Pleasures of the telescope: An Illustrated Guide for Amateur Astronomers and a Popular Description of the Chief Wonders of the Heavens for General ReadersServiss, Garrett Putman
Science
Pleasures of the telescope: An Illustrated Guide for Amateur Astronomers and a Popular Description of the Chief Wonders of the Heavens for General Readers
But what was the meaning of all this? Evidently a catastrophe of some
kind had occurred out there in space. The idea of a collision involving
the transformation of the energy of motion into that of light and heat
suggests itself at once. But what were the circumstances of the
collision? Did an extinguished sun, flying blindly through space, plunge
into a vast cloud of meteoric particles, and, under the lashing impact
of so many myriads of missiles, break into superficial incandescence,
while the cosmical wrack through which it had driven remained glowing
with nebulous luminosity? Such an explanation has been offered by
Seeliger. Or was Vogel right when he suggested that Nova Aurigae could
be accounted for by supposing that a wandering dark body had run into
collision with a system of planets surrounding a decrepit sun (and
therefore it is to be hoped uninhabited), and that those planets had
been reduced to vapor and sent spinning by the encounter, the second
outburst of light being caused by an outlying planet of the system
falling a prey to the vagabond destroyer? Or some may prefer the
explanation, based on a theory of Wilsing's, that _two_ great bodies,
partially or wholly opaque and non-luminous at their surfaces, but
liquid hot within, approached one another so closely that the tremendous
strain of their tidal attraction burst their shells asunder so that
their bowels of fire gushed briefly visible, amid a blaze of spouting
vapors. And yet Lockyer thinks that there was no solid or semisolid mass
concerned in the phenomenon at all, but that what occurred was simply
the clash of two immense swarms of meteors that had crossed one
another's track.
Well, where nobody positively knows, everybody has free choice. In the
meantime, look at the spot in the sky where that little star made its
appearance and underwent its marvelous transformation, for, even if you
can see no remains of it there, you will feel your interest in the
problem it has presented, and in the whole subject of astronomy, greatly
heightened and vivified, as the visitor to the field of Waterloo becomes
a lover of history on the spot.
The remaining objects of special interest in Auriga may be briefly
mentioned: 26, triple star, magnitudes five, eight, and eleven,
distances 12", p. 268 deg., and 26", p. 113 deg.; 14, triple star, magnitudes
five, seven and a half, and eleven, distances 14", p. 224 deg., and 12.6",
p. 342 deg., the last difficult for moderate apertures; lambda, double,
magnitudes five and nine, distance 121", p. 13 deg.; epsilon, variable,
generally of third magnitude, but has been seen of only four and a half
magnitude; 41, double, magnitudes five and six, distance 8", p. 354 deg.;
996, 1067, 1119, and 1166, clusters all well worth inspection, 1119
being especially beautiful.
Public-domain text, read in full here on John Shaqi.
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