Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
If space outside our stellar system is infinite in extent, and if all
the stars within that system are moving unchecked in every conceivable
direction, the result must happen that after immense ages these stars
will have drawn apart to such a distance from each other, that the
system will have entirely disintegrated, and will cease to exist as a
connected whole. Eventually, indeed, as Professor Newcomb points out,
the stars will have separated so far from each other that each will be
left by itself in the midst of a black and starless sky. If, however, a
certain proportion of stars have a speed sufficiently slow, they will
tend under mutual attraction to be brought to rest by collisions, or
forced to move in orbits around each other. But those stars which move
at excessive speeds, such, for instance, as 1830 Groombridge, or the
star in the southern constellation of Pictor, seem utterly incapable of
being held back in their courses by even the entire gravitative force of
our stellar system acting as a whole. These stars must, therefore, move
eventually right through the system and pass out again into the empty
spaces beyond. Add to this; certain investigations, made into the speed
of 1830 Groombridge, furnish a remarkable result. It is calculated,
indeed, that had this star been _falling through infinite space for
ever_, pulled towards us by the combined gravitative force of our entire
system of stars, it could not have gathered up anything like the speed
with which it is at present moving. No force, therefore, which we can
conjure out of our visible universe, seems powerful enough either to
have impressed upon this runaway star the motion which it now has, or to
stay it in its wild course. What an astounding condition of things!
Public-domain text, read in full here on John Shaqi.
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