This
web page is dedicated to the memory of Dr Bob Hunter. It was Bob who formed the
TART and who is responsible for
enthusing and educating many of the people listed on this page. His impact on
us was immense & he is sadly missed.
The main objective of the ‘team’ is to better understand
the processes involved in the generation, migration and emplacement of all
melts & magmas. Our approach is multi-disciplinary, involving mathematical
modeling, geochemistry, geophysics, laboratory observation (textures &
microstructures), and fieldwork. Current field projects include ongoing study
of the Rum layered Intrusion (NW Scotland), the Bushveldt
layered Intrusion (
Fluid Flow &
Physical Properties of Rocks
Origin
& Evolution of Sedimentary Basins
Processes at Slow Spreading Ridges
Biographical
Information & who to contact: Dr. M.J. Cheadle
mailto:(cheadle@uwyo.edu)
Komatiites,
melting in mantle plumes; temperature constraints on the mantle through time
(Dr Mike Cheadle, Dr Kath Silva, Dr Dougal Jerram, with Prof. D.
Sparks – Texas A & M University, Prof. N.T. Arndt –Universite
Joseph Fourier Grenoble, Dr. Mary Gee & Prof.
E.G. Nisbet-RHBNC).
Komatiites are the hottest lavas ever
erupted on Earth (eruption temperatures 1400-1600oC), and therefore
they place important constraints on the temperature of the mantle especially
during the Archaean, where they are most commonly
found. However their origin remains enigmatic, mainly because of their age and
restricted occurrence & because of their preservation. We have studied the
petrology, geochemistry and origin of the freshest known komatiites
from the Belingwe Greenstone Belt in
Examples of
the well preserved Belingwe komatiites.
Spinifex
texture from the upper part of the flows on the left and the texture of the
cumulate zones from the lower part of the flows on the right.
The current ‘hot’ topic about komatiites
is ‘do they represent hot dry magmas or do they represent less hot, wet,
possibly subduction zone magmas’. Dr Mary Gee is
currently measuring water contents in melt inclusions from the Belingwe Komatiites using FTIR
methods. Initial results reveal very low water contents. If komatiites
are indeed ‘dry’ magmas, they must have formed in mantle plumes….. but the implications
for Archaean mantle temperatures are far ranging
(+200-300oC hotter than today).
Prof. Dave Sparks has developed 3-D numerical models of the
temperature distribution within mantle plumes. We use these models, along with
parameterisations of the temperature and pressure dependence of the chemistry
of mantle melts, to predict the composition of melts produced by different
mantle plumes. We’ve investigated the effects of varying mantle temperature,
the variation in lithosphere thickness, and are now attempting to introduce the
effect of water on melting. The work has been used to predict the mantle
conditions required for the generation of komatiites,
and has led to predictions of Archaean mantle
temperatures.
Numerical model
showing two isothermal surfaces (green & blue) which show the effects of
dragging a lithospheric plate over an up-welling
mantle plume. Box depth corresponds to the depth of the upper mantle.
Relevant Publications:
Arndt, N.T., Ginibre, C. Chauval, C., Albarede, F., Cheadle, M.J., Herzberg, C., Jenner, & Lahaye, Y., 1998. Were Komatiites Wet? Geology 26, 739-742.
Silva, K., Cheadle, M. J. & Nisbet E.G., 1997. The Origin of B-1 -zones in Komatiite Flows. Journal of Petrology, 38, 1565-1584.
Nisbet, E. G., Cheadle, M.J., Arndt, N.T., and Bickle, M.J. (1993). Constraining the potential temperature of the Archaean mantle: a review of the evidence from komatiites. Lithos. 30: 291-307.
Renner, R., Nisbet, E.G., Cheadle,M.J., Arndt, N.T., Bickle, M.,Cameron, W.E., 1993. Komatiite
flows from the Reliance Formation,
Nisbet, E.G., Arndt, N.T., Bickle,
M.J., Cameron, W.E., Chauvel, C., Cheadle, M.J., Hegner, E., Kyser,
T.K., Martin, A.,Renner, R.,
Roedder, E., 1987. Uniquely fresh 2.7 Ga old komatiites from the Belingwe greenstone belt,
The origin and
sequence stratigraphy of layered intrusions using
deep seismic reflection and geologic data
(Dr, Mike Cheadle,
Dr Fiona Sargeant, Dr Lisa Worrell, Caroline LoRe, with Prof. N. Arndt - Universite
Joseph Fourier Grenoble).
Layered igneous intrusions represent some of the most
spectacular igneous rocks seen on Earth (The Bushvedt
layered Intrusion of S. Africa may be 300 x 200 x 6 km in size!). They are
assumed to be the frozen remains of magma chambers, which once fed volcanoes
such as those found on
The four mountains (Barkeval,
Hallival, Askival & Trollaval) of the Eastern Layered Series, Rum.
Our group has spent many years understanding and logging the
rocks of the Tertiary Rum intrusion of N.W. Scotland. Rum has an ultramafic layered suite which is at least 1000 cubic
kilometres in volume. We’ve used a multi-disciplinary approach (including
mapping, logging, geophysical, geochemical, textural
& microstructural studies) to better understand
the origin of and the processes that go on within the intrusion. The
incontrovertible evidence for magmatic sedimentological processes has led us to use sequence stratigraphy to describe and interpret the intrusion. As a
test of our ideas, we are currently working on the much larger scale Bushveldt Intusion of
Our aim is to devise a sequence stratigraphic
framework for layered intrusions based on deep seismic data from the Bushveldt layered intrusion (
Photograph of
the typical igneous ‘layering’ seen in the Eastern Layered Series of the Rum
Layered Suite. The photograph shows troctolites (allivalites) and subsidiary peridotites
from Unit 14 on Hallival.
The schematic
on the right shows a postulated mechanism for the formation of the layering. It
attempts to show the importance of both in-situ crystal growth on the floor of
the chamber AND deposition of crystals by sedimentary processes.
Interpreted
seismic from the Bushveldt Layered Intrusion: the
ultimate way to do the sequence stratigraphy of
layered intrusions
Relevant Publications:
Upton, B.G.J., McClurg, J., Skovgaard, A.C., Kirstein, L., Cheadle, M., Emeleus, C.H., Wadsworth, W.J., and Fallick, A.E., 2002 Picritic magmas and the Rum ultramafic complex, Scotland. Geological Magazine, 139, 437-542.
Cheadle, M., Emeleus, H. & Jerram, D., 1999. The Geology of the Isle of Rum, IUGG fieldtrip guide, 55pp.
Cheadle, M.J., Curry, M. Emeleus, C.H. & Hunter R.H., 1997. Rumbustious! Earth Heritage, 8, 10-13.
Emeleus, C.H., Cheadle, M.J., Hunter, R.H.,
Bedard, J.H.,
The
quantification of rock textures and application of textural studies to the
understanding the origin of rocks
(Dr. Mike Cheadle, Caroline LoRe, Dr. Dougal Jerram, Dr. Lisa Worrell, Dr. John Wheeler (
There is much to be learned from textural
studies of rocks. This important avenue of research is often overlooked because
it may require lengthy periods of time acquiring data by microscope study. New
developments in computer aided image analysis and automated SEM study are now
making textural analysis an exciting area of research. We are both developing
new methods for analysing textures and are using existing methods to constrain
the processes that occur during the formation of rocks.
Dr Dougal Jerram has devised innovative cluster analysis techniques to quantify
the packing of grains in rocks. Packing is an often overlooked parameter
(unlike grain-size, etc.) which yields important information about how much
compaction a rock has undergone and how the grains in that rock accumulated. We
hope to use cluster analysis studies to quantify the degree of compaction in
rocks.
Illustration
of serial sections produced from a 3-D reconstruction of randomly packed sphere
data set from Finney (1970). The serial section make
it possible to 'walk' through the texture and inspect the distribution of pore
space and also 'random clusters of spheres'.
Dr. Lisa Worrell and Caroline LoRe
are using electron backscatter microscopy to map the crystallographic preferred
orientation (CPO) of crystals in rocks, to compare with the shape preferred
orientation (SPO) of those crystals. These fabric measurements provide
important information about how igneous cumulates form and the processes by
which they compact and solidify. They are studying rocks from both the Rum
& Bushveldt Intrusions and their results will
help confirm whether processes like current flow and/or compaction played a
role in the formation of the Rum cumulates.
We have recently obtained a state-of-the-art Electron BackScatter Diffraction (EBSD) system at the Department of
Geology and Geophysics as part of our Materials Characterization Lab. We will
use it to study the microstructure and crystallography of materials;
both of which fundamentally control the physical properties and reflects
both the crystallization and deformation history of the material. Consequently
the ability to efficiently acquire such information from rocks and other
materials is essential for geoscientists to fully understand how rocks
crystallize and deform. Electron Backscatter Diffraction (EBSD) microscopy
allows crystallographic data to be generated quickly and effectively within a microstructural framework. An EBSD system fitted to a
conventional Scanning Electron Microscope (SEM) with an automated stage can
measure crystal orientation directions in most types of polycrystalline
materials to the sub-micron level at speeds of up to 0.2s per spot analysis.
The equipment permits rapid determination of the absence or presence of
crystallographic preferred orientations (CPOs) within
a material, and provides statistical data describing the crystal misorientation distribution (MOD) of a material. It also
permits 3-D crystallographic, grain-size or texture mapping and phase
identification and indexing of the facets or cleavage planes of individual
crystals.
The pictures
to the left shows a small section of a pyroxene gabbro
from the
And to the
right is a grain map collected totally automatically using the EBSD system.
Pole figures determined
using the EBSD system for the plagioclase crystals in the rock.
The system
allows the very efficient determination of crystal fabrics in rocks.
Magma
generation, migration and crystallisation, including 3-D numerical models of crystallising
media.
(Dr. Mike Cheadle,
Dr. Mike Elliott).
The group has concentrated on
developing numerical models to mimic the 3-D crystallisation of materials. We
have previously developed 3-D models of texturally equilibrated materials and,
recently, Dr Mike Elliott has developed 3-D numerical models of non-equilibrated
crystallising media. Both single and multiphase systems consisting of different
grain shapes and sizes can be modelled. The computer programs can generate 3-D
images and 2-D slices through both texturally equilibrated and un-equilibrated
materials. These models give insights into the way rocks crystallise and can be
used to test our traditional models of crystallisation. They also permit
calculation of the evolving permeability of a crystallising system and hence
are fundamental to understanding magma generation and migration. One
interesting result is that crystal shape has an extremely important effect on
permeability at porosities of less than 10%.
The pictures
above show the results of the 3-D crystallisation model. The figure on the left
shows a completely crystallised cube of crystals and the lower picture shows
the zoning within those crystals. The figure on the right shows the results of
partially crystallising a cube. The upper figure shows the crystals and the
lower figure the pore space between the crystals.
One of the applications of this work is to test
the validity of dihedral angle measurements on 2-D sections. Here we show that
measurements of the 2-D dihedral angle distribution of pores in a totally
un-equilibrated rock (squares) are very similar to those measured for quartz + H20 &
olivine and H20.
Relevant Publications:
Jerram, D.A. & Cheadle, M.J., 2000. On the cluster analysis of grains and crystals in rocks. American Mineralogist, 85, 47-67.
Prior, D.J., Boyle, A.P., Brenker, F., Cheadle, M.J., Day, A., Lopez, G., Potts, G.J., Reddy, S.M., Spiess, R., Trimby, P.W., Wheeler, J., & Zetterström, L., 1999. The application of Electron Backscatter Diffraction and Orientation Contrast Imaging in the SEM to textural problems in rocks. American Mineralogist 84, 1741-1759
Elliott, M.T., Cheadle, M.J., & Jerram D.A., 1997. On the Identification of Textural Equilibrium in Rocks using Dihedral Angle Measurements. Geology, 25, 355-358
Elliott, M.T. & Cheadle, M.J., 1997. On the Identification of Textural Equilibrium in Rocks using Dihedral Angle Measurements, Reply. Geology, 25, 1055.
Hunter, R.H., 1996, Texture Development in Cumulate Rocks In Layered Intrusions. Ed. R.G. Cawthorn, Elsevier, 77-101.
Bryon, D.N., Atherton, M.P., Cheadle, M.J. & Hunter, R.H., 1996. Melt movement and the occlusion of porosity in crystallising granitic systems, Mineralogical Magazine, 60, 163-171.
Jerram, D.A., Cheadle, M.J., Hunter, R.H. & Elliott, M.T., 1996. The Spatial Distribution of Grains & Crystals in rocks. Contributions to Mineralogy & Petrology, 125, 60-74.
Hunter, R.H.,
1987, Textural equilibrium in layered igneous rocks:
The physical
properties of two-phase systems, and fluid flow in porous media
(Dr. Mike Cheadle,
Dr. Mike Elliott, Heather Sheldon, Dr John Wheeler (
The models mentioned above allow predictions of the evolving
physical properties (seismic velocity, electrical conductivity and
permeability) of fluid bearing media. Knowledge of these properties is
essential to interpret the results of geophysical investigations of magma
chambers (for example beneath mid-ocean-ridges). The result that crystal shape
is important at low porosities has important implications for the volumes of
magma present in magma chambers. Heather Sheldon is currently writing code to
examine the effects of the physical and chemical
processes that occur on the crystal scale during fluid flow. We intend to
investigate the effect of the complicated feedback between precipitation and
dissolution on permeability as a fluid in chemical dis-equilibrium
with the solid phase moves through its host rock.
Pore space
geometries of perfectly texturally equilibrated materials (the figure on the
left has a dihedral angle of 1o and a very low porosity, the one in
the centre has a dihedral angle of 60o and the one on the right has
a dihedral angle of 180o
Animation showing the
occlusion of porosity.
Watch a portion of a rock crystallise!
The effect of the geometry of crystals on the electrical conductivity of rocks.
Relevant Publications:
Elliott, M.T., Cheadle, M.J., & Jerram D.A., 1997. On the Identification of Textural Equilibrium in Rocks using Dihedral Angle Measurements. Geology, 25, 355-358.
Bryon, D.N., Atherton, M.P., Cheadle, M.J. & Hunter, R.H., 1996. Melt movement and the occlusion of porosity in crystallising granitic systems, Mineralogical Magazine, 60, 163-171.
The generation
and migration of silicic magmas
(Dr. Mike Cheadle,
Dr Matt Jackson, Heather Sheldon, Dr. Mike Atherton (
Dr Matt Jackson produced numerical models for the generation
of silicic magmas by melting the lower crust. The
important result is that the process of melt generation and migration through a
thermal gradient naturally leads to the production of a large volume of a melt
which is chemically the low melt fraction of the lower crust. This result
implies that the tectonic ‘squeezing’ advocated by some, to explain the
generation of a large volume of a small melt fraction, is not necessary.
Heather Sheldon has devised a phase-diagram based numerical model, which
permits investigation of the effects of spatial variations in the initial
composition of the source rock. She shows that a compositionally layered source
rock may develop local pockets of melt, wherever there is an upward change to a
more refractory composition. This spatially complex distribution of melt and
solid is eventually smoothed out by the passing of a larger porosity wave, if
heating continues for long enough.
.
Relevant Publications:
Jackson, M.D., Cheadle, M.J. and Atherton M.P. 2003 Quantitative modeling of granitic melt
generation and segregation in the continental crust, In Press: Journal of
Geophysical Research
The
processes of crustal extension at continental
margins.
Amy Heath (co-supervised by Dr. Pat Shannon (UCD)& Prof. N.J. Kusznir) is
using seismic & bore-hole data to study the Rockall Trough (West of
Ireland). This basin is a prime example of a rift basin that shows evidence of
extensive crustal thinning, but little brittle
faulting. Amy is hoping to determine whether the continental crust ‘broke’
beneath the Rockall Trough.
Relevant Publications:
Nadin, P.A.,
Cheadle, M.J., S. McGeary, M. Warner and D.H. Matthews, 1987. Extensional structures on the western
Understanding
anomalous uplift and magmatism at the South West
Indian Ridge.
(Dr. Mike Cheadle,
Graham Baines, Dr. Barbara John, Professor Nick Kusznir
(
Graham Baines is investigating the processes and mechanisms
which cause anomalous uplift at inside-corner highs and along transverse ridges
adjacent to transform faults at the South West Indian Ridge. He is currently
studying Atlantis Bank, which is an anomalously uplifted core complex that
rises 3 km above sea-floor of the same age.
Flexural uplift due to detachment faulting cannot fully account for this
uplift. Multi-beam bathymetric data and
direct observations have revealed large moderately dipping transform-parallel
normal faults on the Eastern flank of Atlantis Bank. Flexural uplift following such faulting is
consistent with gravity data and accounts for ~1-2 km of anomalous uplift. This faulting may be linked to the contiguous
transverse ridge that extends to the South of Atlantis Bank. Similar transform-parallel faults are also
observed on the most uplifted core-complexes on the Mid-Atlantic Ridge. The coincidence of anomalously elevated
core-complexes and transverse ridges imply that the mechanism of uplift is the
same in both cases.
The
Shinkai6500 (JAMSTEC), which is the deepest going manned submersible.
We used the
Shinkai6500 and the Kaiko ROV (Jamstec)
on a previous cruise to dive to the bottom of the ocean and investigate the
tectonic and magmatic processes occurring there.
A view of the bottom and an anemone from the window of the
submarine.
Future research plans involve the continuation and
development of the projects listed above. In particular:
i)
The origin of Komatiites.
ii)
Studies of the magmatism of the British
margin of the
iii)
The origin of layered Intrusions, igneous cumulates and platinum
deposits, with future work including the Stillwater Complex, the Bushveld Intrusion & the Rum Intrusion.
iv)
Textural studies and better numerical modelling of the evolution
between texturally equilibrated and texturally un-equilibrated rocks. (What is
the real permeability of the mantle? How are melts extracted? And in different
environments {M.O.R’s & Subduction
zones}).
v)
Continuing research into the generation, migration, and
emplacement of granites.
vi)
Application of seismic stratigraphy to
understanding Igneous Intrusions.
vii)
Understanding oceanic core complexes: structure & flexure.
viii)
The origin of the
Dr. Mike Cheadle
mailto:(cheadle@uwyo.edu)
Current Graduate Students
Graham Baines mailto:gbaines@uwyo.edu
Caroline LoRe
mailto:clore@uwyo.edu
Heather
Sheldon mailto:sheldonh@liv.ac.uk
Graduate Students who’ve
graduated
Dr.
Dougal Jerram (Elf
Lectureship,
Dr. Matt Jackson (Lectureship,
Dr.
Mike Elliott (BP-Amoco) mailto:elliotmt@bp.com
Dr.
Amy Heath
Dr. Kath Silva (Shell)
Dr. Fiona Sargeant
Dr. Lisa Worrell (Merebrook
Environmental Engineering Consultants) mailto:lworrell@merebrook.co.uk
Personal
Details:
Current
Employment: Associate
Professor in Geophysics, University of
Current Address: Department of Geology & Geophysics,
Telephone: (307) 766 3206
E-mail: cheadle@uwyo.edu
Education & Qualifications:
Ph.D. Geophysics: “Properties of Texturally Equilibrated Two-Phase Aggregates”,
1989.
M.Sc.Geophysics: ‘The
deep crustal structure of the
1984. COCORP seismic reflection data”,
Last revised: Date