The Earth's BeginningBall, Robert S. (Robert Stawell)
Science
The Earth's Beginning
Ball, Robert S. (Robert Stawell)
Krakatoa (Indonesia); Nebular hypothesis
The most notable fact which emerges from the modern study of the
structure of the heavens is the ever-increasing significance and
importance of the spiral nebulæ. The following pages will have failed in
their object if they have not succeeded in emphasising the fact that the
spiral nebula is, next to a fixed star itself, the most characteristic
type of object in the material universe. With every increase in the
power of the telescope, and with every development of the application of
photography to celestial portraiture, the importance of the spiral
structure in nebulæ becomes of ever-increasing interest.
But I revert to this subject here for the purpose of taking notice of a
suggestive paper by Mr. C. Easton in the “Astrophysical Journal,” Vol.
XII., No. 2, September, 1900, entitled “A New Theory of the Milky Way.”
This paper advances the striking view that the Milky Way is itself a
spiral nebula, and certainly the considerations adduced by Mr. Easton
seem to justify his remarkable conclusion.
It is first to be noticed that the Milky Way extends as an irregular
band completely round the heavens, and that it follows very nearly the
course of a great circle. The curious convolutions of the Milky Way, the
varying star densities of its different parts, would, as shown by Mr.
Easton, be completely accounted for if the Milky Way were a mighty
spiral. We view the ordinary celestial spirals from the outside at an
immense distance in space. We view the Milky Way from a position within
the circuit of the nebula. It has, however, been shown by Mr. Easton
that the centre of the Spiral Nebula is not exactly at the sun. The
centre of the Milky Way is near that superb region of the galaxy which
lies in Cygnus.
Thus, the significance of the spiral structure in the universe becomes
greatly enhanced. The spirals abound in every part of the heavens; they
are placed in every conceivable position and in every possible plane;
they have every range in size from comparatively small objects, whose
destiny is to evolve into a system like our solar system, up to
stupendous objects which include a myriad of such systems. There is now
the further interest that as the sun and the solar system are included
within the Milky Way, and as the Milky Way is a spiral, this earth of
ours is itself at this moment a constituent part of a great spiral.
Finally, I would say that, so far as I have been able to understand the
subject, it appears to me that every advance in our knowledge of the
heavens tends more and more to support the grand outlines of the Nebular
Theory as imagined by Kant and Laplace.
R. S. B.
_May 1, 1909._
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CONTENTS
CHAPTER PAGE
I. —INTRODUCTION 1
Public-domain text, read in full here on John Shaqi.
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