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EXPLORING THE KINDERKEN WORLD
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PLUTO'S VERY STRANGE ORBIT
(Reprinted from TEDDY SPEAKS JUNE 1994) by Marshall Smith
The ninth planet, Pluto, has a very strange orbit. Unlike all the other planets
which have fairly circular orbits around the sun, Pluto has an orbit that is
highly oval or ellipsoid. It is so strange that its orbit moves far beyond the
eighth planet, Neptune, and sometimes even moves Inside the orbit of Neptune.
It currently is Inside Neptune's orbit and is now the eighth planet with
Neptune being outermost or ninth planet.
One theorist has now guessed that Pluto's orbit was pulled out of shape by
interaction with its nearest neighbor Neptune. The theory ls based on the
assumption that all planets were formed out of a primordial cloud of gas and
that originally all the orbits were regular and circular.
Using a computer simulation Renu Malhotra of the Lunar and Planetary Institute
In Houston, reports this possibility in the Journal Nature. She believes that
Neptune's orbit began to expand shortly after the solar system was formed and
thus moved into the region of Pluto and warped it's orbit.
Scott Tremaine, professor of physics and astronomy at the Unlversity of Toronto
In Ontario, says, ''I'd say it looks pretty good.� But that is the kind of
thing scientists say when they have no idea what the truth is but can't find
anything wrong with the theory.
Another scientist, Stanton Peale of the University of California Santa Barbara.
points out that Malhotra's simulation did not produce the extreme tilt (17
degrees) of Pluto's orbit compared to the rest of the planets. This also
is the kind of thing scientists say when they mean the theory is �all wet'' and
can't be true since it does not account for all observed facts.
Many theories have been proposed for Pluto's orbit. Some believe that is was a
planetesimal captured from the multitude of space clutter far beyond the solar
system. Others believe that Pluto is an escaped moon from Neptune.
A much more complete but unpublished theory is that originally Neptune was a
very hot spinning ball of gas. As Neptune cooled over millions of years It
shrank and as a result of the Conservation of Angular Momentum began to rotate
so fast that some material was thrown out or ejected This allowed Neptune to
slow down to a more stable rotation rate. But the material ejected was not
thrown along the line of the ecliptic but at an angle of 17 degrees.
One result of this is that Neptune recoiled and tilted its axis of rotation and
the ejected material was thrown far enough that it escaped the gravitational
field of Neptune and went into orbit around the sun. No matter whether the
ejected material was thrown toward the sun or away from the sun, the material
would form an elliptical orbit around the sun that moves inside and outside the
orbit of Neptune.
The ejected body would have been about 10 percent of the mass of Neptune and
made of the same, mostly gaseous, material. Because the ejected body was so
small its gravity was insufficient to hold the light gasses which escaped into
the vacuum of space. What was left was a tiny rocky core that we call Pluto.
This scenario has been repeated many times in the solar system and is the
primary means for the creation of most of the moons of the planets. Including
the moon of Earth. (This theory will be detailed in an upcoming issue of Teddy
Speaks Magazine)
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