Stellar Evolution and Its Relations to Geological TimeCroll, James
Science
Stellar Evolution and Its Relations to Geological Time
Croll, James
Cosmogony; Geological time; Stars -- Evolution
The theory starts with the assumption that the greater part of the
energy possessed by the universe exists or is stored up in the form of
the motion of stellar masses. The amount of energy which may thus be
stored up is startling to contemplate. Thus a mass equal to that of the
sun, moving with a velocity of 476 miles per second, would possess, in
virtue of that motion, energy sufficient, if converted into heat, to
maintain the present rate of the sun’s radiation for 50,000,000
years.[3] There is nothing extravagant in the assumption of such a
velocity. A comet, for example, having an orbit extending to the path of
the planet Neptune, approaching so near the sun as to almost graze his
surface in passing, would have a velocity within 86 miles of what we
have assumed. Twice this assumed velocity would give 200,000,000 years’
heat; four times the velocity would give 800,000,000 years’ heat; and so
on.
[Footnote 3: Pouillet’s estimate of the rate of solar radiation is here
taken.]
We are at perfect liberty to begin by assuming the existence of stellar
masses in motion; for we are not called upon to explain how the masses
obtained their motion, any more than we have to explain how they came to
have their existence. If the masses were created, they may as likely
have been created in motion as at rest; and if they were eternal, they
may as likely have been eternally in motion as eternally at rest.
Eternal motion is just as warrantable an assumption as eternal matter.
When we reflect that space is infinite—at least in thought—and that, for
aught we know to the contrary, bodies may be found moving throughout its
every region, we see that the amount of energy may be perfectly
illimitable.
But, illimitable as the amount of the energy may be, it could be of no
direct service while it existed simply as the motion of stellar masses.
The motion, to be available, must be transformed into heat: the motion
of translation into molecular, or some other form of motion. This can be
done in no other way than by arresting the motion of the masses. But how
is such motion to be arrested? How are bodies as large as our earth,
moving at the rate of hundreds of miles per second, to have their motion
stopped? According to the theory this is effected by _collision_: by
employing the motion of the one body to arrest that of the other.
Public-domain text, read in full here on John Shaqi.
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