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Farndon - The science book

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Farndon The science book
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London New York Melbourne Munich and Delhi Project art editor - Katie - photo 1
London New York Melbourne Munich and Delhi Project art editor - Katie - photo 2
London, New York, Melbourne, Munich, and Delhi
Project art editor - Katie Cavanagh
Senior Editor - Georgina Palffy
Managing art Editor - Lee Griffiths
Managing Editor - Stephanie Farrow
Publishing Director - Jonathan Metcalf
Art Director - Phil Ormerod
Publisher - Andrew Macintyre
Jacket Designer - Laura Brim
Jacket Editor - Maud Whatley
Jacket Design Development Manager - SophiaMTT
Pre-production Producer - Adam Stoneham
Producer - Mandy Inness
Illustrations - James Graham, Peter Liddiard
produced for DK by - TALLTREE LTD
Editors - Rob Colson, Camilla Hallinan, DavidJohn
Design and Art Direction - Ben Ruocco
- DK Digital Publishing Team
Senior Digital Producer - Miguel Cunha
Head of Digital Media, Delhi - Manjari Hooda
Senior Editorial Manager - Lakshmi Rao
Editor - Srishti Malasi
Technical Manager - Gaurav Gupta
Software Engineer - Punkaj Vaid
Digital Design Manager - Nain Rawat
Senior Digital Designer - Susant Pati
Operations Assistant - Tauhid Nasir
- DK Delhi
Project Editor - Priyaneet Singh
Assistant Art Editor - Vidit Vashisht
DTP Designer - Jaypal Chauhan
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Managing Art Editor - Govind Mittal
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original styling by - STUDIO 8
First published in Great Britain in 2014 by Dorling Kindersley Limited, 80 Strand,London, WC2R 0RL
A Penguin Random House Company
2 4 6 8 10 9 7 5 3 1 - 001 - 192893 - Aug/2014
Copyright 2014 Dorling Kindersley Limited
All rights reserved. No part of this publication may be reproduced, stored in aretrieval system, or transmitted in any form or by any means, electronic,mechanical, photocopying, recording, or otherwise, without the prior writtenpermission of the copyright owner.
A CIP catalogue record for this book is available from the British Library.
ISBN: 9781409350156
This digital edition published 2015 - ISBN: 9780241202364
Discover more at www.dk.com
INTRODUCTION Science is an ongoing search for truth a perpetual struggle to - photo 3
INTRODUCTION

Science is an ongoing search for truth a perpetual struggle to discoverhow the Universe works that goes back to the earliest civilizations. Driven by humancuriosity, it has relied on reasoning, observation, and experiment. The best known ofthe ancient Greek philosophers, Aristotle, wrote widely on scientific subjects and laidfoundations for much of the work that has followed. He was a good observer of nature,but he relied entirely on thought and argument, and did no experiments. As a result, hegot a number of things wrong. He asserted that big objects fall faster than little ones,for example, and that if one object had twice the weight of another, it would fall twiceas fast. Although this is mistaken, no one doubted it until the Italian astronomerGalileo Galilei disproved the idea in 1590. While it may seem obvious today that a goodscientist must rely on empirical evidence, this was not always apparent.

The scientific method

A logical system for the scientific process was first put forward by theEnglish philosopher Francis Bacon in the early 17th century. Building on thework of the Arab scientist Alhazen 600 years earlier, and soon to be reinforcedby the French philosopher Ren Descartes, Bacons scientific method requiresscientists to make observations, form a theory to explain what is going on, andthen carry out an experiment to see whether the theory works. If it seems to betrue, then the results may be sent out for peer review, in which people workingin the same or a similar field are invited to pick holes in the argument, and sofalsify the theory, or to repeat the experiment to make sure that the resultsare correct.

Making a testable hypothesis or a prediction is always useful. Englishastronomer Edmond Halley, observing the comet of 1682, realized that it wassimilar to comets reported in 1531 and 1607, and suggested that all three werethe same object, in orbit round the Sun. He predicted that it would return in1758, and he was right, though only just it was spotted on 25 December. Today,the comet is known as Halleys Comet. Since astronomers are rarely able toperform experiments, evidence can come only from observation.

Experiments may test a theory, or be purely speculative. When the NewZealand-born physicist Ernest Rutherford watched his students fire alphaparticles at gold leaf in a search for small deflections, he suggested puttingthe detector beside the source, and to their astonishment some of the alphaparticles bounced back off the paper-thin foil. Rutherford said it was as thoughan artillery shell had bounced back off tissue paper and this led him to a newidea about the structure of the atom.

An experiment is all the more compelling if the scientist, while proposing anew mechanism or theory, can make a prediction about the outcome. If theexperiment produces the predicted result, the scientist then has supportingevidence for the theory. Even so, science can never prove that a theory iscorrect; as the 20th-century philosopher of science Karl Popper pointed out, itcan only disprove things. Every experiment that gives predicted answers issupporting evidence, but one experiment that fails may bring an entire theorycrashing down.

Over the centuries, long-held concepts such as a geocentric Universe, the fourbodily humours, the fire-element phlogiston, and a mysterious medium calledaether have all been disproved and replaced with new theories. These in turn areonly theories, and may yet be disproved, although in many cases this is unlikelygiven the evidence in their support.

"All truths are easy to understand once they are discovered; the point isto discover them."

Galileo Galilei

Progression of ideas

Science rarely proceeds in simple, logical steps. Discoveries may be madesimultaneously by scientists working independently, but almost every advancedepends in some measure on previous work and theories. One reason for buildingthe vast apparatus known as the Large Hadron Collider, or LHC, was to search forthe Higgs particle, whose existence was predicted 40 years earlier, in 1964.That prediction rested on decades of theoretical work on the structure of theatom, going back to Rutherford and the work of Danish physicist Niels Bohr inthe 1920s, which depended on the discovery of the electron in 1897, which inturn depended on the discovery of cathode rays in 1869. Those could not havebeen found without the vacuum pump and, in 1799, the invention of the battery and so the chain goes back through decades and centuries. The great Englishphysicist Isaac Newton famously said, If I have seen further, it is by standingon the shoulders of giants. He meant primarily Galileo, but he had probablyalso seen a copy of Alhazens Optics

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