up to the track layer, and an increasing trend in both δ13C and δ18O values characterizes the 1 m-thick interval underneath the tracklayer at San Gabriel.
Second, Chemical Index of Alteration values calculated from elemental geochemistry are above 80 in all study locations, suggesting a moderate to intense alteration of landmasses under greenhouse conditions. The absence of a strong negative δ13C excursion associated with track layers suggests either a lack of well-developed vegetation on land that would constitute a source of soil-respired CO2, or the preferential preservation of undertrack layers. In the latter case, negative δ13C values associated with the track layer would have been eroded during a subsequent sea-level rise, resulting in a stratigraphic hiatus. This observation could serve as a tool to differentiate true track from undertrack layers developed under greenhouse climate conditions.