"Once I had learnt my twelve times table (at the age of three) it was downhill all the way." -- Fred Hoyle
Sir Fred Hoyle FRS (24 June 1915 – 20 August 2001) was an English astronomer and mathematician noted primarily for his contribution to the theory of stellar nucleosynthesis and his often controversial stance on other cosmological and scientific matters...in particular his rejection of the "Big Bang" theory, a term originally coined by him as a jocular, perhaps disparaging, name for the theory which was the main rival to his own. In addition to his work as an astronomer, Hoyle was a writer of science fiction, including a number of books co-written with his son Geoffrey Hoyle. Hoyle spent most of his working life at the Institute of Astronomy at Cambridge and served as its director for a number of years. He died in Bournemouth, England, after a series of strokes.
"I don't see the logic of rejecting data just because they seem incredible.""Space isn't remote at all. It's only an hour's drive away if your car could go straight upwards.""The man who voyages strange seas must of necessity be a little unsure of himself. It is the man with the flashy air of knowing everything, who is always with it, that we should beware of.""There is a coherent plan in the universe, though I don't know what it's a plan for.""Things are the way they are because they were the way they were."
Hoyle was born in Gilstead, West Yorkshire, England, near Bradford, where his father, Ben Hoyle, worked in the wool trade. His mother, Mabel Pickard, had studied music at the Royal College of Music in London. Hoyle was educated at Bingley Grammar School and read mathematics at Emmanuel College, Cambridge.
An early paper of Hoyle's made an interesting use of the anthropic principle. In trying to work out the routes of stellar nucleosynthesis, he observed that one particular nuclear reaction, the triple-alpha process, which generates carbon, would require the carbon nucleus to have a very specific energy for it to work. The large amount of carbon in the universe, which makes it possible for carbon-based life-forms (e.g. humans) to exist, demonstrated that this nuclear reaction must work. Based on this notion, he made a prediction of the energy levels in the carbon nucleus that was later borne out by experiment.
However, those energy levels, while needed in order to produce carbon in large quantities, were statistically very unlikely. Hoyle later wrote:
Would you not say to yourself, "Some super-calculating intellect must have designed the properties of the carbon atom, otherwise the chance of my finding such an atom through the blind forces of nature would be utterly minuscule." Of course you would . . . A common sense interpretation of the facts suggests that a superintellect has monkeyed with physics, as well as with chemistry and biology, and that there are no blind forces worth speaking about in nature. The numbers one calculates from the facts seem to me so overwhelming as to put this conclusion almost beyond question.
Hoyle, an atheist until that time, said that this suggestion of a guiding hand left him "greatly shaken." Consequently, he began to believe in a guiding force in the universe, which led him to a belief in panspermia. Those who advocate the intelligent design hypothesis sometimes cite Hoyle's work in this area to support the claim that the universe was fine tuned in order to allow intelligent life to be possible. Alfred Russel of the Uncommon Descent community has even gone so far as labeling Hoyle "an atheist for ID". Some of Hoyle's thoughts in this area have been referred to as "Hoyle's fallacy" by detractors.
His co-worker William Alfred Fowler eventually won the Nobel Prize for Physics in 1983 (with Subrahmanyan Chandrasekhar), but for some reason Hoyle’s original contribution was overlooked, and many were surprised that such a notable astronomer missed out. Fowler himself in an autobiographical sketch affirmed Hoyle’s pioneering efforts:
The concept of nucleosynthesis in stars was first established by Hoyle in 1946. This provided a way to explain the existence of elements heavier than helium in the universe, basically by showing that critical elements such as carbon could be generated in stars and then incorporated in other stars and planets when that star "dies". The new stars formed now start off with these heavier elements and even heavier elements are formed from them. Hoyle theorized that other rarer elements could be explained by supernovas, the giant explosions which occasionally occur throughout the universe, whose temperatures and pressures would be required to create such elements.
While having no argument with the Lemaître theory (later confirmed by Edwin Hubble's observations) that the universe was expanding, Hoyle disagreed on its interpretation. He found the idea that the universe had a beginning to be philosophically troubling, as many argued that a beginning implies a cause, and thus a creator (see Kalam cosmological argument). Instead, Hoyle, along with Thomas Gold and Hermann Bondi (with whom he had worked on radar in World War II), argued for the universe as being in a "steady state". The theory tried to explain how the universe could be eternal and essentially unchanging while still having the galaxies we observe moving away from each other. The theory hinged on the creation of matter between galaxies over time, so that even though galaxies get further apart, new ones that develop between them fill the space they leave. The resulting universe is in a "steady state" in the same manner that a flowing river is - the individual water molecules are moving away but the overall river remains the same.
The theory was one alternative to the Big Bang which agreed with key observations of the day, namely Hubble's red shift observations, and Hoyle was a strong critic of the Big Bang. Ironically, he is responsible for coining the term "Big Bang" on BBC radio's Third Programme broadcast at 1830 GMT on 28 March 1949. It is popularly reported that Hoyle intended this to be pejorative, but the script from which he read aloud clearly shows that he intended the expression to help his listeners. In addition, Hoyle explicitly denied that he was being insulting and said it was just a striking image meant to emphasize the difference between the two theories for radio listeners.
Hoyle, unlike Gold and Bondi, offered an explanation for the appearance of new matter by postulating the existence of what he dubbed the "creation field", or just the "C-field", which had negative pressure in order to be consistent with the conservation of energy and drive the expansion of the universe. These features of the C-field anticipated the later development of cosmic inflation. They jointly argued that continuous creation was no more inexplicable than the appearance of the entire universe from nothing, although it had to be done on a regular basis. In the end, mounting observational evidence convinced most cosmologists that the steady state model was incorrect and that the Big Bang was the theory that agreed best with observations, although Hoyle continued to support and develop his theory. In 1993, in an attempt to explain some of the evidence against the steady state theory, he presented a modified version called "quasi-steady state cosmology" (QSS), but the theory is not widely accepted.
The evidence that resulted in the Big Bang's victory over the steady state model, at least in the minds of most cosmologists, included the discovery of the cosmic microwave background radiation in the 1960s, the distribution of "young galaxies" and quasars throughout the Universe in the 1980s, a more consistent age estimate of the universe and most recently the observations of the COBE satellite in the 1990s and the Wilkinson Microwave Anisotropy Probe launched in 2001, which showed unevenness in the microwave background in the early universe, which corresponds to currently observed distributions of galaxies.
Hoyle appeared in a series of radio talks on astronomy for the BBC in the 1950s; these were collected in the book The Nature of the Universe, and he went on to write a number of other popular science books. In 1957 he was elected a Fellow of the Royal Society, and he was knighted in 1972. He was jointly awarded the Crafoord Prize by the Royal Swedish Academy of Sciences.
In the play Sur la route de Montalcino, the character of Fred Hoyle confronts Georges Lemaître on a fictional journey to the Vatican in 1957.
In his later years, Hoyle became a staunch critic of theories of chemical evolution used to explain the naturalistic origin of life. With Chandra Wickramasinghe, Hoyle promoted the theory that life evolved in space, spreading through the universe via panspermia, and that evolution on earth is driven by a steady influx of viruses arriving via comets. In 1982, Hoyle presented Evolution from Space for the Royal Institution's Omni Lecture. After considering what he thought of as a very remote probability of evolution he concluded: Published in his 1982/1984 books Evolution from Space (co-authored with Chandra Wickramasinghe), Hoyle calculated that the chance of obtaining the required set of enzymes for even the simplest living cell was one in 1040,000. Since the number of atoms in the known universe is infinitesimally tiny by comparison (1080), he argued that even a whole universe full of primordial soup would grant little chance to evolutionary processes. He claimed:
The notion that not only the biopolymer but the operating program of a living cell could be arrived at by chance in a primordial organic soup here on the Earth is evidently nonsense of a high order.
Hoyle compared the random emergence of even the simplest cell to the likelihood that "a tornado sweeping through a junk-yard might assemble a Boeing 747 from the materials therein." Hoyle also compared the chance of obtaining even a single functioning protein by chance combination of amino acids to a solar system full of blind men solving Rubik's Cube simultaneously. (See the watchmaker analogy for similar reasoning.) Hoyle's statements and this line of reasoning (at various levels of accuracy) appears frequently in support of intelligent design. Mainstream evolutionary biology rejects Hoyle's interpretation of statistics, and supporters of modern evolutionary theory, such as Richard Dawkins, refer to this as "Hoyle's fallacy".
Further occasions on which Hoyle aroused controversy included his questioning the authenticity of fossil Archaeopteryx and his condemnation of the failure to include Jocelyn Bell in the Nobel Prize award recognizing the development of radio interferometry and its role in the discovery of pulsars.
The most important of Hoyle's contributions was probably his work on nucleosynthesis: the idea that the chemical elements were synthesized from primordial hydrogen and helium in stars. Many thought it unfair that a Nobel prize was awarded to his collaborator William A Fowler, but Hoyle himself was excluded from the prize.
Hoyle had a famously heated argument with Martin Ryle of the Cavendish Radio Astronomy Group about Hoyle's steady state theory, which somewhat restricted collaboration between the Cavendish group and the Cambridge Institute of Astronomy during the 1960s.
As did Thomas Gold, Hoyle defended primordial origin of natural hydrocarbons (oil and natural gas)."The suggestion that petroleum might have arisen from some transformation of squashed fish or biological detritus is surely the silliest notion to have been entertained by substantial numbers of persons over an extended period of time." Fred Hoyle, 1982.
Hoyle also wrote science fiction. In his first novel, The Black Cloud, most intelligent life in the universe takes the form of interstellar gas clouds; they are surprised to learn that intelligent life can also form on planets. He wrote a television series, A for Andromeda, which was also published as a novel. His play Rockets in Ursa Major had a professional production at the Mermaid Theatre in 1962.
The Black Cloud, 1957
Ossian's Ride, 1959
A for Andromeda, 1962 (co-authored with John Elliot)
Fifth Planet, 1963 (co-authored with Geoffrey Hoyle)
The Andromeda Breakthrough, 1965 (co-authored with John Elliot)
October the First Is Too Late, 1966
Element 79, 1967
Rockets in Ursa Major, 1969 (co-authored with Geoffrey Hoyle)
Seven Steps to the Sun, 1970 (co-authored with Geoffrey Hoyle)
The Inferno, 10/1973 (co-authored with Geoffrey Hoyle)
The Molecule Men and the Monster of Loch Ness, 1973 (co-authored with Geoffrey Hoyle)
Into Deepest Space, 1974 (co-authored with Geoffrey Hoyle)
The Incandescent Ones, 1977 (co-authored with Geoffrey Hoyle)
The Westminster Disaster, 10/1978 (co-authored with Geoffrey Hoyle)
Comet Halley, 11/1985
The Frozen Planet of Azuron, 1982 (Ladybird Books, co-authored with Geoffrey Hoyle)
The Energy Pirate, 1982 (Ladybird Books, co-authored with Geoffrey Hoyle)
The Planet of Death, 1982 (Ladybird Books, co-authored with Geoffrey Hoyle)
The Giants of Universal Park, 1982 (Ladybird Books, co-authored with Geoffrey Hoyle)
Most of these are independent of each other. Andromeda Breakthrough is a sequel to A for Andromeda and Into Deepest Space is a sequel to Rockets in Ursa Major. The four Ladybird Books are intended for children.
The Nature of the Universe - a series of broadcast lectures, Basil Blackwell, Oxford 1950 (early use of the big bang phrase)
Frontiers of Astronomy, Heinemann Education Books Limited, London, 1955. - The Internet Archive. HarperCollins, ISBN 0060027606 ISBN 978-0060027605
Burbidge, E.M., Burbidge, G.R., Fowler, W.A. and Hoyle, F., Synthesis of the Elements in Stars, Revs. Mod. Physics29:547–650, 1957, the famous B²FH paper after their initials, for which Hoyle is most famous among professional cosmologists.
Astronomy, A history of man's investigation of the universe, Crescent Books, Inc., London 1962 LC 62-14108
Galaxies, Nuclei, and Quasars, Harper & Row, Publishers, New York, 1965 LC-65-20996
Nicolaus Copernicus, Heinemann Educational Books Ltd., London, p. 78, 1973
Astronomy and Cosmology: A Modern Course, 1975, ISBN 0-7167-0351-3
Energy or Extinction? The case for nuclear energy, 1977, Heinemann Educational Books Limited, ISBN 0-435-54430-6. In this provocative book Hoyle establishes the dependence of Western civilization on energy consumption and predicts that nuclear fission as a source of energy is essential for its survival.
Ten Faces of the Universe, 1977, W. H. Freeman and Company (San Francisco), ISBN 0-7167-0384X, ISBN 0-7167-0383-1
Lifecloud - The Origin of Life in the Universe, Hoyle, F. and Wickramasinghe C., J. M. Dent and Sons, 1978. ISBN 0-460-04335-8
Commonsense in Nuclear Energy, Fred Hoyle and Geoffrey Hoyle, 1980, Heinemann Educational Books Ltd., ISBN 0-435-54432-2
The big bang in astronomy, New Scientist92(1280):527, November 19, 1981.
Ice, the Ultimate Human Catastrophe,1981, ISBN 0826400647 Snippet view from Google Books
The Intelligent Universe, 1983
Evolution from space (the Omni lecture) and other papers on the origin of life 1982, ISBN 0894900838
Evolution from Space: A Theory of Cosmic Creationism, 1984, ISBN 0-671-49263-2
With Jayant Narlikar and Chandra Wickramasinghe, The extragalactic universe: an alternative view, Nature346:807–812, August 30, 1990.
The Origin of the Universe and the Origin of Religion,1993, ISBN 1559210834
Home Is Where the Wind Blows: Chapters from a Cosmologist's Life (autobiography) Oxford University Press 1994, ISBN 0-19-850060-2
Mathematics of Evolution, (1987) University College Cardiff Press, (1999) Acorn Enterprises LLC., ISBN 0-9669934-0-3
With G. Burbridge and Narlikar J. V. A Different Approach to Cosmology, Cambridge University Press 2000, ISBN 0-521-66223-0
Alan P. Lightman and Roberta Brawer, Origins: The Lives and Worlds of Modern Cosmologists, Harvard University Press, 1990. A collection of interviews, mostly with the generation (or two) of cosmologists after Hoyle, but also including an interview with Hoyle himself. Several interviewees testify to Hoyle's influence in popularizing astronomy and cosmology.
Dennis Overbye, Lonely Hearts of the Cosmos: The Scientific Quest for the Secret of the Universe, HarperCollins, 1991. ISBN 0330295853 Second edition (with new afterword), Back Bay, 1999. Gives a biographical account of modern cosmology in a novel-like fashion. Complementary to Origins.
Simon Mitton, Conflict in the Cosmos: Fred Hoyle's Life in Science, Joseph Henry Press, 2005. ISBN 0-309-09313-9 or, Fred Hoyle: A Life in Science, Aurum Press, 2005. ISBN 1-85410-961-8
Douglas Gough, editor, The Scientific Legacy of Fred Hoyle, Cambridge University Press, 2005. ISBN 0-521-82448-6
Chandra Wickramasinghe, A Journey with Fred Hoyle: The Search for Cosmic Life, World Scientific Publishing, 2005. ISBN 981-238-912-1
Jane Gregory, Fred Hoyle's Universe, Oxford University Press, 2005. ISBN 0-19-850791-7
