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Comment: Publisher: Dover Publications
Date of Publication: 2004
Binding: paperback
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Aristarchus of Samos: The Ancient Copernicus (Dover Books on Astronomy) Paperback – December 9, 2004


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Editorial Reviews

About the Author

Thomas Little Heath: Bringing the Past to Life
Thomas Little Heath (1861–1940) was unusual for an authority on many esoteric, and many less esoteric, subjects in the history of mathematics in that he was never a university professor. The son of an English farmer from Lincolnshire, Heath demonstrated his academic gifts at a young age; studied at Trinity College, Cambridge, from 1879 to 1882; came away with numerous awards; and obtained the top grade in the 1884 English Civil Service examination. From that foundation, he went to work in the English Treasury, rose through the ranks, and by 1913, was permanent secretary to the Treasury, effectively the head of its operations. He left that post in 1919 at the end of the first World War, worked several years at the National Debt office, and retired in 1926.

During all of that time, however, he became independently one of the world's leading authorities on the history of mathematics, especially on the history of ancient Greek mathematics. Heath's three-volume edition of Euclid is still the standard, it is generally accepted that it is primarily through Heath's great work on Archimedes that the accomplishments of Archimedes are known as well as they are.

Dover has reprinted these and other books by Heath, preserving over several decades a unique legacy in the history of mathematical scholarship.

In the Author's Own Words:
"The works of Archimedes are without exception, monuments of mathematical exposition; the gradual revelation of the plan of attack, the masterly ordering of the propositions, the stern elimination of everything not immediately relevant to the purpose, the finish of the whole, are so impressive in their perfection as to create a feeling akin to awe in the mind of the reader." — Thomas L. Heath

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Product Details

  • Series: Dover Books on Astronomy
  • Paperback: 448 pages
  • Publisher: Dover Publications (December 9, 2004)
  • Language: English
  • ISBN-10: 0486438864
  • ISBN-13: 978-0486438863
  • Product Dimensions: 8.5 x 5.5 x 0.9 inches
  • Shipping Weight: 1.1 pounds (View shipping rates and policies)
  • Average Customer Review: 5.0 out of 5 stars  See all reviews (4 customer reviews)
  • Amazon Best Sellers Rank: #1,002,095 in Books (See Top 100 in Books)

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20 of 20 people found the following review helpful By Einsteinian on July 2, 2006
Format: Paperback
This old (early twentieth century) book is not just about Aristarchus, the "Greek Copernicus" -- that comes in the final chapters. Rather, it is the best survey I know of ancient Greek astronomy, starting from the very beginning. I kept coming across references to this book by Sir Thomas Heath in books on the Copernican revolution, e.g. those by Angus Armitage and Thomas Kuhn, and finally decided to read it -- after having bought his smaller volume on Greek astronomy, also reprinted by Dover.

Heath really goes into detail on each of the ancient schools of astronomy in Greece. There were in fact a good many points of view -- the earth-centered view, the view that the earth rotates daily about its axis, the view of everything going around a fiery center, the "concentric spheres" variant of Eudoxus of the earth centered view, the Aristotelian variant of that, the eventual Ptolemaic view of epicycles and all that ... and finally the view of Aristarchus, which was essentially the Copernican sun-centered view (but without Copernicus' marvelous insights into how such a view simplified everything).

Heath not only goes into detail about each of these schools of thought -- it can be pretty rough going trying to follow all of this, especially because of the esoteric modes of speaking they often employed -- he also gives pithy summaries of what each school was saying, and a critical evaluation of their worth and influence.

If you really want to gain an appreciation of the variety of the ancient Greek schools of thought, of their struggle and progress over seven centuries in describing the motions in the heavens, of the reasonableness of much of their thinking, of the magnificence of their achievement -- I heartily recommend this book, then I recommend, either before or after, exploring the Copernican revolution and the rest of the scientific revolution, in the books by Armitage, Kuhn, Hall, and others.
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13 of 13 people found the following review helpful By thoughtful reader on May 20, 2008
Format: Paperback
Thomas Heath published this book in 1913. As he explains, he was first motivated by a request from a friend to produce a translation of Aristarchus's treatise "On the sizes and distances of the sun and the moon." In that book Aristarchus does not say anything about heliocentrism or the motion of the earth, but we know from ancient reports that he was an early heliocentrist, probably the first. However, at the time Heath wrote this, the definitive studies of ancient heliocentrism and the earth's motion had been written by Schiaparelli, who insisted that Aristarchus had been anticipated by Heraclides Ponticus. (Yes, Schiaparelli was the astronomer who found "canali" on Mars!) Heath took the opportunity to set the record straight, and ended up writing a fantastic study of Greek astronomy up to Aristarchus in the 3rd century BC. The book is nearly a hundred years old, so don't rely on it as your only source if you want a detailed up-to-date picture of early astronomy. (If that's what you want, start with James Evans's "History and Practice of Ancient Astronomy" and work from the footnotes.) But this is a real classic, constantly cited by later authors, and more readable than a lot of what you will find written on Greek astronomy. Heath's translation of Aristarchus's work, at the back of the book, became the definitive English translation.

If you want to know more about what the Greeks did after Aristarchus, I recommend, in addition to Evans's book mentioned above, JLE Dreyer's "A History of Astronomy from Thales to Kepler," another classic survey from about the same time.
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4 of 5 people found the following review helpful By Viktor Blasjo on May 15, 2010
Format: Paperback
Although this book contains much historical background, the highlight, in my opinion, is the complete translation of Aristarchus' only extant work, On the distances and sizes of the sun and moon (c. -270). I am going to summarise this work here. My summary will contain all the main results of the treatise, and indicate what is essentially Aristarchus' derivations. However, my summary will be a simplification in that I will assume that the sun lights up exactly half the moon, whereas Aristarchus knows that this is not quite true and so has a small correction factor in the calculations to account for this.

I will use this notation: E, M, S are the centers of the earth, moon and sun respectively, and E', M', S' are points on their apparent perimeters.

The ratio of the distances from the earth to the moon and from the earth to the sun can be determined by measuring the angle MES at half moon. For at half moon the angle EMS=90° and the angle MES is measurable, so we know all angles of this triangle and thus the ratios of its sides.

The ratio of the sizes of the moon and the sun can then be inferred at a solar eclipse. For at a solar eclipse, the moon precisely covers the sun. Thus EMM' is similar to ESS', with the scaling factor discovered above, i.e. SS':MM'::ES:EM.

The ratio of the distance of the moon to its size can be inferred from its angular size. For the angle EMM'=90° and the angle MEM' is measurable, so we know all angles of this triangle and thus the ratios of its sides.

These distances can be related to the radius of the earth at a lunar eclipse. For the shadow that the earth casts on the moon is about two moon-diameters wide.
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