To Explain the World: The Discovery of Modern Science (76 page)

BOOK: To Explain the World: The Discovery of Modern Science
7Mb size Format: txt, pdf, ePub

Photo by Matt Valentine

STEVEN WEINBERG
is a theoretical physicist and winner of the Nobel Prize in Physics, the National Medal of Science, the Lewis Thomas Prize for the Scientist as Poet, and numerous honorary degrees and other awards. He is a member of the National Academy of Science, the Royal Society of London, the American Philosophical Society, and other academies. A longtime contributor to
The New York Review of Books
, he is the author of
The First Three Minutes, Dreams of a Final Theory, Facing Up
, and
Lake Views
, as well as leading treatises in theoretical physics. He holds the Josey Regental Chair in Science at the University of Texas at Austin.

Discover great authors, exclusive offers, and more at
hc.com
.

Also by Steven Weinberg

Lectures on Quantum Mechanics

Lake Views

Cosmology

Glory and Terror

Facing Up

The Quantum Theory of Fields

Dreams of a Final Theory

Elementary Particles and the Laws of Physics

The Discovery of Subatomic Particles

The First Three Minutes

Gravitation and Cosmology

Credits

COVER DESIGN BY MILAN BOZIC

COVER PHOTOGRAPHS: © DAVID BUKACH/
GETTY IMAGES (CONSTELLATION MAP);
© SHEILA TERRY/GETTY IMAGES (EYE)

Illustrations by Ron Carboni

Copyright

TO EXPLAIN THE WORLD.
Copyright © 2015 by Steven Weinberg. All rights reserved under International and Pan-American Copyright Conventions. By payment of the required fees, you have been granted the nonexclusive, nontransferable right to access and read the text of this e-book on-screen. No part of this text may be reproduced, transmitted, downloaded, decompiled, reverse-engineered, or stored in or introduced into any information storage and retrieval system, in any form or by any means, whether electronic or mechanical, now known or hereafter invented, without the express written permission of HarperCollins e-books.

FIRST EDITION

Library of Congress Cataloging-in-Publication Data has been applied for.

ISBN: 978-0-06-234665-0

EPub Edition February 2015 ISBN 9780062346674

15 16 17 18 19  
DIX
/
RRD
  10 9 8 7 6 5 4 3 2 1

About the Publisher

Australia

HarperCollins Publishers Australia Pty. Ltd.

Level 13, 201 Elizabeth Street

Sydney, NSW 2000, Australia

www.harpercollins.com.au

Canada

HarperCollins Canada

2 Bloor Street East - 20th Floor

Toronto, ON M4W 1A8, Canada

www.harpercollins.ca

New Zealand

HarperCollins Publishers New Zealand

Unit D1 63 Apollo Drive

Rosedale 0632

Auckland, New Zealand

www.harpercollins.co.nz

United Kingdom

HarperCollins Publishers Ltd.

1 London Bridge Street

London SE1 9GF, UK

www.harpercollins.co.uk

United States

HarperCollins Publishers Inc.

195 Broadway

New York, NY 10007

www.harpercollins.com

*
As pointed out by Gregory Vlastos, in
Plato’s Universe
(University of Washington Press, Seattle, 1975), an adverbial form of the word
kosmos
was used by Homer to mean “socially decent” and “morally proper.” This use survives in English in the word “cosmetic.” Its use by Heraclitus reflects the Hellenic view that the world is pretty much what it should be. The word appears in English also in the cognates “cosmos” and “cosmology.”

*
In fact (as discussed in Technical Note 2), whatever may have been proved by Theaetetus,
Elements
does not prove what it claims to prove, that there are only five possible convex regular solids.
Elements
does prove that for regular polyhedrons, there are just five combinations of the number of sides of each face of a polyhedron and of the number of faces that meet at each vertex, but it does not prove that for each combination of these numbers there is just one possible convex regular polyhedron.

*
The Greek word
kineson
, which is usually translated as “motion,” actually has a more general significance, referring to any sort of change. Thus Aristotle’s classification of types of cause applied not only to change of position, but to any change. The Greek word
fora
refers specifically to change of location, and is usually translated as “locomotion.”

*
It was generally supposed in the ancient world that when we see something the light travels from the eye to the object, as if vision were a sort of touching that requires us to reach out to what is seen. In the following discussion I will take for granted the modern understanding, that in vision light travels from the object to the eye. Fortunately, in analyzing reflection and refraction, it makes no difference which way the light is going.

*
The Assayer
is a polemic against Galileo’s Jesuit adversaries, taking the form of a letter to the papal chamberlain Virginio Cesarini. As we will see in
Chapter 11
, Galileo in
The Assayer
was attacking the correct view of Tycho Brahe and the Jesuits that comets are farther from Earth than the Moon is. (The quotation here is taken from the translation by Maurice A. Finocchiaro, in
The Essential Galileo
, Hackett, Indianapolis, Ind., 2008, p. 183.)

*
Pierre Gassendi was a French priest and philosopher who tried to reconcile the atomism of Epicurus and Lucretius with Christianity.

*
To be more precise, this is known as the “synodic” lunar month. The 27-day period for the Moon to return to the same position relative to the fixed stars is known as the “sidereal” lunar month.

*
This does not happen every month, because the plane of the orbit of the Moon around the Earth is slightly tilted with respect to the plane of the orbit of the Earth around the Sun. The Moon crosses the plane of the Earth’s orbit twice every sidereal month, but this happens at full moon, when the Earth is between the Sun and the Moon, only about once every 18 years.

*
The equinox is the moment when the Sun in its motion against the background of stars crosses the celestial equator. (In modern terms, it is the moment when the line between the Earth and the Sun becomes perpendicular to the Earth’s axis.) At points on the Earth with different longitude, this moment occurs at different times of day, so there may be a one-day difference in the date that different observers report the equinox. Similar remarks apply to the phases of the Moon.

*
It has been argued (in O. Neugebauer,
A History of Ancient Mathematical Astronomy
, Springer-Verlag, New York, 1975, pp. 1093–94), that Aristotle’s reasoning about the shape of the Earth’s shadow on the Moon is inconclusive, since an infinite variety of terrestrial and lunar shapes would give the same curved shadow.

*
Samuel Eliot Morison cited this argument in his biography of Columbus (
Admiral of the Ocean Sea
, Little Brown, Boston, Mass., 1942) to show, contrary to a widespread supposition, that it was well understood before Columbus set sail that the Earth is a sphere. The debate in the court of Castile over whether to support the proposed expedition of Columbus concerned not the shape of the Earth, but its
size
. Columbus thought the Earth was small enough so that he could sail from Spain to the east coast of Asia without running out of food and water. He was wrong about the size of the Earth, but of course was saved by the unexpected appearance of America between Europe and Asia.

*
There is a fascinating remark by Archimedes in
The Sand Reckoner
, that Aristarchus had found that the “Sun appeared to be about
1
/
720
part of the zodiac” (
The Works of Archimedes
, trans. T. L. Heath, Cambridge University Press, Cambridge, 1897, p. 223). That is, the angle subtended on Earth by the disk of the Sun is
1
/
720
times 360°, or 0.5°, not far from the correct value 0.519°. Archimedes even claimed that he had verified this by his own observations. But as we have seen, in his surviving work Aristarchus had given the angle subtended by the disk of the Moon the value 2°, and he had noted that the disks of the Sun and Moon have the same apparent size. Was Archimedes quoting a later measurement by Aristarchus, of which no report has survived? Was he quoting his own measurement, and attributing it to Aristarchus? I have heard scholars suggest that the source of the discrepancy is a copying error or a misinterpretation of the text, but this seems very unlikely. As already noted, Aristarchus had concluded from his measurement of the angular size of the Moon that its distance from the Earth must be between 30 and
45
/
2
times greater than the Moon’s diameter, a result quite incompatible with an apparent size of around 0.5°. Modern trigonometry tells us on the other hand that if the Moon’s apparent size were 2°, then its distance from the Earth would be 28.6 times its diameter, a number that is indeed between 30 and
45
/
2
. (The Sand Reckoner is not a serious work of astronomy, but a demonstration by Archimedes that he could calculate very large numbers, such as the number of grains of sand needed to fill the sphere of the fixed stars.)

*
There is a famous ancient device known as the Antikythera Mechanism, discovered in 1901 by sponge divers off the island of Antikythera, in the Mediterranean between Crete and mainland Greece. It is believed to have been lost in a shipwreck sometime around 150 to 100 BC. Though the Antikythera Mechanism is now a corroded mass of bronze, scholars have been able to deduce its workings by X-ray studies of its interior. Apparently it is not an orrery but a calendrical device, which tells the apparent position of the Sun and planets in the zodiac on any date. The most important thing about it is that its intricate gearwork provides evidence of the high competence of Hellenistic technology.

*
The celestial latitude is the angular separation between the star and the ecliptic. While on Earth we measure longitude from the Greenwich meridian, the celestial longitude is the angular separation, on a circle of fixed celestial latitude, between the star and the celestial meridian on which lies the position of the Sun at the vernal equinox.

*
On the basis of his own observations of the star Regulus, Ptolemy in
Almagest
gave a figure of 1° in approximately 100 years.

*
Eratosthenes was lucky. Syene is not precisely due south of Alexandria (its longitude is 32.9° E, while that of Alexandria is 29.9° E) and the noon Sun at the summer solstice is not precisely overhead at Syene, but about 0.4° from the vertical. The two errors partly cancel. What Eratosthenes had really measured was the ratio of the circumference of the Earth to the distance from Alexandria to the Tropic of Cancer (called the summer tropical circle by Cleomedes), the circle on the Earth’s surface where the noon Sun at the summer solstice really is directly overhead. Alexandria is at a latitude of 31.2°, while the latitude of the Tropic of Cancer is 23.5°, which is less than the latitude of Alexandria by 7.7°, so the circumference of the Earth is in fact 360°/7.7° = 46.75 times greater than the distance between Alexandria and the Tropic of Cancer, just a little less than the ratio 50 given by Eratosthenes.

*
For the sake of clarity, when I refer to planets in this chapter, I will mean just the five: Mercury, Venus, Mars, Jupiter, and Saturn.

*
We can see the correspondence of days of the week with planets and the associated gods in the names of the days of the week in English. Saturday, Sunday, and Monday are obviously associated with Saturn, the Sun, and the Moon; Tuesday, Wednesday, Thursday, and Friday are based on an association of Germanic gods with supposed Latin equivalents: Tyr with Mars, Wotan with Mercury, Thor with Jupiter, and Frigga with Venus.

Other books

Learn to Fly by Heidi Hutchinson
Chameleon Wolf by Glenn, Stormy, Flynn, Joyee
Historia de la vida del Buscón by Francisco de Quevedo
Whisper by Kathleen Lash
Deep Summer by Gwen Bristow
SEARCH FOR THE LOST SOUL by McKinsey, Kattie
Nightingale by Aleksandr Voinov
Homer’s Daughter by Robert Graves
The Key by Marianne Curley