THE STRUCTURE OF THE UNIVERSE.—If the distance of each star were known in addition to its position in the sky, our knowledge of the present structure of the universe would be complete. In order to determine the change in the structure, it would be only necessary to know the motions of the stars. We know the positions of a great number of the stars and their motions across the line of sight; we know also the velocities in the line of sight of a few, and the distances of a still smaller number. The data for the solution of the problem are therefore very meagre. Nevertheless, there are indirect methods of attacking the problem which may tend to lead one to an approximate solution, and it is these methods which form the subject of the very instructive article which appears in the July number of Science Progress by Mr. H. Spencer Jones, of the Royal Observatory, Greenwich. The idea, as he states, that the centre of our system is occupied by an immense sun, many thousands of times larger and more glorious than our own sun, and that round about it are millions of lesser suns of various sizes, together forming the nucleus of an immense spiral nebula, of which the spiral arms coiling around the nucleus appear to us as the Milky Way, and that this to us immense system is but one, and perhaps a comparatively small, island universe amongst thousands or millions of other island universes in space, is an idea which by its magnificence appeals to the mind of man. What forms the substance of the article is the basis of truth upon which this conception is founded, and the straightforward and clear way in which the author has marshalled his evidence makes the article of particular interest.
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