The Measurement of Starlight: Two Centuries of Astronomical Photometry

The Measurement of Starlight: Two Centuries of Astronomical Photometry

by J. B. Hearnshaw
ISBN-10:
0521403936
ISBN-13:
9780521403931
Pub. Date:
05/02/1996
Publisher:
Cambridge University Press
ISBN-10:
0521403936
ISBN-13:
9780521403931
Pub. Date:
05/02/1996
Publisher:
Cambridge University Press
The Measurement of Starlight: Two Centuries of Astronomical Photometry

The Measurement of Starlight: Two Centuries of Astronomical Photometry

by J. B. Hearnshaw
$205.0
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Overview

Astronomical photometry is the science of measuring the brightness and colors of stars and other celestial objects. This authoritative volume traces the fascinating historical development of astronomical photometry from visual techniques at the time of William Herschel in the 1780s to the birth of photometry with charge-coupled devices in the 1970s. In this intriguing survey, the author shows how the advent of new technology has revolutionized the science of photometry at each stage of its development, and what dramatic advances have been achieved despite several major disasters—especially in the practice of photographic photometry. This book also clearly illustrates the critical relationship between the development of a science and the technology it uses.

Product Details

ISBN-13: 9780521403931
Publisher: Cambridge University Press
Publication date: 05/02/1996
Pages: 526
Product dimensions: 6.14(w) x 9.21(h) x 1.14(d)

Table of Contents

Preface; Acknowledgements; List of illustrations; 1. Early stellar magnitudes; 2. Visual estimates of stellar magnitudes and colour; 3. Visual photometry; 4. Photographic photometry, 1839–1922; 5. The origins of photoelectric photometry; 6. Photometry at longer wavelengths; 7. Photographic photometry from 1922; 8. Photometry and the birth of astrophysics; 9. Photoelectric photometry with the photomultiplier tube; 10. Photometry with electronic area detectors; Sources of illustrations; Index of names; Index of star names; Index of subjects.
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