Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate

Over the past decade the study of Precambrian clastic tidal rhythmites - stacked laminae of sandstone, siltstone and mudstone that display periodic variations in thickness reflecting a strong tidal influence on sedimentation - has provided accurate palaeotidal and palaeorotational data. Palaeotidal...

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Published in:Sedimentary Geology
Main Author: Williams, G.
Format: Article in Journal/Newspaper
Language:English
Published: ELSEVIER SCIENCE BV 1998
Subjects:
Online Access:http://hdl.handle.net/2440/13870
https://doi.org/10.1016/S0037-0738(98)00027-X
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spelling ftunivadelaidedl:oai:digital.library.adelaide.edu.au:2440/13870 2023-05-15T16:41:23+02:00 Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate Williams, G. 1998 http://hdl.handle.net/2440/13870 https://doi.org/10.1016/S0037-0738(98)00027-X en eng ELSEVIER SCIENCE BV Sedimentary Geology, 1998; 120(1-4):55-74 0037-0738 http://hdl.handle.net/2440/13870 doi:10.1016/S0037-0738(98)00027-X Journal article 1998 ftunivadelaidedl https://doi.org/10.1016/S0037-0738(98)00027-X 2023-02-05T19:51:43Z Over the past decade the study of Precambrian clastic tidal rhythmites - stacked laminae of sandstone, siltstone and mudstone that display periodic variations in thickness reflecting a strong tidal influence on sedimentation - has provided accurate palaeotidal and palaeorotational data. Palaeotidal records obtained from tidal rhythmites may be systematically abbreviated, however, and derived periods and frequencies can be misleading. The validity of such values, including past length of day, can be assessed by testing for internal self-consistency through application of the laws of celestial mechanics. Such a test supports the estimated length of day of 21.9 ± 0.4 h derived from the late Neoproterozoic (~620 Ma) Elatina-Reynella rhythmites in South Australia, and the indicated mean rate of lunar retreat of 2.16 ± 0.31 cm/year since ~620 Ma. The validity of estimated lengths of day obtained from other Precambrian tidal rhythmites remain unverified because the data sets contain only one primary value directly determined from the rhythmites. The Elatina-Reynella data militate against significant Earth expansion at least since ~620 Ma, and suggest that the free nutation or 'tipping' of the Earth's fluid core has undergone a resonance with the Earth's annual forced nutation since the Neoproterozoic. Glaciogenic deposits are readily distinguishable from ejecta resulting from impacts with Earth-crossing bodies. Palaeomagnetic data, based on the geocentric axial dipole model for the geomagnetic field, indicate that Neoproterozoic and Palaeoproterozoic glaciation and cold climate near sea level occurred in low palaeolatitudes. This enigmatic finding may imply global glaciation or an increased obliquity of the ecliptic, and is relevant to modelling the effect of ice sheet formation on the Earth's obliquity history by obliquity-oblateness feedback mechanisms. Through multidisciplinary studies, clastic sedimentology and geophysics together can make substantial contributions to understanding Precambrian Earth-Moon dynamics ... Article in Journal/Newspaper Ice Sheet The University of Adelaide: Digital Library Sedimentary Geology 120 1-4 55 74
institution Open Polar
collection The University of Adelaide: Digital Library
op_collection_id ftunivadelaidedl
language English
description Over the past decade the study of Precambrian clastic tidal rhythmites - stacked laminae of sandstone, siltstone and mudstone that display periodic variations in thickness reflecting a strong tidal influence on sedimentation - has provided accurate palaeotidal and palaeorotational data. Palaeotidal records obtained from tidal rhythmites may be systematically abbreviated, however, and derived periods and frequencies can be misleading. The validity of such values, including past length of day, can be assessed by testing for internal self-consistency through application of the laws of celestial mechanics. Such a test supports the estimated length of day of 21.9 ± 0.4 h derived from the late Neoproterozoic (~620 Ma) Elatina-Reynella rhythmites in South Australia, and the indicated mean rate of lunar retreat of 2.16 ± 0.31 cm/year since ~620 Ma. The validity of estimated lengths of day obtained from other Precambrian tidal rhythmites remain unverified because the data sets contain only one primary value directly determined from the rhythmites. The Elatina-Reynella data militate against significant Earth expansion at least since ~620 Ma, and suggest that the free nutation or 'tipping' of the Earth's fluid core has undergone a resonance with the Earth's annual forced nutation since the Neoproterozoic. Glaciogenic deposits are readily distinguishable from ejecta resulting from impacts with Earth-crossing bodies. Palaeomagnetic data, based on the geocentric axial dipole model for the geomagnetic field, indicate that Neoproterozoic and Palaeoproterozoic glaciation and cold climate near sea level occurred in low palaeolatitudes. This enigmatic finding may imply global glaciation or an increased obliquity of the ecliptic, and is relevant to modelling the effect of ice sheet formation on the Earth's obliquity history by obliquity-oblateness feedback mechanisms. Through multidisciplinary studies, clastic sedimentology and geophysics together can make substantial contributions to understanding Precambrian Earth-Moon dynamics ...
format Article in Journal/Newspaper
author Williams, G.
spellingShingle Williams, G.
Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate
author_facet Williams, G.
author_sort Williams, G.
title Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate
title_short Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate
title_full Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate
title_fullStr Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate
title_full_unstemmed Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth-Moon dynamics and palaeoclimate
title_sort precambrian tidal and glacial clastic deposits: implications for precambrian earth-moon dynamics and palaeoclimate
publisher ELSEVIER SCIENCE BV
publishDate 1998
url http://hdl.handle.net/2440/13870
https://doi.org/10.1016/S0037-0738(98)00027-X
genre Ice Sheet
genre_facet Ice Sheet
op_relation Sedimentary Geology, 1998; 120(1-4):55-74
0037-0738
http://hdl.handle.net/2440/13870
doi:10.1016/S0037-0738(98)00027-X
op_doi https://doi.org/10.1016/S0037-0738(98)00027-X
container_title Sedimentary Geology
container_volume 120
container_issue 1-4
container_start_page 55
op_container_end_page 74
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