کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
6429823 1634770 2014 12 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
High elevation of the 'Nevadaplano' during the Late Cretaceous
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
پیش نمایش صفحه اول مقاله
High elevation of the 'Nevadaplano' during the Late Cretaceous
چکیده انگلیسی


- Clumped isotope thermometry is applied to Late Cretaceous and Paleocene terrestrial carbonates.
- The temperature estimates reflect summer conditions.
- When corrected for climate change, the temperature difference is 13.0 °C.
- The temperature difference implies a minimum elevation of 2.2-3.1 km for central Nevada.
- Uncertainties in our estimate broaden the range to ⩾2 km.

During the Late Cretaceous, central Nevada may have been a high elevation plateau, the Nevadaplano; some geodynamic models of the western US require thickened crust and high elevations during the Mesozoic to drive the subsequent tectonic events of the Cenozoic while other models do not. To test the hypothesis of high elevations during the late Mesozoic, we used carbonate clumped isotope thermometry to determine the temperature contrast between Late Cretaceous to Paleocene carbonates atop the putative plateau in Nevada versus carbonates from relatively low paleoelevation central Utah site. Lacustrine carbonates from the Nevada site preserve summer temperatures ∼13 °C cooler than summer temperatures from paleosol carbonates from the Utah site, after correcting for ∼1.2 °C of secular climatic cooling between the times of carbonate deposition at the two sites. This ∼13 °C temperature difference implies an elevation difference between the two sites of ∼2.2-3.1 km; including uncertainties from age estimation and climate change broadens this estimate to ⩾2 km. Our findings support crustal thickness estimates and Cenozoic tectonic models that imply thickened crust and high elevation in Nevada during the Mesozoic.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volume 386, 15 January 2014, Pages 52-63
نویسندگان
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