|
|
|
|||||||||||||||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |
1 Department of Geology, Asutosh College, Kolkata 700 026, India
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 (21001600 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.
Key Words: tidal rhythmite tidal cycles lunar orbital periodicity Earth-Moon system Paleoproterozoic Chaibasa Formation
This article has been cited by other articles:
![]() |
S. M. Reddy and D. A. D. Evans Palaeoproterozoic supercontinents and global evolution: correlations from core to atmosphere Geological Society, London, Special Publications, January 1, 2009; 323(1): 1 - 26. [Abstract] [Full Text] [PDF] |
||||
![]() |
R. Mazumder, J. P. Rodriguez-Lopez, M. Arima, and A. J. van Loon Palaeoproterozoic seismites (fine-grained facies of the Chaibasa Formation, east India) and their soft-sediment deformation structures Geological Society, London, Special Publications, January 1, 2009; 323(1): 301 - 318. [Abstract] [Full Text] [PDF] |
||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |