A Jupiter Hypothesis

Binary Gaseous Protoplanets formed Jupiter

by Joseph_Sixpack

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Abstract:  The intuitive hypothesis is advanced that Jupiter 
(and all other gaseous planets) were formed by the union of 
two or more gaseous protoplanets which today are still 
responsible for and help to explain the high rotation 
velocities of mass at Jupiters polar areas.

This theory goes forward with the hypothesis that All 
Gaseous planets like Jupiter, Saturn, and Uranus, have at 
their polar areas, mass that is very rapid in its orbital 
motion.  Such rotational velocities might be explained by 
the assumption that Jupiter was formed initially by two or 
more gaseous protoplanets in mutually closing and of course, 
accelerating orbits.

The rings of all the gaseous planets seem to be the result 
of such a closing gaseous protoplanet merger and the rapidly 
rotating masses at the polar areas of the gaseous planets 
seem intuitively to add evidence of that reality.

The rings of the gaseous planets are the leftover mass that 
had sufficient x-y vectored velocity to maintain an orbit 
status instead of being accreted into the mass of the 
closing binary system.

What is left in the center core of the binary or higher 
merging protoplanets, for example, at the core of Jupiter 
and the other remaining gaseous planets, may be that which, 
now gravitationally enhanced, enables the relevant magnetic 
fields that surround the objects.    

These types of structures are probably VERY common in the 
cosmos due to normal accretion processes that take place.

From a census point of veiw, these gaseous protoplanet 
structures probably exist from boulder sized all the up to 
full blown near self igniting stars.

Anyhow, that is joe's intuitive hypothesis about the nature 
of Jupiter and all the ringed gaseous planets.  They are 
just composed of dirt and proto-dirt gaseous elements.  
That's all.  At their core the residual binaries are in very 
fast mutual orbit due to the physics of the closing 
mechanism.  At the poles of that type of planet, fast moving 
orbital materials would exist.  Even high speed surface 
winds may be in some way related to the original binary 
closing of two gaseous proto-planets.  The subject needs a 
lot more sciencing done.  Joe's imaginative hypotheses 
aren't going to do the job.

If a third gaseous proto-planet makes its way into the sun's 
spacetime dimple and hits jupiter, who knows, maybe that 
will be enough to start a fusion process going, and then we 
can have really weird days and nights.  That ought to drive 
the bunnies nuts.  :-)


That brings us to the Sun An investigation (if it hasn't already been done) into the orbit speed of the polar regions, or just beneath it, in our own sun, might shed some new data into the nature of the formation of our own star, whether by simple accretion or by accelerated accretion by mergers with other proto-suns. .
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