HISTORY OF STRATIGRAPHY AND THE AGE OF THE EARTH AT
THE END OF 18TH
CENTURY AND 19TH CENTURY
THE USE OF THE HISTORY
OF GEOLOGY TO TEACH PUPILS ABOUT GEOLOGICAL TIME
Abstract
Nobody can fail to be aware of the worldwide celebrations,
which accompanied the start of the year 2000. Why did this date generate so much interest?
Was it because of the Millennium Bug or was it the number 2000? It seems appropriate to
consider 1000 years and how long that really represents in geological terms. Geology is
the only science to deal in time as a currency. It is also the science which is least
taught in school. So it seems appropriate to examine the history of the geological column
how it was developed, by whom and where and how the perception of the age of the
Earth has changed with the centuries. This introduces students to the history of spatial
and temporal awareness through history and how scientists have changed their theories with
advancing knowledge, travel, fieldwork, and technological ideas. New ideas have arisen and
new terminology.
Introduction
Geology is one of the few sciences to study the fourth
dimension. It is also the science which is least taught in school. Therefore the lecture
starts by looking, literally, at how long geological time is i.e. the age of the earth. It
is difficult to understand the length of time involved and therefore use is made of
everyday analogies. Visual, audio and tactile senses are used to strengthen the awareness
of this difficult concept. Secondly, the geological stratigraphic column is used to
illustrate the history of how scientists debated the age of the earth and how that
relative timescale can be used to put an age on earth materials. This introduces students
to two concepts firstly the history of exploring geological time and secondly how human
perception of nature's time has changed through history, by highlighting that there is a
difference between age and time.
These topics will be further illustrated on the fieldtrip
to the volcano Mount Teide.
Geological
Time
There are 2 ways of looking at geological time - in a
relative way and in an absolute way. Members of the audience will be used to illustrate
this.
First interactive part
This will involve the audience.
- Ask the audience to note on a piece of paper the oldest
thing they own. Summarise this verbally.
- Two people who are obviously different in age, are chosen
and then the audience is asked to either write down why one is older or younger than the
other and then to discuss with the person next to them or to share this with the whole
audience. Ask the people first if they mind being guinea pigs!!
- Secondly, ask the audience to decide how they would actually
put figures to the age of the person. If possible, ask the 2 people how old they are or
when they were born. They probably will not know the hour of their birth. So assume 12.00
- noon. Then ask the audience to work out in years, days and then hours how old they are.
This brings in the concept of scale and relates directly to the hourglass or the alarm
clock ticking. At the end of the lecture, you will ask the audience to add one to the age
they have worked out.
Person 1 = age x 365(days in a year) + (difference in date
in month born from todays date) x 24 (hours in a day. You may need to add more if it
is not noon.) = a
Person 2 = age x 365 (days in a year) + (date in month
born) x 24 (hours in a day) = b
e.g. David is 25 and born on the 8th of the
month. Today is 1st of the month and it is 12.00. So David is 25 x 365 + 7 days
old x 24 for the hours = 219,168 hours old. This introduces the students to very large
numbers but they feel an ownership as they can relate to it. At the end of the lecture add
1.
During the 19th century, geologists could only
reconstruct a relative time scale. The actual age and duration since the Earths
birth in millions remained unknown until the dawn of the 20th century. Table 1 shows the main people involved in the story.
RELATIVE TIME
The geological column
The development of the chronostratigraphic scale or the
stratigraphic column is seen by some scientists as one of the most significant
achievements in geology. Its development started during the age of heroism within geology
end of the 18th century. It fulfills the prime goal in geology by
establishing the global standard for a timescale in which to put earth materials. Most of
the divisions was developed over a period of 50 years in the first part of the 19th
century (See Fig. 1). Most of the systems were established
from the study of the stratigraphic record in Europe and were initially defined on the
lithology or rock types alone. An example of this is the Triassic divided into 3 parts by
Von Alberti in Germany in 1834. The development of the stratigraphic column was furthered
by Murchison who in 1835 defined his Silurian system using fossils as evidence. Perhaps
this helped Darwin further clarify his ideas. However it must be remembered that William
Smith, the canal surveyor, had already published his geological map of Britain in 1815 and
he had adopted a holistic approach based on all observations.
The stratigraphic column is now universally accepted across
the world and the names of the individual time units are shown in Table
2. The one exception to this is the Carboniferous first named in Britain after the
vast coal deposits found. However only the top half of this period contains coal. The
bottom part is composed of marine limestones and in recognition of this, the USGS in 1953
further subdivided the system into Mississippian and Pennsylvanian. However this
terminology is only widespread in America and not in Europe.
The chronostratigraphic scale is a summation of all
stratigraphical knowledge and as such there is no one cliff or quarry section on the Earth
at which all units are exposed. It forms the basis of all geological maps and correlation.
As it forms such an important part of geological study, the development of the stratigraphic column through the eighteenth and nineteenth
centuries follows the thinking and expansion of the geological perspective on the age of
the earth.
Within this history of geology lecture this will be
explored in 2 ways.
Firstly, in a relative way by exploring the idea of
comparative time using the 5 main principles employed within stratigraphy.
- Principle of Superposition
- Principle of Uniformitarianism
- Principle of Faunal succession
- Principle of Cross cutting relationships
- Principle of Inclusions.
Second to explore the history of the use of absolute time
within geology
The second area of study will be achieved using firstly the
debate about the age of the earth using Archbishop Usshers calculation and the bible
and secondly Lord Kelvin, the discovery of radioactivity and its application to the above
debate by Ernest Rutherford. From here the use and limitations of half lives in
radioactive elements will be explored.
The
Principles
The principles of stratigraphy are discussed using the main
scientists involved.
- Principle of superposition
Look at the work of Steno (1638 1687)
Steno was born in Copenhagen as Neils Steensen. He studied
medicine and anatomy there and in Paris. He traveled widely and eventually became the
court physician to Grand Duke Ferdinand II in Florence.
His observations were based on a comparison of modern and
fossil sharks teeth. He worked in the hills around Tuscany and was able to
appreciate that the sediments had been deposited in a primeval ocean.
He described his ideas on the relationships between strata
in De solido intra solidum naturaliter contento dissertationis prodromus (1669).
"At what time there was formed any bed, the matter
incumbent on it was all fluid and by consequence, when the lowest Bed was laid, none of
the upper Beds was extant.
When any Bed was formed, its inferior surface, and that of
its sides, did answer to the surfaces of the interior Body and of the Bodies lateral.
.Beds, either perpendicular to the Horizontal, or
inclined to it, have been at another time parallel to the same."
From these observations, we have the Principle of
Superposition, basically what lies on top is the youngest.

Figure 2.
What is the youngest deposit in this diagram?
- Principle of uniformitarianism
The work of James Hutton (1726 1797)
James Hutton was born in Edinburgh in Scotland where he
studied law and then chemistry and medicine at university, first in Edinburgh but later in
Paris and Leiden. He completed his studies in 1749. James Hutton never practiced medicine
but instead studied improved mixed farming techniques in Norfolk in England. Here new
scientific ideas on farming were developing following enclosure of the fields. First-hand
experience of crop rotation and improved road transport allowed Hutton to take his ideas
back to Berwickshire in Scotland and apply them to land he had inherited. It was from his
time in Norfolk that we can trace Huttons interest in rocks and minerals. His ideas
on geology developed and mushroomed after he moved to Edinburgh but this time spent in
Norfolk and Berwickshire is important in his developing and observing geological
structures and sections. He realised that the marine erosion he saw at work on the coasts
of England and Scotland and the intrusion of granite into other rocks demanded an
explanation and that the time taken for these processes to occur must be longer than the
6000 years accepted at that time as the age of the Earth. Hutton believed in observation
and then theory and explanation. His observations on Isle of Arran in 1787and at Siccar
Point (Fig.3.) in 1788, are known worldwide. He gave us the
axiom "The present is the key to the past".
From these observations he developed the idea of
unconformities (as shown in Fig. 3) which represented a vast
amount of time. The processes involved in their formation i.e. deposition, subsequent
uplift, folding and then erosion, subsidence and further deposition, must take time and
Hutton's observations showed him that 6000 years was just not long enough for this to
happen. As he himself says:-
"The purpose of this dissertation is to form some
estimate with regard to the time the globe of this Earth has existed, as a world
maintaining plants and animals
The solid parts of the present land appear , in
general, to have been composed of the productions of the sea
Hence we find reason to
conclude
.. 2dly. That , before the present land was made, there had
subsisted a world composed of sea and land, in which were tides and currents, with such
operations at the bottom of the sea as now take place. And.
Lastly That, while the present land was forming at the
bottom of the ocean, the former land maintained plants and animals, at least, the sea was
the inhabited by animals, in similar manner as it is at present."
Abstract of a Dissertation, 1785
"This earth, like the body of an animal is wasted at
the same time that it is repaired. It has a state of growth and augmentation; it has
another state, which is that of diminution and decay"
. "We find no vestige
of a beginning no prospect of an end"
Theory of the Earth, 1795.
Huttons ideas were being published at a time of
political unrest and controversies were feared. He also has a difficult writing style. His
"Theory of the Earth" ran to 1204 pages. 6 additional chapters were found a
century later. Both these facts led to his initial ideas being dismissed by many. As
Humphrey Davy (1805) states "Dr. Hutton is obscure and perplexed from the multitude
of facts which crowded on his mind." However, his long term friend, John Playfair
translated his ideas into readable English in 1802 as "Illustrations of the Huttonian
Theory" five years after his death.
To summarise, Huttons geology rests on the concept of
continuous natural processes working over periods of time that are infinitely long
compared with a human life span. Decay and erosion of the land produce the sediments and
running water moves it to the sea. The internal heat of the earth converts them from
sediments to rocks.
Figure 3, Siccar Point
- Principle of Faunal succession
The work of Baron Georges Cuvier (1769 1832) &
William Smith (1769 1839)
Baron Georges Cuvier was born in Montbeliard in 1769 in
what was at that time the Duchy of Wurttemberg to become Germany in the following century.
However following the French Revolution Montbeliard was annexed by the French and Cuvier
became French. He attended school in Stuttgart where he had a broad education and became
fluent in German. This was to stand him in good stead later when he moved to Paris as few
of his colleagues could speak both French and German. At that time French was the premier
language as English is today. This allowed him to be exposed to the scientific literature
of both those central European cultures.
Cuvier had always had an interest in natural history from a
boy and eventually after tutoring in Normandie, he managed to secure a job after the
Terror of the French Revolution, at the Museum National dHistoire Naturalle as a
junior assistant. This was to become his scientific and domestic home for the rest of his
life. Many publications on comparative anatomy of marine invertebrates and then mammals
followed. His work on the 3 species of elephants and the fact that mammoths were related
to none of them and were extinct caused a stir. He emphasized the importance of
comparative anatomy as a tool for establishing the theory of the Earth.
His empirical work on the alternation between freshwater
and marine fossils and sediments with Brongniart on the Paris basin and his rigorous and
painstaking analysis of these fossil shells led to his advocacy of catastrophic events to
explain geological phenomena. His assertion that he had discovered whole fauna of extinct
mammals which were distinct from living ones was his primary concern. The physical cause
of the processes, which led to this, were only of secondary importance to him. Cuvier
regarded catastrophies as part of the order of nature
and they had repeatedly occurred in the course of
Earths history. Hence we had a faunal succession.
Figure 4 Cuvier's example of an unconformity and faunal
succession

William Smith was styled by Sedgwick "The father of
English Geology"
William Smith was born in Churchill, Oxfordshire into
exactly the opposite type of family on the other side of the English Channel but in the
same year as Cuvier. He was the son of a village blacksmith who died when he was a young
boy. He had to support himself from an early age and was trained as a surveyor. At this
time canal, building was important in Britain and Smith was employed by companies in this
pursuit. He was a keen observer and realized that set faunas followed one another in
strict sequence. Eventually he became confident enough to predict rock types based on
their fossil content. He traveled widely with his work covering as much as 16,000km a
year, a huge distance in those days, mostly on horseback. Eventually he produced the first
geological "map of England and Wales with part of Scotland", in 1815. In 1819,
he published part of a work entitled Strata identified by organized fossils.
However William Smith never felt confident about his writing and never joined a scientific
society. His greatest contribution was his field observations and his synthesis into a
geological map.
These three principles apply to sedimentary strata. However
2 other principles are also used. They are the principles
of cross cutting relationships and principle of inclusions.
The Stratigraphic Column
Table 2
The first stratigraphic period to be recognised was the
Tertiary in 1760 by Arduino, a mining expert working in the Venetian Republic. He
distinguished 4 separate stages or orders one above the other. These were Primary,
Secondary, Tertiary and Quaternary, the Atesine Alps, the Alpine foothills, the sub-Alpine
foothills and the plains of the river Po respectively. The second, the Jurassic, a
well-recognised name nowadays, was named by Von Humboldt in 1795, the same year that James
Hutton published his "Theory of the Earth" in Scotland. This was based on the
work done in the Jura Mountains of France. While social revolution surpressed new
stratigraphic idea development in Europe, no new systems were acknowledged. Following the
Treaty of Versailles in 1815, relative time was debated again. In 1822 the Carboniferous
was recognised in Northern England by Conybeare and Phillips and at the same time the
Cretaceous in France by dHalloy. The majority of period names were then devised. The
last section of the stratigraphic column to be recognised was the Ordovician in 1879
following the lengthy debate or indeed argument between Sedgwick and Murchison in Wales.
Once the stratigraphic column was complete, type sections could be agreed and debated.
ABSOLUTE TIME
Introduction
Absolute time had to await the discovery of radioactivity
in 1896 by Antoine-Henri Becquerel and later the recognition that radium radiates heat
continuously by the Curies and Laborde in 1903. The suggestion by Lord Rutherford in 1903
that radioactive elements could be used to date rocks was revolutionary and Strutt
demonstrated that radioactive elements were widespread in minerals throughout rocks. In
1907, Bertram Borden Boltwood suggested that the rate of disintegration of uranium into
lead could be used to actually date rocks Thus the higher the percentage of lead in an ore
the older the rock.
With the new radiometric dating methods, geologists could
calibrate the relative scale of geological time thereby creating an absolute one. Arthur
Holmes was the first geologist to construct a time scale (1927), based on radiometric
dating and many time scales have been constructed since for the Cambrian upwards
(Phanerozoic Gk. Plainly evident life). It is being refined even to this day as more
isotopic data become available.
Radiometric
dating
Radiometric dating techniques were developed at the
beginning of the 20th century and use the regular rate of decay of unstable,
radioactive elements such as U-235, K-40, Rb-87 and C-14 to their daughter products either
in a single step or through a series of steps. These elements resemble virtual
"clocks" within the earths rocks and form the geologists
timekeepers. This decay is accompanied by the emission of radiation or particles (alpha,
beta or gamma rays) from the nucleus, by nuclear capture or by ejection of orbital
electrons. Thus heat is given off and this was an important point in the 1903 lecture by
Ernest Rutherford when debating the age of the Earth in the company of Lord Kelvin at the
Geological Society of London. If a daughter product is stable, it accumulates until the
parent isotope has completely decayed. If a daughter isotope is also radioactive,
equilibrium is reached when the daughter decays as fast as it formed.
The radioactivity of an element is described in terms of
half-life, the time the element takes to lose 50% of its activity by decay.
Diagram
This can cover a large scale of time from billions of years
to microseconds. At the end of the period constituting one half-life, half of what was
left is halved again, leaving one quarter of the original quantity and so on. Every
radioactive element has its own half-life e.g. C-14 is 5730 years.
Limitations
There are however some limitations in the use of
radiometric dating.
- The minerals making up the rocks must contain suitable
radioactive elements within their crystal lattices
- The rocks must be the correct age to start with for the
half-life available.
Thus it is useless trying to date a shell 1 million years
old with C-14 as there will be no C-14 left. Similarly, it is no good trying to date pure
sandstone composed only of Quartz, SiO2, using the U-235 method, as Quartz does
not normally contain uranium.
Conclusion
Perhaps one of the best known scientists in the world is
Charles Darwin. What is less well known is that he trained as a geologist. You will hear
about a little of his work from John Cartwright. The understanding of the development of
mans perception of time, both relative and absolute and the age of the earth have
helped us understand the context of our place on the planet on which we live.
Notes
As well as straight teaching/lecturing, the 2/3 interactive
parts to the lecture will be expanded within the workshops. It is hoped that 3 of the 5
principles will be illustrated in a fieldtrip up the volcano El Teide. However it is
possible to illustrate several principles in an urban setting using building stones for
example the principle of superposition.
BIBLIOGRAPHY
Blundell D.J. and Scott A.C., (1998) Lyell: the past is the
key to the present, Geological Society of London, ISBN 1862390185
Bowler P, (1992) The fontana history of the environmental
sciences, Fontana Press ISBN 0006861849
Craig G.Y. and Hull J.H., (1998), James Hutton - Present
and future, Geological Society of London, ISBN 1862390266
Dean D., (1992), James Hutton and the history of geology,
Cornell University Press, ISBN 0801426669
Hallam A., (1984), Great Geological controversies, Oxford
University Press, ISBN 0198544308
Hellman H., (1998), Great Feuds in science, Ten of the
liveliest disputes ever, John Wiley, ISBN 04714169803
Holland C.H., (1999), The idea of time, John Wiley, ISBN
0471985457
Oldroyd D., (1996), Thinking about the Earth: a history of
ideas in geology, Athlone Press, ISBN 0485114321
Playfair, J. (1805), Biographical account of the late Dr.
James Hutton, F.R.S. Edin., Transactions of the Royal Socieety of Edinburgh, V,
(III),39-99.
Rudwick M.J.S., (1997), Georges Cuvier, fossil bones and
geological catastrophes, University of Chicago Press, ISBN 0226731073
Workshop
The workshops will involve
- A loud ticking clock and a timer set for one hour
- Perhaps a sand hour glass if available
- a piece of string measured at various intervals to show
prominent earth events,
- 2 members of the audience (if not already done in the
lecture)
- a cartoon geological cross section
This has then introduced the audience to the 2 ways of
looking at geological time.
The last two principles will hopefully be illustrated in
the field at Mount Teide and in the workshop exercise.
- Principle of cross cutting relationships
- Principle of inclusions.
It will be possible to illustrate at least one of these on
the field excursion. It will be shown how these can be illustrated in an urban environment
using windows and doorways in a building.
Workshops
Activity 1
Length of string exercise
The string and significant dates can be varied depending on
the country in which this exercise is being done (e.g. Black Death). Obviously, the events
on the string could vary between Britain and for example Spain or Greece. Use a scale of 1
cm per 1000 years. This is significant as it will be the year 2001.
| Event
|
Years Ago |
| Today, |
0 |
| Birth of Jesus Christ, |
2,000 |
| Age of the Earth according
Archbishop Ussher |
6000 |
| End of Ice age in Northern Europe,
|
10,000 |
| Evidence of first Homo sapiens in
Europe, |
500,000 |
| Tenerife |
8,500,000 |
| Gran Canaria 1 |
3,500,000 |
| Extinction of dinosaurs |
65,000,000 |
| Age of the earth according to Lord
Kelvin (1846) |
100,000,000 |
| Age of the earth according to Lord
Kelvin (1866) |
20-400,000,000 First |
| appearance in fossil record of
multicellular algae |
2,100,000,000 |
| Oldest rock on earth |
3,800,000,000 |
| Birth of Earth |
~ 4,600,000,000 |
Activity 2
Bible exercise
Natural scientists were interested throughout the 16th,
17th centuries to know the age of the earth and many calculations were
produced. However in 1658 Archbishop Ussher came up with a date which the whole of the
Christian world seemed to initially accept. How did Archbishop Ussher of Armagh come up
with 09.00 26th October 4004BC in 1658?
An analysis of the first book of the Old Testament seems
the obvious place to start. The beginning of Genesis details the creation and then goes on
to list in detail Adam and his decendants. Students will try to calculate how many years
are accounted for in the Old Testament of the bible.
A discussion will then take place as to why there might be
a discrepancy both between student group addition! And Archbishop Ussher's calculation.
What else could scientists of that time be concerned about and where do the errors arise.
Activity 3
Cartoon cross section exercise. What happened first?
| Work out the geological sequence of the section and decide
which principles could have been used at the following dates |
| 1000AD |
| 1500AD |
| 1832AD |
Table 1 List of principle players on
the stage
| Name |
Dates |
Nationality/place
of work |
| Leonardo di Vinci |
1452-1519 |
Italian/Apennines, N. Italy |
| Archbishop James Ussher |
1581-1656 |
Irish, age of the earth (bible) |
| Robert Hooke |
1635-1703 |
English/Faunal succession hints |
| Nicholaus (Neils) Steno |
1638-1687 |
Dane/Italy |
| G. Arduino |
1714-1795 |
Italian/Venice |
| James Hutton |
1726-1797 |
Scottish/Scotland |
| Alexander von Humboldt |
1769-1859 |
German |
| Georges Cuvier |
1769-1832 |
French/Paris basin |
| William Smith |
1769-1839 |
English/England |
| William Buckland |
1784-1846 |
English |
| Adam Sedgwick |
1785-1873 |
English/ England & North Wales |
| Roderick Murchison |
1792-1871 |
English/ South Wales |
| Charles Lyell |
1797-1875 |
Scottish/England |
| Lord Kelvin (William Thomson) |
1824-1907 |
Scottish |
| Archibald Geike |
1835-1924 |
Scottish/Scotland |
| Charles Lapworth |
1842-1920 |
English/Mid Wales |
| Pierre Curie |
1859-1906 |
French/Paris |
| (Lord Rayleigh) Ernest Rutherford |
1871-1937 |
English |
| Arthur Holmes |
1890-1965 |
English |
| James Croll |
1921-1990 |
Scottish/Scotland |
Table 2 STRATAGRAPHIC COLUMN
| 1970Neogene Quaternary |
Néogène: Quaternaire |
Neogeno: Cuaternario |
1829 Desnoyers; 1833 Reboul (redefined) |
| Pleistocene |
Pleistocéne |
Pleisteceno |
1833 Charles Lyell |
| Pliocene |
Pliocéne |
Plioceno |
1833 Charles Lyell |
| Miocene |
Miocéne |
Mioceno |
1833 Charles Lyell |
---------- |
---------- |
---------- |
|
| 1970 Paleogene Oligocene |
Paléogène Oligocéne |
Paleogen: Oligoceno |
1854 H. Von Beyrich |
| Eocene |
Eocéne |
Eoceno |
1833 Charles Lyell |
| Palaeocene |
Palaeocéne |
Paleoceno |
1874 W.P.Schimper |
---------- |
---------- |
---------- |
|
| Cretaceous |
Crétacé |
Cretàcico |
1822 Omalius d'Holloy |
| Jurassic |
Jurassique |
Juràsico |
1795 Alexander von Humboldt. |
| Triassic |
Trias |
Triàsico |
1834 F. Von Alberti |
---------- |
---------- |
---------- |
|
| Permian |
Permien |
Pérmico |
1841 Murchison |
| Carboniferous (Pennsylvanian Mississippian) |
Carbonifére |
Carbonifero |
1822 British consensus 1953 US division |
| Devonian |
Devonien |
Devonico |
1840 Murchison & Sedgewick |
| Silurian |
Silurien |
Silurico |
1835 Sedgewick & Murchison 1839 Global recognition Murchison |
| Ordovician |
Ordovicien |
Ordovicico |
1902 Charles Lapworth |
| Cambrian |
Cambrien |
Càmbrico |
1835 Sedgewick & Murchison |
---------- |
---------- |
---------- |
|
| Precambrian |
Precambrien |
Precàmbrico |
|
|