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Index
Cover Page
Title Page
Copyright Page
Contents
About the Author
Acknowledgements
List of Illustrations
Introduction: The Most Important Fact
Part Zero: Prologue
2.712 – Taking the temperature of the Universe
Part One: How Do We Know the Ages of Stars?
1 2.898 – Prehistory: Spectra and the nature of stars
Locating lines
Hunting helium
Hunting hydrogen
The heat of the Sun
The heat of the stars
The heat inside
2 0.008 – At the heart of the Sun
A French connection
No free lunch
Seats of enormous energies
A hotter place?
A quantum of solace
3 7.65 – Making ‘metals’
Cycles and chains of fusion
Rocks of ages
From the Bomb to the stars
The last should be first
Stardust
4 13.2 – The ages of stars
Hertzsprung, Russell and the diagram
Ashes to ashes
Globular cluster ages
White dwarf ages
Radiometric ages and the oldest known star
Part Two: How Do We Know the Age of the Universe?
5 31.415 – Prehistory: Galaxies and the Universe at large
The power of pure reason
One step forward, two steps back
Nebular spectroscopy
First steps
The long and winding road
An unresolved debate
A universe destroyed
6 575 – The discovery of the expanding Universe
Surprising speeds
Taking the credit
A Russian revolution
A Priestly intercession
7 75 – Sizing up the cosmic soufflé
Einstein’s lost model
Keeping it simple
Across the Universe
Doubling the distances
Hubble’s heir
Another Great Debate
8 13.8 – Surveys and satellites
The culmination of a tradition
Too perfect?
The dark side
Supernovae and superexpansion
Sounding out the Universe
Ultimate truth
Glossary
Sources and Further Reading
End Notes
Index
Footnotes
Prologue
Chapter 1
Chapter 2
Chapter 3
Chapter 4
Chapter 5
Chapter 6
Chapter 7
Chapter 8
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