Humberside Geologist No. 14

Humberside Geologist Online

The Geochemistry of the Red Clays of Holderness and their origin.

 by Caroline Memczak,
Jo Burns, Lauren Knowles, 
Steve Martin and Louise Southern,
with a contribution by Mike Horne.

Extra data is available on the CD-ROM of Humberside Geologist number 14.

Abstract.

This research was carried out as a forensic science undergraduate project at the University of Hull, Department of Chemistry. Samples of red clay (with no gravel or pebble content) and red boulder clay from the coast of Holderness were compared with clays of known geological age and origin. The techniques used included ICP analysis, SEM analysis, acid carbonate testing, microscopy and particle sizing. The red boulder clays showed similarities with a weathered boulder clay. The red clays showed similarities with unweathered boulder clay. They showed no affinity to the Red Chalk or Mercia Mudstone.

Introduction

This project was trying to ascertain if it was possible to prove conclusively whether one or more rocks came from the same source by using currently existing analytical methods and instruments. To answer this question several different samples of red clays were selected for use in this experiment.

Geological background

The Boulder Clays (or Tills) of Holderness were deposited by the Ice Ages of the late Quaternary by glaciers that had travelled from the Lake District, Scotland, Northern England and Scandinavia. We have evidence for this from the erratic rocks and fossils that can now be found in Holderness (Horne & Harrison 1992, Horne 2000, Rockett 1992).

Thin layers of red and grey clay and soft chalk can be seen between the layers of the Tills in the cliffs of Holderness or occasionally as beach exposures (Bisat in Catt and Madgett 1981, Fenton 1977). The chalk in these 'rafts' is younger that the chalk exposed in East Yorkshire, and has probably been picked up by the glaciers as they moved across the bed of the North Sea (Horne, ongoing research). The grey clays seem to be of Late Jurassic age, from evidence collected by Stuart Jones and Chris Brogden. But what is the origin of the bands of red clay and red boulder clay? There are several possibilities :-

The samples.

Samples of red clay from a beach exposure at Aldbrough, East Yorkshire [sample numbers ALD2005-3, ALD2005-5, ALD2005-VR] and Red Boulder Clay from the "Red Band" in the boulder clay cliffs at Aldbrough [ALD2005-2] , Hornsea [HORNRBC] and Mappleton [MAP2005] were collected by Anne Horne, Mike Horne and Gordon Ostler in 2005. These were compared with other samples of red clays and boulder clay.
 
Sample number
Geographical Location
Geological Age
Description
ALD-2005-2 Aldbrough (NGR TA260392 ) Pleistocene Red boulder clay
ALD-2005-3 Aldbrough(NGR TA260392 ) Pleistocene Red clay
ALD-2005-5 Aldbrough(NGR TA260392 ) Pleistocene Red laminated clay
ALD-2005-VR Aldbrough(NGR TA260392 ) Pleistocene Very red clay
BOOKBARN Book Barn, Hallowtrow, Somerset. (NGR ST6356 ) Triassic Red clay - Mercia Mudstone Group
HOLMEOSM Church Hill, Holme-On-Spalding-Moor. (NGR SE819388) Holocene Red Soil - ?derived from Mercia Mudstone Formation or an early glaciation.
HORNBC Hornsea (NGR TA2118446941 ) Pleistocene Boulder Clay (unweathered)
HORNRBC Hornsea(NGR TA2118446941 ) Pleistocene Red Boulder Clay
HORNWBC Hornsea(NGR TA2127746629 ) Quaternary  Weathered Boulder Clay
MAP2005 Mappleton(NGR TA230434 ) Pleistocene Red boulder clay
SE452766 Sugar Loaf Bay, Portishead, Somerset. (NGR SE452766)  Devonian Red clay from the Old Red Sandstone.
SPEETON Speeton (NGR TA153755 ) Albian, Cretaceous Red marl from Red Chalk Formation.
 

Most of the samples were collected from coastal locations, except SE452766, HOLMEOSM and BOOKBARN.

Techniques used -

[safety note - the specialist chemical techniques were carried out in a science laboratory and for safety reasons should not be repeated at home!]

ICP

Inductively Coupled Plasma- Optical Emission Spectrometry (ICP-OES) is a solution based technique for elemental analysis. An ICP is a very high temperature (7000-8000 K) excitation source that efficiently desolvates, vaporises, excites and ionises atoms.

The most essential step in analysis is the sample preparation; as unless appropriate sampling schemes and suitable procedures are used to prepare samples any subsequent analysis will be wasted. The sample needs to be ground up to give a small particle size and then dissolved in acid. A weak acid is generally referred to as a leach and while it may result in a quantitative extraction of the elements of interest, most of the sample will remain undissolved. Strong acid attacks are generally referred to as digestions and these are more powerful than leaches. For the experiment carried out in this project, aqua regia digestion was used. Aqua regia is a 3:1 mixture of hydrochloric and nitric acids. Nitric acid destroys organic matter and oxidises sulphide material. It reacts with concentrated hydrochloric acid to generate aqua regia according to the equation:-

 3HCl + HNO3 ==> 2H2O + NOCl + Cl2

Aqua regia is an effective solvent for most base metal sulphates, sulphides, oxides and carbonates but only provides a partial digestion for most rock forming elements. This acid digestion is greatly speeded up when combined with microwave digestion. This prepares samples at high temperature in closed vessels and allows smaller quantities of acid to be used. It also ensures that certain inorganic compounds that are quite resistant to acid attack are digested. The digested sample can then finally be diluted and analysed. This analysis could then give detailed information on the chemical composition of the samples.

An aqua regia solution (100 ml) was made by mixing concentrated hydrochloric acid (75 ml) and concentrated nitric acid (25 ml). The solution was left to stand overnight in a fume cupboard to allow the chlorine gas to escape and the bright orange colour to develop. Each sample (0.3 g) was added to the digestion containers and aqua regia solution (5ml) added before the containers were loaded into the microwave digestion machine. This digestion was carried out at 80 p.s.i. for 10 minutes and then the samples left to cool. The samples were removed and added to a 25 ml conical flask ensuring thorough rinsing of the containers and then the flasks made up to the mark with water. These samples were diluted further by taking 1ml of sample and adding it to a 10 ml conical flask and made up to the mark with 2% HNO3. The samples could then finally be analysed using the ICP-OES instrument.

Scanning Electron Microscopy

SEM analysis involves directing a beam of electrons at the sample. Electrons are emitted from the sample and collected by a detector which converts them into a small electric signal. This signal contains a variety of information about a single point on the sample surface. To form an image of the sample a large number of points over an area need to be analysed, and the final image is built up from the number of electrons emitted from each point. To enable all of this to occur, samples need to be prepared carefully to withstand the vacuum inside the microscope but they also need to be made conductive. This is achieved by sputtering or vacuum evaporation to put a thin carbon or metallic coating onto the sample.

Scanning electron microscopes are often coupled with x-ray analysers. This is because x-rays are produced whenever an electron beam interacts with matter and these can be used very effectively to give information about the chemical compositions of the sample. Energy Dispersive X-ray micro analysers (EDX) are the most commonly used as these can detect almost all elements simultaneously and these elements are identified from their characteristic energies and their concentration can be derived from the count rate. This chemical composition is achieved using bulk analysis rather than spot analysis. This is because bulk analysis gives an area analysis and so the best overview of the sample, whereas spot analysis is best used for analysing a specific grain.

The sample pellets were produced by the method and equipment normally used to make K Br discs for Infra-red analysis. The powdered samples and pellets were then sent for analysis. The analyses represent an average of five spot samples.

Acid Carbonate Testing

A recorded amount (about 25g) of each of the powdered rock samples was taken and mixed with a small amount of de-ionised water and then dilute hydrochloric slowly was added. Once the samples had stopped fizzing more acid was added until the reaction with the samples was complete. The samples were filtered to remove the liquid and the remaining solids transferred to filter paper and dried. After thorough drying the samples could be re-weighed and the carbonate content calculated. The acid reacts with the calcium carbonate in the rock samples and hence the weight of the rocks, once the acid has been filtered off, decreases providing an indication of the amount of carbonate in each of the samples.

Particle Sizing

For this analysis the samples were first boiled in water with a de-flocculating agent to break the rock down into a slurry. This slurry was put through a set of sieves to filter out the minerals and bits of rock in the sample, and this allowed all the silt and clay to be removed. The set of sieves used had the following mesh sizes: 63um, 250um, 500um and 1mm.

Optical Microscopy

Once the particle sizing had been carried out microscopic analysis of the fractions could be done to see what grains, and possibly minerals were present. This part of the research used the particle-sized samples: a selection of the samples from the 500 um -1mm and 250 um -500 um particle size ranges were looked at under a microscope. The different types of particulates seen were categorised and counted. About 200-300 particulates were counted for each sample; this was to ensure that the results obtained gave a true representation of what each sample contained.

 

Results and discussion -

ICP analysis -

ICP analysis provided the best results of the project in terms of answering the question of whether the samples could be matched to one another. Although it could not provide a definite answer that two samples were identical, it did show there were two groups of similar compositions, and one group with significantly different compositions to the rest. 

Sample Name
% of Al 
% of Ba
% of Ca
% of Cd
% of Cu
% of K
% of Mg
BOOKBARN
1.131
0.033
0.347
0.002
0.001
0.403
0.402
ALD-2005-5
1.062
0.011
5.072
0.001
0.001
0.223
0.823
HOLMEOSM
2.778
0.011
6.388
0.001
0.001
0.934
4.075
SE452766
1.607
0.012
3.965
0.001
0.002
0.37
2.96
ALD-2005-2
1.565
0.016
3.611
0.001
0.002
0.331
1.044
SPEETON
2.008
0.007
16.757
0.001
0.002
0.507
0.467
ALD-2005-3
1.803
0.014
6.889
0.001
0.001
0.416
1.182
HORNWBC
1.497
0.011
3.894
0.001
0.002
0.341
1.048
MAP2005
1.4
0.015
2.831
0.001
0.001
0.303
1.022
ALD-2005-VR
1.9
0.014
6.951
0.001
0.002
0.452
1.108
HORNRBC
1.754
0.015
2.17
0.001
0.002
0.402
1.146
HORNBC
1.716
0.013
5.014
0.001
0.001
0.424
0.978
   
Sample Name
% of Mn
% of Na
% of Ni
% of Pb
% of S
% of Si
BOOKBARN
0.115
0.005
0.002
0.001
0.01
0.209
ALD-2005-5
0.044
0.265
0.003
0.001
0.204
0.152
HOLMEOSM
0.079
0.028
0.005
0.001
0.024
0.198
SE452766
0.106
0.113
0.004
0.002
0.074
0.261
ALD-2005-2
0.061
0.388
0.004
0.001
0.112
0.32
SPEETON
0.127
0.12
0.007
0.001
0.016
0.133
ALD-2005-3
0.063
0.238
0.004
0.001
0.208
0.18
HORNWBC
0.046
0.087
0.003
0.001
0.421
0.179
MAP2005
0.051
0.17
0.004
0.001
0.117
0.173
ALD-2005-VR
0.059
0.252
0.004
0.001
0.157
0.319
HORNRBC
0.047
0.102
0.004
0.003
0.109
0.156
HORNBC
0.044
0.176
0.003
0.001
0.29
0.19
   
Sample Name
% of Sr
% of Fe
% of P
% of Ti
% of V
% of Zn
BOOKBARN
0.026
3.522
0.135
0.049
0.003
0.005
ALD-2005-5
0.029
2.215
0.218
0.017
0.003
0.006
HOLMEOSM
0.026
3.325
0.281
0.026
0.003
0.007
SE452766
0.027
3.448
0.261
0.019
0.002
0.02
ALD-2005-2
0.03
3.092
0.233
0.023
0.007
0.007
SPEETON
0.054
2.597
0.499
0.026
0.005
0.006
ALD-2005-3
0.037
3.033
0.248
0.026
0.004
0.007
HORNWBC
0.029
3.103
0.234
0.019
0.004
0.007
MAP2005
0.032
3.19
0.241
0.021
0.003
0.008
ALD-2005-VR
0.041
3.18
0.259
0.025
0.004
0.007
HORNRBC
0.027
3.191
0.228
0.026
0.003
0.007
HORNBC
0.031
2.69
0.22
0.03
0.004
0.006
 These results show that the rocks can be divided into three groups:-

Group A

BOOKBARN, SPEETON, SE452766 and HOLMEOSM.

BOOKBARN and SPEETON are very obviously different to the other samples. BOOKBARN contains a very large amount of iron whilst SPEETON is mostly made up of calcium. SE452766 and HOLMEOSM have elemental compositions that are very similar but are from opposite ends of the country, with SE452766 originating from Somerset and HOLMEOSM from Yorkshire. Therefore these two samples are unlikely to have originated from the same source even though they are elementally similar.

Group B

HORNBC, ALD-2005-5, ALD-2005-3 and ALD-2005-VR.

All of these samples have virtually the same elemental composition. They contain about 5% calcium and have a significant amount of iron in them. HORNBC was essentially used as a standard as it was known to be a boulder clay. Therefore the conclusion can be drawn that the other three samples in the group are most probably also boulder clays and originate from the same area/source.

Group C

HORNWBC, ALD-2005-2, MAP2005and HORNRBC.

These four rocks are compositionally similar; they contain roughly an equal ratio of iron and calcium. HORNWBC is known to be a weathered boulder clay and in comparison to HORNBC (boulder clay) has less calcium but more iron present. This could show that the weathering slightly alters the percentage elemental composition of rocks. Hence, HORNRBC, ALD-2005-2 and MAP2005could originate from the same area/source as HORNWBC or it could just be rocks that have undergone a similar weathering process.

Although these differences cannot be explained in terms of locations, it does provide evidence that samples have similarities in their various compositions. It may also be an indicator that they possibly originate from the same areas before the glacial movements of the Ice Age.

 SEM Analysis -

Morphological information

Scanning Electron Microscopy (SEM) provided images of the powdered samples at a micrometre size, as well as a basic elemental composition of the sample. Pictures of all 12 of the samples were taken using the scanning electron microscope; each sample was photographed at three different magnifications.

The morphological information is seen the SEM pictures. These were taken at three different magnifications for each sample. To obtain the pictures a smooth surface needs to be achieved which is done by grinding the sample into a fine powder. Unfortunately this destroys some of the surface characteristics and so an accurate comparison of the samples cannot be carried out. It is also difficult to carry out a comparison due to the samples all being quite similar and there being no characteristic features such as fossils being present.

Compositional information

Using an X-ray detector, an elemental breakdown on the samples was also possible using the SEM apparatus. The compositional data was obtained by randomly analysing five spots on the sample and then taking an average of the results. The results of this are summarised in the tables below:

Raw Data
 
Sample
Na
Mg
Al
Si
S
Cl
K
Ca
Ti
Fe
O
SPEETON
0.41
1.05
9.19
19.8
0.05
0.59
2.26
18.4
0.43
6.25
41.54
SE452766
0.24
3.26
10.22
25.68
0.15
0.9
4.64
2.71
0.5
6.63
45.07
MAP2005
0.72
1.77
10.72
26.87
0.11
0.22
3.42
2.9
0.64
6.69
45.93
HORNWBC
0.45
1.77
12.71
25.08
0.3
0.1
3.07
4.14
0.54
5.88
45.97
HORNRBC
0.48
1.78
12.68
25.7
0.28
0.86
3.09
2.23
0.62
6.24
46.04
HOLMEOSM
0.31
5.46
8.97
23.65
0.05
0.04
3.92
6.59
0.48
6.27
44.25
BOOKBARN
0.2
1.2
9.02
28.92
0.05
0.01
5.87
0.52
0.55
7.76
45.9
ALD-2005-VR
0.81
1.59
10.22
24.51
0.14
0.5
3.19
7.9
0.52
6.15
44.47
ALD-2005-5
0.78
1.51
9.36
26.06
0.21
0.56
2.93
7.49
0.6
5.38
45.12
ALD-2005-3
0.75
1.53
9.43
25.19
0.18
0.4
2.96
8.72
0.55
5.6
44.69
ALD-2005-2
0.94
1.73
10.51
25.99
0.07
0.53
3.67
3.79
0.55
7.05
45.17
HORNBC
0.63
1.59
10.99
24.11
0.46
0.93
2.8
7.4
0.5
5.86
44.73
Percentages without oxygen and silicon:-
 
Sample 
Na 
Mg 
Al 
 
Cl
Ca 
Ti 
Fe 
SPEETON 
1.06053 
2.71599 
23.77134 
0.12933 
1.52613 
5.84584 
47.67201 
1.11226 
16.16658 
SE452766 
0.82051 
11.1453
34.94017 
0.51282 
3.07692 
15.86325 
9.26496 
1.70940 
22.66667 
MAP2005
2.64803 
6.50975 
39.42626 
0.40456 
0.80912 
12.57815 
10.66569 
2.35381 
24.60463 
HORNWBC 
1.55387 
6.11188 
43.88812 
1.03591 
0.34530 
10.60083 
14.29558 
1.86464 
20.30387 
HORNRBC 
1.69851 
6.29866 
44.86907 
0.99080 
3.04317 
10.93418 
7.89101 
2.19391 
22.08068 
HOLMEOSM 
0.96603 
17.0146 
27.95263 
0.15581 
0.12465 
12.21564 
20.53599 
1.49579 
19.53880 
BOOKBARN 
0.79428 
4.76569 
35.82208 
0.19857 
0.03971 
23.31215 
2.06513 
2.18427 
30.81811 
ALD-2005-VR 
2.61122 
5.12573 
32.94649 
0.45132 
1.61186 
10.28369 
25.46744 
1.67634 
19.82592 
ALD-2005-5 
2.70645 
5.23942 
32.47745 
0.72866 
1.94310 
10.16655