The evolution of worlds from nebulaeDean, Lee Parker
Science
The evolution of worlds from nebulae
Dean, Lee Parker
Nebular hypothesis
When the sun reached out to earth it must have had a diameter of nearly
200 million miles, but having now contracted to a diameter of less than
one million of miles, should it not have a density ten times greater
than earth’s, instead of one so much less? For if the solid parts when
out at Neptune began to fall toward the sun’s centre, they should
have continued to fall until they reached it, or until they had met
a density greater than their own. We must remember even at the sun’s
present surface a body would fall with much greater velocity than on
earth’s surface because of its greater weight. With the density of our
earth more than five times that of water, and twice that of solid rock,
all heavy substances must gravitate toward its centre; whereas on the
surface of the sun the gravitation is more than 27 times stronger. If
then the sun were ever a fire-mist reaching out to earth, it would
seem that nothing should have prevented the earth from falling with
lightning-like speed to the sun’s centre, as its volume was 8,000,000
times larger than now, and even its present volume would hold 900
thousand worlds like ours before it would have a like density.
2d. _Gravitation._ We see the sun to-day as a perfect sphere, but does
a body that is a sphere ever throw off rings by rotary movement? When a
body in its revolutions throws off rings by rotating, instead of being
spherical it is of a flattened, or grind-stone shape, and the rings are
hurled from it by the centrifugal force overpowering the gravitation;
hence we cannot think that the sun’s rings,—being of enormous
circumference and necessarily of a light or fluid substance in order
to be thrown off,—could form into spheres unless the centrifugal force
was extremely great.
Let us suppose that Neptune was thrown off from the sun as a ring, like
those we see around Saturn; and, as it is now about 3,000 millions
of miles distant from the sun’s centre, before it was detached it
must have had a diameter of about 6,000 millions of miles, with a
circumference of over 18,000 million miles. Now, as Neptune has about
100 times the volume of earth,[5] its ring could have been no more than
40 miles square; for 1600 square miles multiplied by 18,000 million
miles, the distance around that ring, will give more than Neptune’s
volume. How then could any substance so exceedingly thin draw to itself
this enormous distance of 18,000 millions of miles, any more than a
thread a thousand miles in length could draw itself together into a
ball, without the thread’s breaking into a million pieces?
Public-domain text, read in full here on John Shaqi.
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