The Scientists

A History of Science Told Through the Lives of Its Greatest Inventors

Illustrated by Adam Hook
Look inside
In this new and landmark history of modern science, author and trained astrophysicist John Gribbin recounts the development of science over the past five-hundred years—as seen specifically through the lives and achievements of individual scientists.

John Gribbin has written extensively before on scientific subjects such as the theory of everything, the existence of reality, and Schrödinger's cat. However, in The Scientists, he shifts his focus to the people who have conceived and produced modern science's theories, inventions, and innovations. He examines the times in which these scientists lived and worked and how their particular contributions influenced the overall development and direction of scientific inquiry. In the process, Gribbin not only re-evaluates the significance of such venerable icons as Galileo, Isaac Newton, Albert Einstein and Linus Pauling, but he also examines lesser lights whose stories have been undeservedly neglected.

Invaluable for those studying the history of science, and useful for those considering the impact of science on stages of history from the Renaissance and up to the present-day, The Scientists is ultimately a completely original, expansive, and nuanced survey of the most important scientific figures of the past half-millennium.

"Well written and scholarly, it is still accessible....[Gribbin] also clearly understands the important role that technology played in making science's greatest discoveries possible....Highly recommended for public and academic libraries or as a text for the history of science."
Library Journal

"As expansive (and as massive) as a textbook...explores the development of modern science through the individual stories of philosophers and scientists both renowned and overlooked."
Publishers Weekly

"Admirably ambitious in scope.... Highly recommended." M. Schiff, CUNY College of Staten Island for Choice Magazine (American Library Association)

“Essential reading...tells the story of science as a sequence of witty, information-packed tales...complete with humanizing asides, glimpses of the scientist’s personal life and amusing anecdotes.”
London Sunday Times, Books of the Year


TABLE OF CONTENTS
List of Illustrations
xi
Acknowledgements xv
Introduction xvii

Book One: OUT OF THE DARK AGES

1. Renaissance Men
Emerging from the dark — The elegance of Copernicus — The Earth moves! — The
orbits of the planets — Leonard Digges and the telescope — Thomas Digges and the
infinite Universe — Bruno: a martyr for science? — Copernican model banned by
Catholic Church — Vesalius: surgeon, dissector and grave-robber — Fallopio and
Fabricius — William Harvey and the circulation of the blood

2. The Last Mystics
The movement of the planets — Tycho Brahe — Measuring star positions — Tycho’s
supernova — Tycho observes comet — His model of the Universe — Johannes Kepler:
Tycho’s assistant and inheritor — Kepler’s geometrical model of the Universe — New
thoughts on the motion of planets: Kepler’s first and second laws — Kepler’s third
law — Publication of the Rudolphine star tables — Kepler’s death

3. The First Scientists
William Gilbert and magnetism — Galileo on the pendulum, gravity and
acceleration — His invention of the ‘compass’ — His supernova studies —
Lippershey’s reinvention of the telescope — Galileo’s developments thereon —
Copernican ideas of Galileo judged heretical — Galileo publishes
Dialogue on the
Two Chief World Systems — Threatened with torture, he recants — Galileo
publishes
Two New Sciences — His death

Book Two: THE FOUNDING FATHERS
4. Science Finds its Feet 107
Rene´ Descartes and Cartesian co-ordinates — His greatest works — Pierre Gassendi:
atoms and molecules — Descartes’s rejection of the concept of a vacuum —
Christiaan Huygens: his work on optics and the wave theory of light — Robert Boyle:
his study of gas pressure — Boyle’s scientific approach to alchemy — Marcello
Malpighi and the circulation of the blood — Giovanni Borelli and Edward Tyson: the
increasing perception of animal (and man) as machine.

5. The ‘Newtonian Revolution’ 149
Robert Hooke: the study of microscopy and the publication of Micrographia —
Hooke’s study of the wave theory of light — Hooke’s law of elasticity — John
Flamsteed and Edmond Halley: cataloguing stars by telescope — Newton’s early life
— The development of calculus — The wrangling of Hooke and Newton — Newton’s
Principia Mathematica: the inverse square law and the three laws of motion —
Newton’s later life — Hooke’s death and the publication of Newton’s
Opticks

6. Expanding Horizons 193
Edmond Halley — Transits of Venus — The effort to calculate the size of an atom —
Halley travels to sea to study terrestrial magnetism — Predicts return of comet —
Proves that stars move independently — Death of Halley — John Ray and Francis
Willughby: the first-hand study of flora and fauna — Carl Linnaeus and the naming
of species — The Comte de Buffon:
Histoire Naturelle and thoughts on the age of
the Earth — Further thoughts on the age of the Earth: Jean Fourier and Fourier
analysis — Georges Couvier: Lectures in Comparative Anatomy; speculations on
extinction — Jean-Baptiste Lamarck: thoughts on evolution

Book Three:T HE ENLIGHTENMENT
7. Enlightened Science I:Chemistry catches up 241
The Enlightenment — Joseph Black and the discovery of carbon dioxide — Black on
temperature — The steam engine: Thomas Newcomen, James Watt and the
Industrial Revolution — Experiments in electricity: Joseph Priestley — Priestley’s
experiments with gases — The discovery of oxygen — The chemical studies of Henry
Cavendish: publication in the
Philosophical Transactions — Water is not an
element — The Cavendish experiment: weighing the Earth — Antoine-Laurent
Lavoisier: study of air; study of the system of respiration — The first table of
elements; Lavoisier renames elements; he publishes
Elements of Chemistry

Lavoisier’s execution
8. Enlightened Science II:Progress on all fronts 285
The study of electricity: Stephen Gray, Charles Du Fay, Benjamin Franklin and
Charles Coulomb — Luigi Galvani, Alessandro Volta and the invention of the electric
battery — Pierre-Louis de Maupertuis: the principle of least action — Leonhard Euler:
mathematical description of the refraction of light — Thomas Wright: speculations
on the Milky Way — The discoveries of William and Caroline Herschel — John
Michell — Pierre Simon Laplace, ‘The French Newton’: his
Exposition — Benjamin
Thompson (Count Rumford): his life — Thompson’s thoughts on convection — His
thoughts on heat and motion — James Hutton: the uniformitarian theory of geology

Book Four: THE BIG PICTURE
9. The ‘Darwinian Revolution’ 319
Charles Lyell: His life — His travels in Europe and study of geology — He publishes
the
Principles of Geology — Lyell’s thoughts on species — Theories of evolution:
Erasmus Darwin and
Zoonomia — Jean-Baptiste Lamarck: the Lamarckian theory
of evolution — Charles Darwin: his life — The voyage of the
Beagle — Darwin
develops his theory of evolution by natural selection — Alfred Russel Wallace — The
publication of Darwin’s
Origin of Species

10. Atoms and Molecules 359
Humphry Davy’s work on gases; electrochemical research — John Dalton’s atomic
model; first talk of atomic weights — Jons Berzelius and the study of elements —
Avogadro’s number — William Prout’s hypothesis on atomic weights — Friedrich
Wo¨hler: studies in organic and inorganic substances — Valency — Stanislao
Cannizzaro: the distinction between atoms and molecules — The development of
the periodic table, by Mendeleyev and others — The science of thermodynamics —
James Joule on thermodynamics — William Thomson (Lord Kelvin) and the laws of
thermodynamics — James Clerk Maxwell and Ludwig Boltzmann: kinetic theory and
the mean free path of molecules — Albert Einstein: Avogadro’s number, Brownian
motion and why the sky is blue

11. Let There be Light 400
The wave model of light revived — Thomas Young: his double-slit experiment —
Fraunhofer lines — The study of spectroscopy and the spectra of stars — Michael
Faraday: his studies in electromagnetism — The invention of the electric motor and
the dynamo — Faraday on the lines of force — Measuring the speed of light — James
Clerk Maxwell’s complete theory of electromagnetism — Light is a form of
electromagnetic disturbance — Albert Michelson and Edward Morley: the
Michelson—Morley experiment on light — Albert Einstein: special theory of relativity
— Minkowski: the geometrical union of space and time in accordance with
this theory

12. The Last Hurrah! of Classical Science 442
Contractionism: our wrinkling planet? — Early hypotheses on continental drift —
Alfred Wegener: the father of the theory of continental drift — The evidence for
Pangea — The radioactive technique for measuring the age of rocks — Holmes’s
account of continental drift — Geomagnetic reversals and the molten core of the
Earth — The model of ‘sea-floor spreading’ — Further developments on continental
drift — The ‘Bullard fit’ of the continents — Plate tectonics — The story of Ice Ages:
Jean de Charpentier — Louis Agassiz and the glacial model — The astronomical
theory of Ice Ages — The elliptical orbit model — James Croll — The Milankovitch
model — Modern ideas about Ice Ages — The impact on evolution

Book Five: MODERN TIMES
13. Inner Space 487
Invention of the vacuum tube — ‘Cathode rays’ and ‘canal rays’ — William Crookes:
the Crookes tube and the corpuscular interpretation of cathode rays — Cathode rays
are shown to move far slower than light — The discovery of the electron — Wilhelm
Rontgen & the discovery of X-rays — Radioactivity; Becquerel and the Curies —
Discovery of alpha, beta and gamma radiation — Rutherford’s model of the atom —
Radioactive decay — The existence of isotopes — Discovery of the neutron — Max
Planck and Planck’s constant, black-body radiation and the existence of energy
quanta — Albert Einstein and light quanta — Niels Bohr — The •rst quantum model
of the atom — Louis de Broglie — Erwin Schro¨dinger’s wave equation for electrons —
The particle-based approach to the quantum world of electrons — Heisenberg’s
uncertainty principle: wave—particle duality — Dirac’s equation of the electron —
The existence of antimatter — The strong nuclear force — The weak nuclear force;
neutrinos — Quantum electrodynamics — The future? Quarks and string

14. The Realm of Life 529
The most complex things in the Universe — Charles Darwin and nineteenth-century
theories of evolution — The role of cells in life — The division of cells — The discovery
of chromosomes and their role in heredity — Intracellular pangenesis — Gregor
Mendel: father of genetics — The Mendelian laws of inheritance — The study of
chromosomes — Nucleic acid — Working towards DNA and RNA — The
tetranucleotide hypothesis — The Chargaff rules — The chemistry of life — Covalent
bond model and carbon chemistry — The ionic bond — Bragg’s law — Chemistry as a
branch of physics — Linus Pauling — The nature of the hydrogen bond — Studies of
fibrous proteins — The alpha-helix structure — Francis Crick and James Watson: the
model of the DNA double helix — The genetic code — The genetic age of
humankind — Humankind is nothing special

15. Outer Space 572
Measuring the distances of stars — Stellar parallax determinations — Spectroscopy
and the stuff of stars — The Hertzsprung—Russell diagram — The colour—magnitude
relationship and the distances to stars — The Cepheid distance scale — Cepheid stars
and the distances to other galaxies — General theory of relativity outlined — The
expanding Universe — The steady state model of the Universe — The nature of the
Big Bang — Predicting background radiation — Measuring background radiation —
Modern measurements: the COBE satellite — How the stars shine: the nuclear
fusion process — The concept of ‘resonances’ — CHON and humankind’s place in
the Universe — Into the unknown

Coda: The Pleasure of Finding Things Out
613
Bibliography 617
Index 625
From the Introduction

My aim is to outline the development of Western science, from the Renaissance to (roughly) the end of the twentieth century. This means leaving to one side the achievements of the Ancient Greeks, the Chinese, and the Islamic scientists and philosophers who did so much to keep the search for knowledge about our world alive during the period that Europeans refer to as the Dark and Middle Ages. But it also means telling a coherent story, with a
clear beginning in both space and time, of the development of the world view that lies at the heart of our understanding of the Universe, and our place in it today. For human life turned out to be no different from any other kind of life on Earth. As the work of Charles Darwin and Alfred Wallace established in the nineteenth century, all you need to make human beings out of amoebas is the process of evolution by natural selection, and plenty of time.

All the examples I have mentioned here highlight another feature of the story-telling process. It is natural to describe key events in terms of the work of individuals who made a mark in science ­ Copernicus, Vesalius, Darwin, Wallace and the rest. But this does not mean that science has progressed as a result of the work of a string of irreplaceable
geniuses possessed of a special insight into how the world works. Geniuses maybe (though not always); but irreplaceable certainly not. Scientific progress builds step by step, and as the example of Darwin and Wallace shows, when the time is ripe, two or more individuals may make the next step independently of one another. It is the luck of the draw, or historical accident, whose name gets remembered as the discoverer of a new phenomenon. What is much more important than human genius is the development of technology, and it is no surprise that the start of the scientific revolution `coincides' with the development of the telescope and the microscope.

I can think of only one partial exception to this situation, and even there I would qualify the exception more than most historians of science do. Isaac Newton was clearly something of a special case, both because of the breadth of his scientific achievements and in particular because of the clear way in which he laid down the ground rules on
which science ought to operate. Even Newton, though, relied on his immediate predecessors, in particular Galileo Galilei and Rene´ Descartes, and in that sense his contributions followed naturally from what went before. If Newton had never lived, scientific progress might have been held back by a few decades. But only by a few decades.

Edmond Halley or Robert Hooke might well have come up with the famous inverse square law of gravity; Gottfried Leibniz actually did invent calculus independently of Newton (and made a better job of it); and Christiaan Huygens's superior wave theory of light was held back by Newton's espousal of the rival particle theory.

None of this will stop me from telling much of my version of the history of science in terms of the people involved, including Newton. My choice of individuals to highlight in this way is not intended to be comprehensive; nor are my discussions of their individual lives and work intended to be complete. I have chosen stories that represent the
development of science in its historical context. Some of those stories, and the characters involved, may be familiar; others (I hope) less so.

But the importance of the people and their lives is that they reflect the society in which they lived, and by discussing, for example, the way the work of one specific scientist followed from that of another, I mean to indicate the way in which one generation of scientists influenced the next. This might seem to beg the question of how the ball got rolling in the first place ­ the `first cause'. But in this case it is easy to find the first cause ­ Western science got started because the Renaissance happened. And once it got started, by giving a boost to technology it ensured that it would keep on rolling, with new scientific ideas leading to improved technology, and improved technology providing the scien- tists with the means to test new ideas to greater and greater accuracy.

Technology came first, because it is possible to make machines by trial and error without fully understanding the principles on which they operate. But once science and technology got together, progress really took off.

I will leave the debate about why the Renaissance happened when and where it did to the historians. If you want a definite date to mark the beginning of the revival of Western Europe, a convenient one is 1453, the year the Turks captured Constantinople (on 29 May). By then, many Greek-speaking scholars, seeing which way the wind was
blowing, had already fled westwards (initially to Italy), taking their archives of documents with them. There, the study of those documents was taken up by the Italian humanist movement, who were interested in using the teaching found in classical literature to re-establish civilization along the lines that had existed before the Dark Ages. This does rather neatly tie the rise of modern Europe to the death of the last vestige of the old Roman Empire. But an equally important factor, as many people have argued, was the depopulation of Europe by the Black Death in the fourteenth century, which led the survivors to question the whole basis of society, made labour expensive and encour- aged the invention of technological devices to replace manpower.

Even this is not the whole story. Johann Gutenberg's development of moveable type in the mid-fifteenth century had an obvious impact on what was to become science, and discoveries brought back to Europe by another technological development, sailing ships capable of crossing the oceans, transformed society.

Dating the end of the Renaissance is no easier than dating the beginning ­ you could say that it is still going on. A convenient round number is 1700; but from the present perspective an even better choice of date might be 1687, the year Isaac Newton published his great work Philosophiae Naturalis Principia Mathematica (The Mathematical
Principles of Natural Philosophy) and, in the words of Alexander Pope, `all was light'.

The point I want to make is that the scientific revolution did not happen in isolation, and certainly did not start out as the mainspring of change, although in many ways science (through its influence on technology and on our world view) became the driving force of Western civilization. I want to show how science developed, but I don't have space to do justice to the full historical background, any more than most history books have space to do justice to the story of science. I don't even have space to do justice to all of the science here, so if you want the in-depth story of such key concepts as quantum theory, evolution by natural selection or plate tectonics, you will have to look in other books (including my own). My choice of events to highlight is necessarily incomplete, and therefore to some extent subjective, but my aim is to give a feel for the full sweep of science, which has taken us from the realization that the Earth is not at the centre of the Universe and that human beings are `only' animals, to the theory of the Big Bang and a complete map of the human genome in just over 450 years.
John Gribbin, PhD, trained as an astrophysicist at the University of Cambridge before becoming a full-time science writer. His books include the highly acclaimed In Search of Schrödinger's Cat, The First Chimpanzee, In Search of the Big Bang, In the Beginning, In Search of the Edge of Time, In Search of the Double Helix, The Stuff of the Universe (with Martin Rees), Stephen Hawking: A Life in Science, and Einstein: A Life in Science (with Michael White). View titles by John Gribbin

About

In this new and landmark history of modern science, author and trained astrophysicist John Gribbin recounts the development of science over the past five-hundred years—as seen specifically through the lives and achievements of individual scientists.

John Gribbin has written extensively before on scientific subjects such as the theory of everything, the existence of reality, and Schrödinger's cat. However, in The Scientists, he shifts his focus to the people who have conceived and produced modern science's theories, inventions, and innovations. He examines the times in which these scientists lived and worked and how their particular contributions influenced the overall development and direction of scientific inquiry. In the process, Gribbin not only re-evaluates the significance of such venerable icons as Galileo, Isaac Newton, Albert Einstein and Linus Pauling, but he also examines lesser lights whose stories have been undeservedly neglected.

Invaluable for those studying the history of science, and useful for those considering the impact of science on stages of history from the Renaissance and up to the present-day, The Scientists is ultimately a completely original, expansive, and nuanced survey of the most important scientific figures of the past half-millennium.

"Well written and scholarly, it is still accessible....[Gribbin] also clearly understands the important role that technology played in making science's greatest discoveries possible....Highly recommended for public and academic libraries or as a text for the history of science."
Library Journal

"As expansive (and as massive) as a textbook...explores the development of modern science through the individual stories of philosophers and scientists both renowned and overlooked."
Publishers Weekly

"Admirably ambitious in scope.... Highly recommended." M. Schiff, CUNY College of Staten Island for Choice Magazine (American Library Association)

“Essential reading...tells the story of science as a sequence of witty, information-packed tales...complete with humanizing asides, glimpses of the scientist’s personal life and amusing anecdotes.”
London Sunday Times, Books of the Year


TABLE OF CONTENTS
List of Illustrations
xi
Acknowledgements xv
Introduction xvii

Book One: OUT OF THE DARK AGES

1. Renaissance Men
Emerging from the dark — The elegance of Copernicus — The Earth moves! — The
orbits of the planets — Leonard Digges and the telescope — Thomas Digges and the
infinite Universe — Bruno: a martyr for science? — Copernican model banned by
Catholic Church — Vesalius: surgeon, dissector and grave-robber — Fallopio and
Fabricius — William Harvey and the circulation of the blood

2. The Last Mystics
The movement of the planets — Tycho Brahe — Measuring star positions — Tycho’s
supernova — Tycho observes comet — His model of the Universe — Johannes Kepler:
Tycho’s assistant and inheritor — Kepler’s geometrical model of the Universe — New
thoughts on the motion of planets: Kepler’s first and second laws — Kepler’s third
law — Publication of the Rudolphine star tables — Kepler’s death

3. The First Scientists
William Gilbert and magnetism — Galileo on the pendulum, gravity and
acceleration — His invention of the ‘compass’ — His supernova studies —
Lippershey’s reinvention of the telescope — Galileo’s developments thereon —
Copernican ideas of Galileo judged heretical — Galileo publishes
Dialogue on the
Two Chief World Systems — Threatened with torture, he recants — Galileo
publishes
Two New Sciences — His death

Book Two: THE FOUNDING FATHERS
4. Science Finds its Feet 107
Rene´ Descartes and Cartesian co-ordinates — His greatest works — Pierre Gassendi:
atoms and molecules — Descartes’s rejection of the concept of a vacuum —
Christiaan Huygens: his work on optics and the wave theory of light — Robert Boyle:
his study of gas pressure — Boyle’s scientific approach to alchemy — Marcello
Malpighi and the circulation of the blood — Giovanni Borelli and Edward Tyson: the
increasing perception of animal (and man) as machine.

5. The ‘Newtonian Revolution’ 149
Robert Hooke: the study of microscopy and the publication of Micrographia —
Hooke’s study of the wave theory of light — Hooke’s law of elasticity — John
Flamsteed and Edmond Halley: cataloguing stars by telescope — Newton’s early life
— The development of calculus — The wrangling of Hooke and Newton — Newton’s
Principia Mathematica: the inverse square law and the three laws of motion —
Newton’s later life — Hooke’s death and the publication of Newton’s
Opticks

6. Expanding Horizons 193
Edmond Halley — Transits of Venus — The effort to calculate the size of an atom —
Halley travels to sea to study terrestrial magnetism — Predicts return of comet —
Proves that stars move independently — Death of Halley — John Ray and Francis
Willughby: the first-hand study of flora and fauna — Carl Linnaeus and the naming
of species — The Comte de Buffon:
Histoire Naturelle and thoughts on the age of
the Earth — Further thoughts on the age of the Earth: Jean Fourier and Fourier
analysis — Georges Couvier: Lectures in Comparative Anatomy; speculations on
extinction — Jean-Baptiste Lamarck: thoughts on evolution

Book Three:T HE ENLIGHTENMENT
7. Enlightened Science I:Chemistry catches up 241
The Enlightenment — Joseph Black and the discovery of carbon dioxide — Black on
temperature — The steam engine: Thomas Newcomen, James Watt and the
Industrial Revolution — Experiments in electricity: Joseph Priestley — Priestley’s
experiments with gases — The discovery of oxygen — The chemical studies of Henry
Cavendish: publication in the
Philosophical Transactions — Water is not an
element — The Cavendish experiment: weighing the Earth — Antoine-Laurent
Lavoisier: study of air; study of the system of respiration — The first table of
elements; Lavoisier renames elements; he publishes
Elements of Chemistry

Lavoisier’s execution
8. Enlightened Science II:Progress on all fronts 285
The study of electricity: Stephen Gray, Charles Du Fay, Benjamin Franklin and
Charles Coulomb — Luigi Galvani, Alessandro Volta and the invention of the electric
battery — Pierre-Louis de Maupertuis: the principle of least action — Leonhard Euler:
mathematical description of the refraction of light — Thomas Wright: speculations
on the Milky Way — The discoveries of William and Caroline Herschel — John
Michell — Pierre Simon Laplace, ‘The French Newton’: his
Exposition — Benjamin
Thompson (Count Rumford): his life — Thompson’s thoughts on convection — His
thoughts on heat and motion — James Hutton: the uniformitarian theory of geology

Book Four: THE BIG PICTURE
9. The ‘Darwinian Revolution’ 319
Charles Lyell: His life — His travels in Europe and study of geology — He publishes
the
Principles of Geology — Lyell’s thoughts on species — Theories of evolution:
Erasmus Darwin and
Zoonomia — Jean-Baptiste Lamarck: the Lamarckian theory
of evolution — Charles Darwin: his life — The voyage of the
Beagle — Darwin
develops his theory of evolution by natural selection — Alfred Russel Wallace — The
publication of Darwin’s
Origin of Species

10. Atoms and Molecules 359
Humphry Davy’s work on gases; electrochemical research — John Dalton’s atomic
model; first talk of atomic weights — Jons Berzelius and the study of elements —
Avogadro’s number — William Prout’s hypothesis on atomic weights — Friedrich
Wo¨hler: studies in organic and inorganic substances — Valency — Stanislao
Cannizzaro: the distinction between atoms and molecules — The development of
the periodic table, by Mendeleyev and others — The science of thermodynamics —
James Joule on thermodynamics — William Thomson (Lord Kelvin) and the laws of
thermodynamics — James Clerk Maxwell and Ludwig Boltzmann: kinetic theory and
the mean free path of molecules — Albert Einstein: Avogadro’s number, Brownian
motion and why the sky is blue

11. Let There be Light 400
The wave model of light revived — Thomas Young: his double-slit experiment —
Fraunhofer lines — The study of spectroscopy and the spectra of stars — Michael
Faraday: his studies in electromagnetism — The invention of the electric motor and
the dynamo — Faraday on the lines of force — Measuring the speed of light — James
Clerk Maxwell’s complete theory of electromagnetism — Light is a form of
electromagnetic disturbance — Albert Michelson and Edward Morley: the
Michelson—Morley experiment on light — Albert Einstein: special theory of relativity
— Minkowski: the geometrical union of space and time in accordance with
this theory

12. The Last Hurrah! of Classical Science 442
Contractionism: our wrinkling planet? — Early hypotheses on continental drift —
Alfred Wegener: the father of the theory of continental drift — The evidence for
Pangea — The radioactive technique for measuring the age of rocks — Holmes’s
account of continental drift — Geomagnetic reversals and the molten core of the
Earth — The model of ‘sea-floor spreading’ — Further developments on continental
drift — The ‘Bullard fit’ of the continents — Plate tectonics — The story of Ice Ages:
Jean de Charpentier — Louis Agassiz and the glacial model — The astronomical
theory of Ice Ages — The elliptical orbit model — James Croll — The Milankovitch
model — Modern ideas about Ice Ages — The impact on evolution

Book Five: MODERN TIMES
13. Inner Space 487
Invention of the vacuum tube — ‘Cathode rays’ and ‘canal rays’ — William Crookes:
the Crookes tube and the corpuscular interpretation of cathode rays — Cathode rays
are shown to move far slower than light — The discovery of the electron — Wilhelm
Rontgen & the discovery of X-rays — Radioactivity; Becquerel and the Curies —
Discovery of alpha, beta and gamma radiation — Rutherford’s model of the atom —
Radioactive decay — The existence of isotopes — Discovery of the neutron — Max
Planck and Planck’s constant, black-body radiation and the existence of energy
quanta — Albert Einstein and light quanta — Niels Bohr — The •rst quantum model
of the atom — Louis de Broglie — Erwin Schro¨dinger’s wave equation for electrons —
The particle-based approach to the quantum world of electrons — Heisenberg’s
uncertainty principle: wave—particle duality — Dirac’s equation of the electron —
The existence of antimatter — The strong nuclear force — The weak nuclear force;
neutrinos — Quantum electrodynamics — The future? Quarks and string

14. The Realm of Life 529
The most complex things in the Universe — Charles Darwin and nineteenth-century
theories of evolution — The role of cells in life — The division of cells — The discovery
of chromosomes and their role in heredity — Intracellular pangenesis — Gregor
Mendel: father of genetics — The Mendelian laws of inheritance — The study of
chromosomes — Nucleic acid — Working towards DNA and RNA — The
tetranucleotide hypothesis — The Chargaff rules — The chemistry of life — Covalent
bond model and carbon chemistry — The ionic bond — Bragg’s law — Chemistry as a
branch of physics — Linus Pauling — The nature of the hydrogen bond — Studies of
fibrous proteins — The alpha-helix structure — Francis Crick and James Watson: the
model of the DNA double helix — The genetic code — The genetic age of
humankind — Humankind is nothing special

15. Outer Space 572
Measuring the distances of stars — Stellar parallax determinations — Spectroscopy
and the stuff of stars — The Hertzsprung—Russell diagram — The colour—magnitude
relationship and the distances to stars — The Cepheid distance scale — Cepheid stars
and the distances to other galaxies — General theory of relativity outlined — The
expanding Universe — The steady state model of the Universe — The nature of the
Big Bang — Predicting background radiation — Measuring background radiation —
Modern measurements: the COBE satellite — How the stars shine: the nuclear
fusion process — The concept of ‘resonances’ — CHON and humankind’s place in
the Universe — Into the unknown

Coda: The Pleasure of Finding Things Out
613
Bibliography 617
Index 625

Excerpt

From the Introduction

My aim is to outline the development of Western science, from the Renaissance to (roughly) the end of the twentieth century. This means leaving to one side the achievements of the Ancient Greeks, the Chinese, and the Islamic scientists and philosophers who did so much to keep the search for knowledge about our world alive during the period that Europeans refer to as the Dark and Middle Ages. But it also means telling a coherent story, with a
clear beginning in both space and time, of the development of the world view that lies at the heart of our understanding of the Universe, and our place in it today. For human life turned out to be no different from any other kind of life on Earth. As the work of Charles Darwin and Alfred Wallace established in the nineteenth century, all you need to make human beings out of amoebas is the process of evolution by natural selection, and plenty of time.

All the examples I have mentioned here highlight another feature of the story-telling process. It is natural to describe key events in terms of the work of individuals who made a mark in science ­ Copernicus, Vesalius, Darwin, Wallace and the rest. But this does not mean that science has progressed as a result of the work of a string of irreplaceable
geniuses possessed of a special insight into how the world works. Geniuses maybe (though not always); but irreplaceable certainly not. Scientific progress builds step by step, and as the example of Darwin and Wallace shows, when the time is ripe, two or more individuals may make the next step independently of one another. It is the luck of the draw, or historical accident, whose name gets remembered as the discoverer of a new phenomenon. What is much more important than human genius is the development of technology, and it is no surprise that the start of the scientific revolution `coincides' with the development of the telescope and the microscope.

I can think of only one partial exception to this situation, and even there I would qualify the exception more than most historians of science do. Isaac Newton was clearly something of a special case, both because of the breadth of his scientific achievements and in particular because of the clear way in which he laid down the ground rules on
which science ought to operate. Even Newton, though, relied on his immediate predecessors, in particular Galileo Galilei and Rene´ Descartes, and in that sense his contributions followed naturally from what went before. If Newton had never lived, scientific progress might have been held back by a few decades. But only by a few decades.

Edmond Halley or Robert Hooke might well have come up with the famous inverse square law of gravity; Gottfried Leibniz actually did invent calculus independently of Newton (and made a better job of it); and Christiaan Huygens's superior wave theory of light was held back by Newton's espousal of the rival particle theory.

None of this will stop me from telling much of my version of the history of science in terms of the people involved, including Newton. My choice of individuals to highlight in this way is not intended to be comprehensive; nor are my discussions of their individual lives and work intended to be complete. I have chosen stories that represent the
development of science in its historical context. Some of those stories, and the characters involved, may be familiar; others (I hope) less so.

But the importance of the people and their lives is that they reflect the society in which they lived, and by discussing, for example, the way the work of one specific scientist followed from that of another, I mean to indicate the way in which one generation of scientists influenced the next. This might seem to beg the question of how the ball got rolling in the first place ­ the `first cause'. But in this case it is easy to find the first cause ­ Western science got started because the Renaissance happened. And once it got started, by giving a boost to technology it ensured that it would keep on rolling, with new scientific ideas leading to improved technology, and improved technology providing the scien- tists with the means to test new ideas to greater and greater accuracy.

Technology came first, because it is possible to make machines by trial and error without fully understanding the principles on which they operate. But once science and technology got together, progress really took off.

I will leave the debate about why the Renaissance happened when and where it did to the historians. If you want a definite date to mark the beginning of the revival of Western Europe, a convenient one is 1453, the year the Turks captured Constantinople (on 29 May). By then, many Greek-speaking scholars, seeing which way the wind was
blowing, had already fled westwards (initially to Italy), taking their archives of documents with them. There, the study of those documents was taken up by the Italian humanist movement, who were interested in using the teaching found in classical literature to re-establish civilization along the lines that had existed before the Dark Ages. This does rather neatly tie the rise of modern Europe to the death of the last vestige of the old Roman Empire. But an equally important factor, as many people have argued, was the depopulation of Europe by the Black Death in the fourteenth century, which led the survivors to question the whole basis of society, made labour expensive and encour- aged the invention of technological devices to replace manpower.

Even this is not the whole story. Johann Gutenberg's development of moveable type in the mid-fifteenth century had an obvious impact on what was to become science, and discoveries brought back to Europe by another technological development, sailing ships capable of crossing the oceans, transformed society.

Dating the end of the Renaissance is no easier than dating the beginning ­ you could say that it is still going on. A convenient round number is 1700; but from the present perspective an even better choice of date might be 1687, the year Isaac Newton published his great work Philosophiae Naturalis Principia Mathematica (The Mathematical
Principles of Natural Philosophy) and, in the words of Alexander Pope, `all was light'.

The point I want to make is that the scientific revolution did not happen in isolation, and certainly did not start out as the mainspring of change, although in many ways science (through its influence on technology and on our world view) became the driving force of Western civilization. I want to show how science developed, but I don't have space to do justice to the full historical background, any more than most history books have space to do justice to the story of science. I don't even have space to do justice to all of the science here, so if you want the in-depth story of such key concepts as quantum theory, evolution by natural selection or plate tectonics, you will have to look in other books (including my own). My choice of events to highlight is necessarily incomplete, and therefore to some extent subjective, but my aim is to give a feel for the full sweep of science, which has taken us from the realization that the Earth is not at the centre of the Universe and that human beings are `only' animals, to the theory of the Big Bang and a complete map of the human genome in just over 450 years.

Author

John Gribbin, PhD, trained as an astrophysicist at the University of Cambridge before becoming a full-time science writer. His books include the highly acclaimed In Search of Schrödinger's Cat, The First Chimpanzee, In Search of the Big Bang, In the Beginning, In Search of the Edge of Time, In Search of the Double Helix, The Stuff of the Universe (with Martin Rees), Stephen Hawking: A Life in Science, and Einstein: A Life in Science (with Michael White). View titles by John Gribbin