NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Chicxulub Impact Ejecta in BelizeChicxulub ejecta deposits in Belize provide the closest exposures of ejecta to the crater and the only exposures of proximal ejecta deposited in a terrestrial environment. A quarry on Albion Island in northern Belize exposes Late Cretaceous, possibly Maastrichtian, carbonate platform sediments that were folded, eroded, and subaerially weathered prior to the deposition of coarse ejecta from Chicxulub. These ejecta deposits are composed of a basal, about 1-m-thick clay and dolomite Spheroid Bed overlain by a about 15-m-thick coarse Diamictite Bed. Many and perhaps most of the clay spheroids are altered glass. Many dolomite spheroids have concentric layers and angular cores are probably of accretionary lapilli origin. A slight Ir concentration (111-152 ppt) was detected in the base of the Spheroid Bed. The Diamictite Bed contains about 10% altered glass, rare shocked quartz, 3-8 m diameter boulders and striated and polished cobbles, one with a penetrating rock chip that plastically deformed the cobble. Ejecta deposits extend to the surface at Albion and the maximum thickness in this area is not known. Ejecta deposits are exposed in several roadside quarries in the Cayo District of central Belize. The Late Cretaceous here is also represented by carbonate platform sediments. The upper surface of the carbonate platform is a highly irregular and extensively recrystallized horizon possibly representing deep karst weathering. Approximately 30 in of diamictite overlies this horizon with a texture similar to the Diamictite Bed at the Albion quarry, but with a more diverse lithology. In three locations the Cayo diamictites, contain red clay layers with abundant polished and striated limestone pebbles and cobbles called Pook's Pebbles, several of which have penetrating rock chips and ablated surfaces. We interpret the Albion Spheroid Bed as a deposit from the impact vapor plume and the Albion and Cayo diamictites as the result of a turbulent flow that contained debris derived from the ejecta curtain and local scouring. The polished, striated, and ablated Pook's Pebbles are interpreted as high altitude ballistic ejecta.
Document ID
20000031475
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Ocampo, A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Pope, K.
(Geo Eco Arc Research La Canada, CA United States)
Fischer, A.
(University of Southern California University Park, CA United States)
Alvarez, W.
(California Univ. Berkeley, CA United States)
Fouke, B.
(California Univ. Berkeley, CA United States)
Asaro, F.
(California Univ., Lawrence Berkeley Lab. Berkeley, CA United States)
Webster, C., Jr.
(Loma Linda Univ. CA United States)
Vega, F.
(Ciudad Univ. Mexico City, Mexico)
Smith, J.
(Vrije Univ. Amsterdam, Netherlands)
Fritsche, A. E.
(California State Univ. Northridge, CA United States)
Date Acquired
August 19, 2013
Publication Date
January 1, 1997
Publication Information
Publication: Large Meteorite Impacts and Planetary Evolution
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Available Downloads

There are no available downloads for this record.
No Preview Available