Implications of lunar orbital periodicity from the Chaibasa tidal rhythmite (India) of late Paleoproterozoic age

Details Implications of lunar orbital periodicity from the Chaibasa tidal rhythmite (India) of late Paleoproterozoic age Implications of lunar orbital periodicity from the Chaibasa tidal rhythmite (India) of late Paleoproterozoic age

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004geo....32..841m&link_type=abstract

Geology, vol. 32, Issue 10, p.841

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Scientific paper

Harmonic analysis of the sandstone foreset-laminae thickness series from the Chaibasa tidal rhythmite, India, clearly shows that a normal semidiurnal tidal system with synodic month of ˜32 lunar days was in effect during the late Paleoproterozoic (2100 1600 Ma). The minimum number of solar days in a lunar sidereal month was ˜31. Published quantitative tidal-rhythmite data of others in combination with data derived from the Chaibasa tidal rhythmite indicate long-term stability of the lunar orbit and progressive increase in the Earth-Moon distance during the Proterozoic.

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