Isotopic analyses were performed on a VG Sector Mass Spectrometer in the laboratory of M. D. Feigenson at Rutgers. These ratios were plotted versus depth (Figs. 2, 3). The error bars shown (Figs. 2,3, table 1) are machine precision for each analysis on the mass spectrometer results.
Figure 2: Sr-isotopic values vs. Depth at Bass River. The error bars are machine precision for each analysis.

Figure 3: Sr-isotopic values vs. Depth at Ancora. The error bars refelect the accuracy of each analysis.

Isotopic ratios were converted to ages by correlation with the Sr curve of McArthur and Howard (1988) (Figs. 4 - 6).
Figure 4: An age-depth plot was constructed using the McArthur and Howard Sr curve. Gaps in the data occur where the sediments contained too little SrCO3 to analyze. Error bars are ±1 Ma

Figure 5: An age vs. depth plot for Ancora was constructed by using previously determined sequence boundaries (Miller et. al., 1999). Each sequence was considered separately. Error bars are ±1 Ma

Figure 6: Considering the ages at Ancora as a single data set rather than multiple sets (figure 5) provides a better illustration of the sequences. The r2 value obtained was (0.953). Error bars are ±1 Ma

Sr-isotopic age estimates at Ancora increase within the expected sample error from 65.53 Ma at 643.1 ft (196.0 m) to 80.75 Ma at 921.9 ft (281.0 m). Ages of the individual formations at Bass River are offset from those at Ancora (Fig. 7), although the offset is relatively minor (<2 Ma) for the interval examined.
Figure 7: The Upper Cretaceous sections of the Bass River and the Ancora boreholes are depicted with ages for both sequence boundaries and formations. Note the slight offset in ages between the two boreholes.

Although Sr developed ages at Bass River are thought to be altered by diagenesis (Miller et al. 1999), the offset of ages between the two boreholes in this study are not conclusive.
At Ancora, Sr-isotopic age estimates generally increase with depth from 650 ft (198.1 m) to 950 ft (289.6 m) (Figs. 5, 6). Error bars were added taking into consideration machine error as well as the limitations of the dating technique (i.e., external precision and errors in the age regression). Two plots are provided: 1) using a fixed error of ± 1 m.y as a conservative error estimate (Fig. 8a, left); and 2) using statistical age errors provided by McArthur and Howard (1988) (Fig. 8b, right). Although McArthur and Howard (1998) purport to estimate errors statistically, their errors are extremely small for the interval considered. In contrast to their errors, Sugarman et. al. (1995) estimated the Maastrichtian Sr-isotope/ age regression had an error of approximately ± 1 Ma External precision (sample reproducibility) at Rutgers has been estimated statistically as ± 0.00020/ Ma (Oslick et. al., 1994). Given that the rate of change of Sr-isotopic ratios was 0.00022/ Ma for the interval 70 to 82 Ma (McArthur and Howard, 1998), a minimum error estimate would be ± 0.9 Ma Given that the McArthur and Howard (1998) age errors are unrealistically small, we show errors of ± 1 Ma as a conservative estimate.
Figure 8: a) and b) Error bars from this study are compared to those of McArthur et al. (1998) The error bars of ± 1 Ma better illustrate the interval considered.

The age-depth model shows a distinct hiatus associated with the Navesink/Mount Laurel contact. At 650 ft (198.1 m), the Sr age is 66.5 Ma. A significant offset (hiatus) in the ages occurs between the samples at 650 and at 652 ft (66.5 and 71.5 Ma). This offset correlates with a large spike in the gamma log obtained from Miller et al. (1999 ) (Fig. 9). This confirms work done previously on this sequence boundary (Miller et. al., in press, Miller et. al., 1999). The use of gamma log and lithologic data furnished by Miller's earlier studies supports the location of the sequence boundary detected by this study. The base of the Navesink, dated at approximately 66.5 Ma, and the top of the Mt. Laurel, dated at about 71.5 Ma, constrain the hiatus to a duration of 5.0 Ma Below the Navesink/ Mt. Laurel contact, no other significant offsets (hiatuses) are noted.
The data were broken into three distinct groups corresponding to the Mt. Laurel/Wenonah /Marshalltown, the upper and lower Englishtown, and the Woodbury/Merchantville sequences. Linear regression was performed on each group with r2 values of 0.775, 0.943, and 0.897. However, lumping the ages of all three sequences together (Fig. 6) provided an r2 value of 0.953 and better illustrates the sequences.
Physical stratigraphy requires that some time is not represented at sequence boundaries (i.e. hiatuses should be associated with these boundaries). Due to the brief duration of the other hiatuses, no marked separation was noted in Sr ages. Based on the error estimate described above, a hiatus less than ~1-2 Ma in duration would be too short to be detected. From this estimate it is concluded that the remaining hiatuses in the study are less than ~1-2 Ma Although more samples might better constrain these hiatuses, Sr-isotopic stratigraphy is limited by the errors associated with the dating technique. Some errors may be as large or larger than the actual duration of these hiatuses.
Although no other hiatuses could be readily seen, sequence boundaries could be identified through physical stratigraphy (Miller et. al. 1998, 1999) and dated. The sequence boundary separating the Marshalltown and the Englishtown (757.2 ft. at Ancora) is dated as ~75.0 Ma. The sequence boundary separating the upper and lower Englishtown (792.3 ft. at Ancora) is dated at ~76.2 Ma. The sequence boundary separating the Merchantville from the Cheesequake (945.3 ft. at Ancora) is dated as ~81.7 Ma. The sequence boundaries at 757.2 and 793.2 ft. are interpreted to be real due to kicks in the gamma log and changes of lithology (Fig. 9).
Figure 9: The gamma log and lithology (Miller et. al., 1999) is combined with the age-depth plot from this study. Note the large gamma spike at the Navesink/Mt. Laurel Formation boundary. No other significant offsets (hiatuses) are noted.

The dates of sequences and formations can be tied to the geomagnetic polarity time scale (GPTS) (Fig. 10).
Figure 10: The dates of the sequences were tied into the geomagnetic polarity time scale. The ages of this study link well with the established time scale.

The Sr-isotope stratigraphy predicts that the reversals associated with C33 and C34 should be represented in the fine-grained Wenonah Formation and the C34n/C35r should be represented in the fine-grained Woodbury Formation. Because coarse-grained, shallow-water units (e.g., Mount Laurel Formation) generally are unsuitable for magnetostratigraphy, future studies of magnetostratigraphy should focus primarily on the Wenonah and Woodbury Formations.
A comparison was also made to nannofossil data provided by Miller et. al.(1999). These three nannofossile-derived ages (L. de Romero, written communication, 2000) were plotted along with the Sr age-depth plot for Ancora (Fig. 9). Although the regression line for the age values parallels the plotted nannofossil data, there is an offset of approximately 2.5 Ma from the Sr-isotopic age estimates. We suggest the offset is due to calibration problems between nannofossils and the GPTS or Sr-isotopes and the GPTS. Future work is needed to evaluate both nannofossil-age and Sr-isotopic-age calibration.
Sr-isotope data suggest that sedimentation rates remained fairly constant throughout the Merchantville to Mount Laurel Formations. The sedimentation rate for the interval studied is 8.74 m/Ma (0.0874 cm/ka) This relative constancy is somewhat surprising considering the diverse marine and deepmarine environments represented, but it is consistent with previous studies (Sugarman et. al., 1995)
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