E-Book Overview
In this small book an attempt has been made to set forth the distinguishing features of the chemical phenomena characteristic of outer space. We have allotted special attention to the theoretical and experimental methods of investigation of space, avoiding however, repetition of the material contained in school courses of physics and chemistry. At the same time, striving to make the book as popular as possible, we confined ourselves only to the most essential information concerning the nature of the atomic nucleus, the laws of nuclear energetics, the origin of various kinds of spectra, etc. The scope of the knowledge of physics, chemistry and mathematics given at our secondary schools is quite sufficient for understanding this book.
The textbook is designed for upper grade students of secondary schools. It contains information about the chemical composition of the planets of solar system, meteorites, the Sun, about synthesis of elements on the stars, the methods of studying space chemistry, as well as catalytic nature of nuclear processes.
The author describes the behaviour of substances at very high and very low temperatures and pressures, considers the possibility of the formation of organic compounds in outer space and in pre-biological period on Earth.
E-Book Content
JI. A. HlIKOJIaeB XlfMIIH KOCMOCA
M3AaTeJlLCTBO
«11 pOCBe~eHHe» MOCKB8
Space Chemistry L. NIKOLAEV
Translated from the Russian by Y. NADLER
l\1ir Publishers Moscow
Aa B~
ry
f16
EB Z~
Hl1 8,e)
Alpha Beta Gamma Delta Epsilon Zeta Eta Theta
The Greek Alphabet Iota I .. Kx Kappa AA Lambda MJ.t Mu Nv Nu Xi 8~ 00 Omicron TIn Pi
First published 1976 Revised from the 1974 Russian edition
Pp ~(J'
T't
r"
(1)cp
Xx '1''1' Qoo
Rho Sigma Tau Upsilon Phi Chi Psi Omega
© English translation, Mir Publishers, 1976
CONTENTS
From the Author Chapter I. Research Methods Used in Space Chemistry 1. Light Rays and Chemical Composition 2. "Optical Specifications" of an Atom 3. Cosmic Matter on the Earth 4. Analytical Procedures and Techniques
7 12 12 16 24 29
Chapter II. Chemical Composition of Celestial Bodies. The Solar System 1. Meteorites . . 2. Chemistry of the Solar System 3. The Sun and Planets of the Solar System 4. The Planets
53 56 65
Chapter III. Scope of Earth and Space Chemistry
94
1. G e n e r a l . . . 2. What Happens to Matter at High Pressure 3. What Happens to Matter at High Temperatures
4. Plasma State of Matter Chapter IV. The World of Stars 1. Brightness and Luminosity of Stars . . . . . 2. The Hertzsprung-Russell (HR) Diagram and Stellar Evolution ..... 3. Chemical Composition of Stars 4. Stellar Atmospheres. Light and Gravitation 5. Novae . 6. Supernovae 7. Comets • . .
37
37
94 97 100 103
107 107
108 112 120 123 126
127
5
Chapter V. Nuclear Reactions and Sources of Stellar Energy 1. Constituents of the Atomic Nucleus . 2. Properties of Some Elementary Particles 3. Nuclear Reactions 4. Nuclear Energy Sources 5. Types of Nuclear Reactions 6. Sources of Solar Energy Chapter VI. Evolution of Stars and Synthesis of Elements 1. Stages in the Life History of Stars . . . . . . 2. The Most Important Nuclear Reactions in Stars 3. Interstellar Matter . . . . . . . • 4. Possibility of Formation of Organic Compounds Due to Action of Protons in Solar and Cosmic Radiation . . . 5. Chemistry and Cosmology
129 129 132 135 136 140 145 151
15'1
162 166 168 169
Chapter VII. Prtmary Synthesis of Organic Compounds 1. Physical Factors wh ich Affect Synthesis 2. Action of Light on Matter 3. Relative R ole of V