A Briefer History of Time (2005) - Stephen Hawking
A Briefer History of Time is a 2005 popular-science book by
the English physicist Stephen Hawking and the American physicist Leonard
Mlodinow. It is an update and rewrite of Hawking's 1988 A Brief History of
Time. In this book Hawking and Mlodinow present quantum mechanics, string
theory, the big bang theory, and other topics in a more accessible fashion to
the general public. The book is updated with newly discovered topics, and
informs of recurring subjects throughout the book in greater detail.
A Brief History of Time: From the Big Bang to Black Holes is
a popular-science book on cosmology (the study of the universe) by British
physicist Stephen Hawking. It was first published in 1988. Hawking wrote the
book for nonspecialist readers with no prior knowledge of scientific theories.
In A Brief History of Time, Hawking writes in non-technical
terms about the structure, origin, development and eventual fate of the
universe, which is the object of study of astronomy and modern physics. He
talks about basic concepts like space and time, basic building blocks that make
up the universe (such as quarks) and the fundamental forces that govern it
(such as gravity). He writes about cosmological phenomena such as the Big Bang
and the black holes. He discusses two major theories, general relativity and
quantum mechanics, that modern scientists use to describe the universe.
Finally, he talks about the search for a unifying theory that describes
everything in the universe in a coherent manner.
The book became a bestseller and sold more than 10 million
copies in 20 years. It was also on the London Sunday Times bestseller list for
more than five years and was translated into 35 languages by 2001.
Early in 1983, Hawking first approached Simon Mitton, the
editor in charge of astronomy books at Cambridge University Press, with his
ideas for a popular book on cosmology. Mitton was doubtful about all the
equations in the draft manuscript, which he felt would put off the buyers in
airport bookshops that Hawking wished to reach. With some difficulty, he persuaded
Hawking to drop all but one equation. The author himself notes in the book's
acknowledgements that he was warned that for every equation in the book, the
readership would be halved, hence it includes only a single equation: E = mc2.
The book does employ a number of complex models, diagrams, and other
illustrations to detail some of the concepts it explores.
Today, it is known that the opposite is true: the earth goes
around the sun. The Aristotelian and Ptolemaic ideas about the position of the
stars and sun were disproved in 1609. The first person to present a detailed
argument that the earth revolves around the sun was the Polish priest Nicholas
Copernicus, in 1514. Nearly a century later, Galileo Galilei, an Italian
scientist and Johannes Kepler, a German scientist, studied how the moons of
some planets moved in the sky, and used their observations to validate
Copernicus's thinking. To fit the observations, Kepler proposed an elliptical
orbit model instead of a circular one. In his 1687 book on gravity, Principia
Mathematica, Isaac Newton used complex mathematics to further support
Copernicus's idea. Newton's model also meant that stars, like the sun, were not
fixed but, rather, faraway moving objects. Nevertheless, Newton believed that
the universe was made up of an infinite number of stars which were more or less
static. Many of his contemporaries, including German philosopher Heinrich
Olbers, disagreed.
The origin of the universe represented another great topic of
study and debate over the centuries. Early philosophers like Aristotle thought
that the universe has existed forever, while theologians such as St. Augustine
believed it was created at a specific time. St. Augustine also believed that
time was a concept that was born with the creation of the universe. More than
1000 years later, German philosopher Immanuel Kant thought that time goes back
forever.
In 1929, astronomer Edwin Hubble discovered that galaxies are
moving away from each other. Consequently, there was a time, between ten and twenty
billion years ago, when they were all together in one singular extremely dense
place. This discovery brought the concept of the beginning of the universe
within the province of science. Today, scientists use two partial theories,
Einstein's general theory of relativity and quantum mechanics, to describe the
workings of the universe. Scientists are still looking for a complete unified
theory that would describe everything in the universe. Hawking believes that
the search for such a universal theory, even though motivated by the essential
human need for logic, order and understanding, might affect the survival of the
human species.
In the first chapter, Hawking discusses the history of
astronomical studies, including the ideas of Aristotle and Ptolemy. Aristotle,
unlike many other people of his time, thought that the Earth was round. He came
to this conclusion by observing lunar eclipses, which he thought were caused by
the earth's round shadow, and also by observing an increase in altitude of the
North Star from the perspective of observers situated further to the north.
Aristotle also thought that the sun and stars went around the Earth in perfect
circles, because of "mystical reasons". Second-century Greek
astronomer Ptolemy also pondered the positions of the sun and stars in the
universe and made a planetary model that described Aristotle's thinking in more
detail.
Editions:
1988: The first edition included an introduction by Carl
Sagan that tells the following story: Sagan was in London for a scientific
conference in 1974, and between sessions he wandered into a different room,
where a larger meeting was taking place. "I realized that I was watching
an ancient ceremony: the investiture of new fellows into the Royal Society, one
of the most ancient scholarly organizations on the planet. In the front row, a
young man in a wheelchair was, very slowly, signing his name in a book that
bore on its earliest pages the signature of Isaac Newton... Stephen Hawking was
a legend even then." In his introduction, Sagan goes on to add that
Hawking is the "worthy successor" to Newton and Paul Dirac, both
former Lucasian Professors of Mathematics.
The introduction was removed after the first edition, as it
was copyrighted by Sagan, rather than by Hawking or the publisher, and the
publisher did not have the right to reprint it in perpetuity. Hawking wrote his
own introduction for later editions.
1996, Illustrated, updated and expanded edition: This
hardcover edition contained full-color illustrations and photographs to help
further explain the text, as well as the addition of topics that were not
included in the original book.
1998, Tenth-anniversary edition: It features the same text as
the one published in 1996, but was also released in paperback and has only a
few diagrams included. ISBN 0553109537
2005, A Briefer History of Time: a collaboration with Leonard
Mlodinow of an abridged version of the original book. It was updated again to
address new issues that had arisen due to further scientific development. ISBN
0-553-80436-7
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