Book contents
- Frontmatter
- Contents
- Foreword
- Preface
- I Survey of the Problem
- II Thermodynamics of Radiation
- III Quantum Theory
- IV Polytropic Gas Spheres
- V Radiative Equilibrium
- VI Solution of the Equations
- VII The Mass-Luminosity Relation
- VIII Variable Stars
- IX The Coefficient of Opacity
- X Ionisation, Diffusion, Rotation
- XI The Source of Stellar Energy
- XII The Outside of a Star
- XIII Diffuse Matter in Space
- APP. I Physical and Astronomical Constants
- APP. II References
- INDEX
I - Survey of the Problem
Published online by Cambridge University Press: 01 June 2011
- Frontmatter
- Contents
- Foreword
- Preface
- I Survey of the Problem
- II Thermodynamics of Radiation
- III Quantum Theory
- IV Polytropic Gas Spheres
- V Radiative Equilibrium
- VI Solution of the Equations
- VII The Mass-Luminosity Relation
- VIII Variable Stars
- IX The Coefficient of Opacity
- X Ionisation, Diffusion, Rotation
- XI The Source of Stellar Energy
- XII The Outside of a Star
- XIII Diffuse Matter in Space
- APP. I Physical and Astronomical Constants
- APP. II References
- INDEX
Summary
1. At first sight it would seem that the deep interior of the sun and stars is less accessible to scientific investigation than any other region of the universe. Our telescopes may probe farther and farther into the depths of space; but how can we ever obtain certain knowledge of that which is hidden behind substantial barriers? What appliance can pierce through the outer layers of a star and test the conditions within?
The problem does not appear so hopeless when misleading metaphor is discarded. It is not our task actively to “probe”; we learn what we do learn by awaiting and interpreting the messages dispatched to us by the objects of nature. And the interior of a star is not wholly cut off from such communication. A gravitational field emanates from it, which substantial barriers cannot appreciably modify; further, radiant energy from the hot interior after many deflections and transformations manages to struggle to the surface and begin its journey across space. From these two clues alone a chain of deduction can start, which is perhaps the more trustworthy because it is only possible to employ in it the most universal rules of nature—the conservation of energy and momentum, the laws of chance and averages, the second law of thermodynamics, the fundamental properties of the atom, and so on. There is no more essential uncertainty in the knowledge so reached than there is in most scientific inferences.
- Type
- Chapter
- Information
- The Internal Constitution of the Stars , pp. 1 - 26Publisher: Cambridge University PressPrint publication year: 1988