Open Access Open Access  Restricted Access Subscription Access

Late Cretaceous Diurnal Tidal System: A Study from Nimar Sandstone, Bagh Group, Narmada Valley, Central India


Affiliations
1 Department of Earth Sciences, Indian Institute of Technology, Roorkee 247 667, India
 

Tidalites from the Cenomanian Nimar Sandstone, Bagh Group, Central India, are represented by (i) laterally accreted tidal bundles, (ii) herringbone cross-strata, (iii) sigmoidal cross-strata and (iv) tidal rhythmites with lenticular/wavy bedding. These indicate sedimentation in an upper subtidal to lower intertidal setting within fluvio marine interactive system. Time-series analysis of continuous rhythmic foreset bundles (sub-annual scale) manifests neap-spring tidal cycles within a diurnal tidal system with synodic and sidereal month lengths of ∼28.4 lunar days and ∼26.28 solar days respectively. Estimated Earth-Moon system parameters of the Late Cretaceous reveal no significant changes during the last ∼100 Ma.

Keywords

Cenomanian, Cross-Strata, Lamina Thickness, Lunar Orbital Cyclicity, Tidal Bundles.
User
Notifications
Font Size

Abstract Views: 367

PDF Views: 143




  • Late Cretaceous Diurnal Tidal System: A Study from Nimar Sandstone, Bagh Group, Narmada Valley, Central India

Abstract Views: 367  |  PDF Views: 143

Authors

Biplab Bhattacharya
Department of Earth Sciences, Indian Institute of Technology, Roorkee 247 667, India
Suparna Jha
Department of Earth Sciences, Indian Institute of Technology, Roorkee 247 667, India

Abstract


Tidalites from the Cenomanian Nimar Sandstone, Bagh Group, Central India, are represented by (i) laterally accreted tidal bundles, (ii) herringbone cross-strata, (iii) sigmoidal cross-strata and (iv) tidal rhythmites with lenticular/wavy bedding. These indicate sedimentation in an upper subtidal to lower intertidal setting within fluvio marine interactive system. Time-series analysis of continuous rhythmic foreset bundles (sub-annual scale) manifests neap-spring tidal cycles within a diurnal tidal system with synodic and sidereal month lengths of ∼28.4 lunar days and ∼26.28 solar days respectively. Estimated Earth-Moon system parameters of the Late Cretaceous reveal no significant changes during the last ∼100 Ma.

Keywords


Cenomanian, Cross-Strata, Lamina Thickness, Lunar Orbital Cyclicity, Tidal Bundles.



DOI: https://doi.org/10.18520/cs%2Fv107%2Fi6%2F1032-1037