Precambrian Length of Day and the Validity of Tidal Rhythmite Paleotidal Values

G.E. Williams
Department of Geology and Geophysics, University of Adelaide, Adelaide, SA 5005, Australia

Abstract:

Paleotidal records obtained from sedimentary tidal rhythmites may be systematically abbreviated and so may give incorrect paleotidal and paleorotational values. The validity of determined values, including past length of day (l.o.d.), can be assessed by testing for internal self- consistency through application of the laws of celestial mechanics. Three independent values obtained from the  620-Ma Elatina-Reynella rhythmites in South Australia (14.1 sidereal months/year, 401 sidereal days/year, and 19.5 years for the lunar nodal period), when employed in different equations that make allowance for lunar and solar tidal effects, each give a lunar semimajor axis in the range of 96.5-96.9consistency strongly supports the validity of the derived l.o.d. of 21.9 hours at  620 Ma. The validity of the estimated l.o.d. of 20.9 hours at  900 Ma (revised value, Big Cottonwood rhythmites, Utah) and of 17.1-18.9 hours at  2.5 Ga (Weeli Wolli rhythmites, Western Australia) cannot be assessed in that way because each data set has only one directly determined value. The derived mean rate of lunar retreat of 2.16 cm/year since  620 Ma averts a close approach of the Moon at least since 3 Ga and a lower rate of retreat seems likely during the Proterozoic.

AGU Index Terms: 1239 Rotational variations; Mineralogy, Petrology, and Rock Chemistry; 5450 Orbital and rotational dynamics
Keywords/Free Terms: Length of day, paleorotation, Precambrian, tidal rhythmites.

Geophysical Res. Ltrs. 97GL00234
Vol. 24 , No. 4 , p. 421


© 1997 AGU