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The Universe: Its Beginning
and End

by Lloyd Motz

New York: Charles Scribner's Sons, 1975

Starting with the universe when it was but a few seconds old, Lloyd Motz, Professor of Astronomy at Columbia University in New York, first traces the evolution of matter from its initial inchoate, homogeneous state consisting of neutrons and protons only to its present highly differentiated state consisting of galaxies, stars, plants, some 96 different kinds of atoms, a vast array of complex molecules, and intelligent beings. He then describes the various catastrophes that, in time, can befall the world and lead to its destruction, the ultimate catastrophe being the gravitational collapse of the universe itself, which will destroy all existing structures. In his description of the evolution of the various kinds of matter that now fill the universe, Dr. Motz shows how all the existing structures -- from galaxies down to atomic nuclei -- can be understood in terms of the four basic forces in nature.

The first part of the book deals with the formation of galaxies and stars from the primordial material that stemmed from the "big bang," showing how all the heavy elements such as iron, gold, and uranium were built up from hydrogen and helium in the hot cores of the very oldest stars as these stars evolved over billions of years. These chapters also describe how stars that are massive enough can become neutron stars (pulsars) or black holes after they have exhausted all their nuclear fuel and blown off their outer zones in vast explosions.

Later chapters concern the formation of planets and the origin of life on earth. According to Dr. Motz, life will emerge in the neighborhood of all stars like the sun, so there are billions of potentially life-supporting planets in the universe and some hundreds of millions in our own galaxy. The last two chapters deal with the hierarchy of endings which may occur and consider the question of how the earth can escape destruction. Various provocative possibilities, such as taking the earth entirely out of the solar system and attaching it to another star, are suggested.

 

 
   
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