| Remote Sensing and GIS analysis
of the Strangways and Shoemaker Impact Structures, Australia
German
Contact: Heiko Zumsprekel, Geologisch Paläontologisches Institut,
Corrensstr. 24, D-48149, Tel.: +49-(0)251-83-33908, zumspre@uni-muenster.de
In Australia numerous impact structures of probable or known
Precambrian age have been recognized by remote sensing and following field
investigations during the last years. The good preservation of these
ancient meteorite craters on the Australian continent is mainly due to
two factors: the excellent exposition of moderately deformed and largely
unmetamorphosed Proterozoic sedimentary rocks, and the fairly structural
stability of the Australian craton throughout Earth's history. Besides,
the identification of impact structures is favored by (semi)arid climate
conditions in most parts of inner Australia.
Within the scope of this Phd project the Australian impact structures
Strangways (N.T.) and Shoemaker
(W.A.) were investigated using complementary remote sensing data,
field data acquired between July and September 1999, and previous geological
mapping data conducted by the regional geological surveys and E.M.
and C.S. Shoemaker, respectively. With the construction
of a comprehensive GIS database for both meteorite craters, the study focuses
on a direct comparison of the impact signatures on a micro- (shock metamorphism),
meso- (shatter cones, impactites) and macro-scale (satellite and airborne
imagery). Both craters are comparable regarding (i) target material consisting
of siliciclastic sediments on top of crystalline basement rocks (ii) their
present diameter of about 20 km (Strangways) and 31 km (Shoemaker) and
(iii) their probably Proterozoic age.
Strangways (646 +/- 42 Ma) consists of sedimentary rocks of the Proterozoic
Roper Group which form a collar around a core of granites and gneisses.
During the field work shatter cones have been found in the granitoid basement
and the lower part of the Roper Group (Limmen Sandstone). Remnants of melt-bearing
impactites are limited to a few outcrops in the inner part of the structure.
Impact breccias dominated either by granitoid or sedimentary fragments
are distributed in the N‘ and E‘ part of the core. Further features diagnostic
for an impact event are PDFs found in quartz and feldspar of the granitoid
basement. In the Shoemaker Structure (1630 Ma ?) impactites are totally
removed as the structure is eroded below its previous crater floor. The
granitoid core is surrounded by sedimentary rocks of the Proterozoic Earaheedy
Group which are dropped down in a ring syncline. Indistinct shatter cones
are developed in granitoid rocks and the lower stratigraphic units of the
Earaheedy Group (Yelma and Frere Formation), PDFs occur in granites and
syenites in the N‘ core. Outcrops of upper parts of the Earaheedy Group
and dipping directions indicate that the level of erosion decreases in NE‘
direction.
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ASTER image of the Shoemaker
Impact Structure. The crater is easily detectable by the circular arrangement of
Proterozoic granular iron formations which appear dark in the image. (Acquisition
date 04Nov2000, bands: 3, 2, 1(rgb), coverage ca. 63.5 x 61 km).
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ERS 2 radar image of Strangways
combined with DEM (violet: low topography to yellow: high topography). The crater can be traced by
the circular arrangement of Proterozoic sandstones. The yellow elevated plateaus
in the center consist of post-impact Cretaceous sandstones (coverage ca. 40 x 40 km.).
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After the GIS integration of topographic and geological maps, multispectral
Landsat 5 TM data have been processed in order to obtain highly decorrelated
RGB-colour-composites for visual interpretation and computer-supported
classification. Among the statistical analysis of original TM bands the
use of standard image processing methods like ratioing and principal components
transformation has been evaluated in order to enhance the discrimination
between target materials, impactites (Strangways) and post-impact lithologies.
Especially principal components of higher order lead to a better differentiation
of Proterozoic sedimentary rocks of the Roper and Earaheedy Group, respectively.
Because of the limited spatial (30 x 30 m) and spectral resolution and interferences
between the spectral characteristics of rock types, weathering products
and vegetation types, the results of computer-supported unsupervised and
supervised classifications of Landsat TM data of the Shoemaker Structure
are not satisfactory. The object-oriented classification method represents
a more flexible way and allows the integration of spatial and textural decision
rules in the classification process which can lead to a slight improvement
of the classification results compared with pixel-based methods.
Complementary ERS-SAR radar data have been processed which allow the
analysis of the crater morphologies. The data can be used to add detailed
textural information to digital elevation models by merging methods. Aeroradiometric
data represent powerful additional information which are less influenced
by morphological parameters, surficial deposits and vegetation effects.
As the processing of aeromagnetic data differs significantly from optical
remote sensing data, pre-processed data of the craters supplied by the
Australian Geological Survey Organisation have been used in this case.
The aeromagnetic data allow careful temporal correlations between the intrusion
of dykes and the impact events which correlate with geochronological dating
of the impact structures.
Rock distributions and lineations have been mapped on the basis of a
visual interpretation scheme considering all remote sensing datasets and
have been compared with field observations. In order to reconstruct original
crater diameters, the spatial distribution of shatter cones has been used
leading to an original crater diameter of 21 to 29 km in case of Strangways
and < 42 km in case of the Shoemaker Structure. Among causal connection
between the datasets, the GIS database allows the spatial integration of
field observations and an adequate 2,5-D-visualisation of the crater morphologies.
Regarding further investigations on the Strangways and Shoemaker Structure
the integration of hyperspectral and additional seismic data is suggested.
As the two study cases show, a GIS approach with its central organisation
of impact data can also be successfully applied for the investigation of
other terrestrial impact structures.
Download
the full thesis (in German) as PDF (16 MByte). Send an email for obtaining a
CD-Rom with the GIS data in ArcView/ArcExplorer.
Work has been funded by
the DFG project "Origin and Evolution of the Solar System" performed by
the Institute
of Planetology at the University of Muenster since 1995. The Australian Geological Survey Organisation
is acknowledged for supplying aeroradiometric and aeromagnetic raw data.
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