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Re: Orbital Mechanics - Solar System Simulator

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Re: Orbital Mechanics - Solar System Simulator David Williams 11-24-2006
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Posted by David Williams on November 24, 2006, 10:18 pm
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-> Dave, you're missing the fun. One can set-up a
-> system such that a pea in orbital relation with a
-> pair of cabbages will eventually acquire escape
-> velocity, and be emitted.
-> That's an analogy to an unstable isotope or
-> particle that *transmutes* via emission.
-> Regards
-> Ken

The questioner has already, he says, experienced too much of this fun.
He said that he couldn't set up a stable arrangement with more than
three stars. I tried to show how this is possible.

dow

Posted by Ken S. Tucker on November 26, 2006, 12:25 am
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David Williams wrote:
> -> Dave, you're missing the fun. One can set-up a
> -> system such that a pea in orbital relation with a
> -> pair of cabbages will eventually acquire escape
> -> velocity, and be emitted.
> -> That's an analogy to an unstable isotope or
> -> particle that *transmutes* via emission.
> -> Regards
> -> Ken
>
> The questioner has already, he says, experienced too much of this fun.
> He said that he couldn't set up a stable arrangement with more than
> three stars. I tried to show how this is possible.

But it's not possible.
IIRC, there's no Newtonian stable solution even
with 3 bodies, the solution is chaotic.
The net energy - is of course - conserved, however,
the system takes a path where 2 of the bodies
orbit more and more closely and supply kinetic
energy to the third which acquires the escape,
by sucking kinetic energy from the orbital energy
of the remaining pair. There is no such thing as
a stable *static* arrangement in our universe,
it's all dynamic.
Ken


Posted by rob on November 26, 2006, 3:17 am
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Yeah, that is pretty much what I find with setting up the simulator. But
this is most obvious when you try and create a system with, say, three or
more objects that are of similar mass. Then it is very hard / impossible to
create a stable system. If the objects in your solar system consist of 1 or
2 large objects and a large number of small objects then a relatively stable
system can also be created.

>
> David Williams wrote:
>> -> Dave, you're missing the fun. One can set-up a
>> -> system such that a pea in orbital relation with a
>> -> pair of cabbages will eventually acquire escape
>> -> velocity, and be emitted.
>> -> That's an analogy to an unstable isotope or
>> -> particle that *transmutes* via emission.
>> -> Regards
>> -> Ken
>>
>> The questioner has already, he says, experienced too much of this fun.
>> He said that he couldn't set up a stable arrangement with more than
>> three stars. I tried to show how this is possible.
>
> But it's not possible.
> IIRC, there's no Newtonian stable solution even
> with 3 bodies, the solution is chaotic.
> The net energy - is of course - conserved, however,
> the system takes a path where 2 of the bodies
> orbit more and more closely and supply kinetic
> energy to the third which acquires the escape,
> by sucking kinetic energy from the orbital energy
> of the remaining pair. There is no such thing as
> a stable *static* arrangement in our universe,
> it's all dynamic.
> Ken
>



Posted by Jonathan Silverlight on November 26, 2006, 12:14 pm
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>
>David Williams wrote:
>> -> Dave, you're missing the fun. One can set-up a
>> -> system such that a pea in orbital relation with a
>> -> pair of cabbages will eventually acquire escape
>> -> velocity, and be emitted.
>> -> That's an analogy to an unstable isotope or
>> -> particle that *transmutes* via emission.
>> -> Regards
>> -> Ken
>>
>> The questioner has already, he says, experienced too much of this fun.
>> He said that he couldn't set up a stable arrangement with more than
>> three stars. I tried to show how this is possible.
>
>But it's not possible.
>IIRC, there's no Newtonian stable solution even
>with 3 bodies, the solution is chaotic.
>The net energy - is of course - conserved, however,
>the system takes a path where 2 of the bodies
>orbit more and more closely and supply kinetic
>energy to the third which acquires the escape,
>by sucking kinetic energy from the orbital energy
>of the remaining pair. There is no such thing as
>a stable *static* arrangement in our universe,
>it's all dynamic.
>Ken
>

There are dynamically stable situations of three or more equal masses -
Klemperer Rosettes (the thing Larry Niven mis-spells in Ringworld :-)
<http://en.wikipedia.org/wiki/Klemperer_rosette>
I recall reading an article a few years ago in "Astronomy" or "Sky and
Telescope" about a star that is thought to have been ejected from a
close triple system.

Posted by Ken S. Tucker on November 26, 2006, 3:40 pm
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Jonathan Silverlight wrote:
> >
> >David Williams wrote:
> >> -> Dave, you're missing the fun. One can set-up a
> >> -> system such that a pea in orbital relation with a
> >> -> pair of cabbages will eventually acquire escape
> >> -> velocity, and be emitted.
> >> -> That's an analogy to an unstable isotope or
> >> -> particle that *transmutes* via emission.
> >> -> Regards
> >> -> Ken
> >>
> >> The questioner has already, he says, experienced too much of this fun.
> >> He said that he couldn't set up a stable arrangement with more than
> >> three stars. I tried to show how this is possible.
> >
> >But it's not possible.
> >IIRC, there's no Newtonian stable solution even
> >with 3 bodies, the solution is chaotic.
> >The net energy - is of course - conserved, however,
> >the system takes a path where 2 of the bodies
> >orbit more and more closely and supply kinetic
> >energy to the third which acquires the escape,
> >by sucking kinetic energy from the orbital energy
> >of the remaining pair. There is no such thing as
> >a stable *static* arrangement in our universe,
> >it's all dynamic.
> >Ken
> >
>
> There are dynamically stable situations of three or more equal masses -
> Klemperer Rosettes (the thing Larry Niven mis-spells in Ringworld :-)
> <http://en.wikipedia.org/wiki/Klemperer_rosette>
> I recall reading an article a few years ago in "Astronomy" or "Sky and
> Telescope" about a star that is thought to have been ejected from a
> close triple system.

Jon I must agree with you and dow,
in a perfect universe with an ideal configuration
a gazillion "symmetrical" configurations will
remain stable, (I'm using Newton, GR screws
things up with so-called g-radiation).

But using the greatest supercomputer, you can't
achieve mathematical perfection because you
will always have a limited number of digits.

Let's suppose an n>2 body stable configuration
to start, and 1 friggin asteriod passes threw that
system, in and out but deflected. That asteriod
has now induced a bit of chaos that will break-
down the systems stabilty, in my understanding,
which will eventually decay to an n-1 system, by
eliminating one particle from the original n body
system.

I've argued with Dave (dow) that I find the neutron
~15 minute decay is induced by a neutrino, where
the spin is still conserved.

I think this is a good discussion because principles
that apply to gravitationally bound systems may also
apply in sub-atomic particle decays. That in turn may
provide us some insight into the structure of particles.
Thanks guys
Ken


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