The Bakerian Lecture, 1968 - Review of recent developments in cosmology
It is hard to believe today that most scientists in the year 1920 believed that our Galaxy was all there is to the whole Universe—the ‘island Universe’ as it was then called. The difference between our present day view, with all its subtle complexities, and such a primitive notion has been brought about very largely by the accumulation of observational data. Almost immediately following the year 1920 Hubble disposed of the ‘island Universe’ concept and for the past fifty years astronomers have worked on the basis that our Galaxy is but one among thousands of millions strewn more or less uniformly throughout space. Although observation plays the key role in determining which ideas survive and which are rejected, ideas themselves frequently come from theoretical studies. Already in 1922 Friedmann discovered the theoretical models of the Universe which are now often described as the ‘big bang’ cosmologies. In this lecture I shall not be much concerned with these models, for the personal reason that I happen to be not very interested in them. But it is of relevance that I should explain to you why this is so.