This article is intended to narrate the motives that led up to

the investigation and also the manner in which the work was
planned, executed and terminated
This article is intended to narrate the motives that led up to
the investigation and also the manner in which the work was
planned, executed and terminated. No names are withheld and the
date of every important event is given, so that an interested
reader may be enabled to follow closely upon the order of
things as they occurred and thus form a correct idea of the
importance of the undertaking, the risk entailed in its
accomplishment and how evenly divided was the work among those
who, in the faithful performance of their military duties,
contributed so much for the benefit of mankind; the magnitude
of their achievement is of such proportions, that it loses
nothing of its greatness when we tear away the halo of apparent
heroism that well-meaning but ignorant historians have thrown
about some of the investigators.


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When we apply the spectroscope to celestial objects we find

apparently an endless variety of spectra
When we apply the spectroscope to celestial objects we find
apparently an endless variety of spectra. We shall illustrate
some of the leading characteristics of these spectra as in
Figs. 13 to 18, inclusive, and Figs. 21, 22, 23 and 24. The
spectra of some nebulae consist almost exclusively of isolated
bright lines, indicating that these bodies consist of luminous
gases, as Huggins determined in 1864; but a very faint
continuous band of light frequently forms a background for the
brilliant bright lines. Many of the nebular lines are due to
hydrogen, others are due to helium; but the majority, including
the two on the extreme right in Fig. 13, which we attribute to
the hypothetical element nebulium, and the close pair on the
extreme left, have not been matched in our laboratories and,
therefore, are of unknown origin. Most of the irregular nebulae
whose spectra have been observed, the ring nebulae, the
planetary and stellar nebulae, have very similar spectra,
though with many differences in the details.[1]


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