: Keith Robinson
: Starlight An Introduction to Stellar Physics for Amateurs
: Springer-Verlag
: 9781441907080
: 1
: CHF 42.70
:
: Astronomie: Allgemeines, Nachschlagewerke
: English
: 273
: Wasserzeichen/DRM
: PC/MAC/eReader/Tablet
: PDF

This is a book about the physics of stars and starlight. The story of starlight is truly fascinating. Astronomers analyze and interpret the light from stars using photometry and spectroscopy, then inspirational detective work combines with the laws of physics to reveal the temperatures, masses, luminosities and outer structure of these far away points of light. The laws of physics themselves enable us to journey to the very center of a star and to understand its inner structure and source of energy!

Starlight provides an in-depth study of stellar astrophysics that requires only basic high school mathematics and physics, making it accessible to all amateur astronomers. Starlight teaches amateur astronomers about the physics of stars and starlight in a friendly, easy-to-read way. The reader will take away a profoundly deeper understanding of this truly fascinating subject - and find his practical observations more rewarding and fulfilling as a result.

Acknowledgements5
Contents6
About the Author7
A River of Starlight8
Starlight by Numbers13
Large Numbers and Small Numbers14
The Rule of Indices15
The Rule of Indices for All Indices17
Working with Powers of Ten18
Scientific Notation19
Star Distances by Numbers22
Key Points27
From Light to Starlight29
Let There Be (an Idea About) Light30
Natures Color Palette The Electromagnetic Spectrum36
How to Measure the Wavelength of Light40
The Spectrum, the Whole Spectrum, and Nothing but the Spectrum43
A Brief Note on the Spectroscope45
Light and Energy46
Let There Be Another Idea About Light48
The Parable of the Two Tables Blackbody Radiation52
The Blackbody Spectrum57
The Parable of the Blackbody and the Star60
Key Points62
Space -- The Great Radiation Field64
Rivers of Energy64
Measuring the Radiation Field65
Sunlight Is Intense But Starlight Is Not 70
How Many Light Bulbs Must You Screw in to Make a Star?72
From Flux to Flux Ratio to Magnitude 78
How to Calculate Magnitudes82
Fixing the Magnitude Scale84
Absolute Magnitude A Measure of Stellar Luminosity86
Key Points89
A Multitude of Magnitudes for the Colors of Starlight91
Blackbody Stars64
From Theories of Physics to Astronomical Observations65
Star Partners Color and Magnitude70
Color and Blackbody Temperature72
Measuring Effective Temperatures for Real Stars78
Yet Another Magnitude82
Sorting Out Stellar Spectra84
The HertzsprungRussell Diagram86
Using the HR Diagram Template89
A Different Kind of HR Diagram117
Conclusion118
Key Points119
The Photons Must Get Through -- Radiative Transfer122
Absorption The Photons Get Taken Out64
The Photon Gets a Second Chance (and Maybe More) Scattering65
New Photons for Old Emission70
Symbiotic Nebulae An Illustration of Optical Depth in Action72
Key Points78
First Look Inside a Star -- The Atmosphere147
Simple Radiative Transfer in the Photosphere64
The Chromosphere and the Corona 65
Yet Another Kind of HR Diagram70
A Photosphere Full of Hydrogen Atoms72
The Hydrogen Absorption Lines78
The Ups and Downs of a Hydrogen Atom82
The Ups and Downs of a Hydrogen Atom in a Photosphere84
The Temperature of Vega86
Return to the ColorColor Diagram89
Model Atmospheres for Stars117
Key Points118
Deep Inside a Star176
Hot Gas The Basics64
From a Cylinder of Gas to the Structure of a Star65
The Principles of Stellar Structure70
From a Cylinder of Gas to Stellar Pulsation72
Cepheid Variable Stars The Other Story78
How to Make a Star Pulsate82
Yet Another Gas Cylinder Experiment84
Exciting Stellar Pulsation86
The Right Kind of Gas in the Right Kind of Star89
Details, Details117
From a Cylinder of Gas to a Red Giant Star118
Convection in Stars119
The Stellar Core Source of the River of Starlight207
Nuclear Fusion in Stars The Details210
The CNO Cycle213
Key Points214
In the Space Between Stars216
Winds from the Stars64
Stardust65
When the Galaxy Shrank70
Space Dust72
The Dimming of Starlight78
Through the Atmosphere82
Key Points84
A Star Story 0 10 Billion Years in the Making 235
The Middle of the Story Life on the Main Sequence235
The Beginning of the Story From Atoms to Stars239
The End of the Story Life After the Main Sequence245
Stellar Evolution in Action253
Old Stars, Young Stars, and New Stars from Old257
The Legacy of Starlight259
Conclusion260
Key Points262
Appendix 1: The Greek Alphabet264
Appendix 2: Astronomical and Physical Units and Constants265
Important Units266
Constants267
Physical Constants267
Astronomical Constants267
Appendix 3: The Doppler Effect268
Index270