Interplay of orbital forcing and tectonic pulses in the Cambrian Iberian platform, NE Spain

Citation
Jj. Alvaro et al., Interplay of orbital forcing and tectonic pulses in the Cambrian Iberian platform, NE Spain, INT J E SCI, 89(2), 2000, pp. 366-376
Citations number
45
Categorie Soggetti
Earth Sciences
Journal title
INTERNATIONAL JOURNAL OF EARTH SCIENCES
ISSN journal
14373254 → ACNP
Volume
89
Issue
2
Year of publication
2000
Pages
366 - 376
Database
ISI
SICI code
1437-3254(200009)89:2<366:IOOFAT>2.0.ZU;2-L
Abstract
The stratigraphy of carbonate/shale couplets, cycles and cycle-stacking pat terns in a Cambrian shallow water platform (Iberian Chains, NE Spain) are r elated to sea-level changes driven by orbital forcing and by tectonic pulse s. The interplay of both effects can be discriminated in the Iberian fault- controlled platform, in which the tectonic activity can be analysed by accu rate and detailed biostratigraphic correlations based on trilobite zonation . The stratigraphic hierarchy of rhythmically interbedded limestones and sh ales, in two coeval but structurally separated geodynamic settings, yields cycle ratios of 1.44:1. This ratio is supported by time thickness and spect ral analysis, which is based on a graphic method of analysis: the Map of Gr ey Lines. The cycle ratio seems to be evidence for orbital forcing by obliq uity and precession cycles predicted for early Paleozoic time. Carbonate/sh ale couplets, the smallest rhythmic units recognisable in the field, repres ent short-term, periodic fluctuations in supply of terrigenous sediments an d carbonate productivity of uncertain origin, which could be associated wit h one of several harmonics of the former orbital cycles. The pulsating tect onic activity was approximated by using a quantitative analysis of tectonic ally induced subsidence (Shaw method). Recurrence frequencies of tectonic p ulses were estimated and dated by biostratigraphy. As a result, tectonic di sturbances in the Cambrian Iberian platform show an episodic periodicity co mparable to that of orbital eccentricity cycles, which could mask their rec ognition.