he naked eye on a clear night, and are
often mistaken for comets.
The great nebula in Orion is one of the most noticeable objects in the
heavens. It is noted for its size and brilliancy, and also for the
successful observation which it has been subjected to from time to time.
This large nebula is situated in that part of Orion which is occupied by
several stars known as the Sword Handle. These multiple stars are known
by the name of Theta. Around these multiple stars is to be seen the
nebula, as though the multiple stars really were enveloped by the nebula
extending for a great distance out into space. It is of a faint bluish
colour, with the central parts possessing the greatest brilliancy. The
suggestion arises in our mind as to whether the nebulae are in any ways
indicative of the presence of the electro-magnetic aetherial field that
each star undoubtedly possesses. We learned in Art. 88 that the sun is
an electro-magnet, and that it possesses its electro-magnetic field. We
have also seen in Art. 109 that the zodiacal light, which is to be
observed in connection with our solar system, is really indicative of
the presence of that electro-magnetic field, as it rotates round the
central body. Now, if an observer were situated out in space, where the
nebula of Orion is situated, and could look at our system with
telescopes equally as powerful as those we possess, would not our sun
present an equally nebulous light to them because of the presence of its
electro-magnetic field?
Conversely, if every star possesses an electro-magnetic aetherial field,
as they undoubtedly do, then it seems only reasonable to infer that that
electro-magnetic field possesses a nebulosity which corresponds with our
zodiacal light. The fact that the spectra of the nebulae are continuous,
revealing no dark lines, seems to indicate the purity of some of the
nebulae, and that therefore they are free from all known elements.
So that spectroscopic results seem to confirm this hypothesis, as the
pure Aether that would surround every star, or multiples of stars, would
certainly not reveal any dark lines by means of the spectroscope. Such a
hypothesis, as to the real nature of a nebula, is entirely in harmony
with the theory of the Aether presented in Chapter IV., because being
gravitative it will surround each star or multiples of stars, and
therefore be denser nearest to those stars, and being atomic, there will
be a certain amount of nebulosity m
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