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Outlines of an observational experiment.



 
 
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  #1  
Old February 2nd 08, 11:30 AM posted to sci.astro.amateur
oriel36[_2_]
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Posts: 8,478
Default Outlines of an observational experiment.

The heliocentric orbital motion of the Earth contains an orbital
component which can be discerned by observations of the unique axial/
equatorial orientation of Uranus in its changes with respect to the
Sun.To isolate the Earth's orbital component ,where a location turns
through 360 degrees with respect to the Sun in accordance with
Keplerian orbital motion,requires the use of the GPS system and a
satellite which maintains a fixed postion in accordance with the
orbital component.

The current observations of the orbital component are made from a
geostationary axial/equatorial perspective -

http://www.youtube.com/watch?v=nwTrYVBcx9s

The orbital component is offset by 23 1/2 degrees from axial/
equatorial coordinates,the motion of the solar radiation/orbital
shadow boundary seen in that time lapse footage would be altered to a
isolated orbital perspective by having the orbital stationary
satellite follow a trajectory which deviates from a geostationary
system.

The greatest difficulty is seperating axial and orbital motions/
orientations ,humans can only process one motion and orientation at a
time hence the impossibility of explaining variations in daylight/
darkness,the seasons,the unequal noon cycles using variable axial/
equatorial inclination.The inclusion of a new orbital component based
on changing orientation of a location with respect to the Sun over an
annual orbit is required all observed phenomena and replaces variable
axial inclination,it is also a gorgeous motion in itself, a matter of
straightening up the motion of the solar radiation/orbital shadow
boundary by shifting from a axial geostationary to an orbital
stationary perspective and applying the lessons learned from Uranus
to be applied to the Earth -

http://space.newscientist.com/data/i...2529-1_800.jpg

http://www.youtube.com/watch?v=nwTrYVBcx9s



  #2  
Old February 3rd 08, 12:50 PM posted to sci.astro.amateur
oriel36[_2_]
external usenet poster
 
Posts: 8,478
Default Outlines of an observational experiment.

On Feb 2, 11:30*am, oriel36 wrote:
The heliocentric orbital motion of the Earth contains an orbital
component which can be discerned by observations of the unique axial/
equatorial orientation of Uranus in its changes with respect to the
Sun.To isolate the Earth's orbital component ,where a location turns
through 360 degrees with respect to the Sun in accordance with
Keplerian orbital motion,requires the use of the GPS system and a
satellite which maintains a fixed postion in accordance with the
orbital component.

The current observations of the orbital component are made from a
geostationary axial/equatorial perspective -

http://www.youtube.com/watch?v=nwTrYVBcx9s

The orbital component is offset by 23 1/2 degrees from axial/
equatorial coordinates,the motion of the solar radiation/orbital
shadow boundary seen in that time lapse footage would be altered to a
isolated orbital perspective by having the orbital stationary
satellite follow a trajectory which deviates from a geostationary
system.

The greatest difficulty is seperating axial and orbital motions/
orientations ,humans can only process one motion and orientation at a
time hence the impossibility of explaining variations in daylight/
darkness,the seasons,the unequal noon cycles using variable axial/
equatorial inclination.The inclusion of a new orbital component based
on changing orientation of a location with respect to the Sun over an
annual orbit is required all observed phenomena and replaces variable
axial inclination,it is also a gorgeous motion in itself, a matter of
straightening up the motion of the solar radiation/orbital shadow
boundary by shifting from a axial geostationary to an orbital
stationary perspective *and applying *the lessons learned from Uranus
to be applied to the Earth * -

http://space.newscientist.com/data/i...9/dn12529-1_80...

http://www.youtube.com/watch?v=nwTrYVBcx9s


There are additional sequential images which help discriminate between
axial and orbital components in the various motions of Uranus -

http://astro.berkeley.edu/~imke/Infr..._2001_2005.jpg

The moons of Uranus follow a trajectory much like our own moon follows
Equatorial orientation as a consequence of axial rotation.An axial/
equatorial geostationary satellite will have roughly the same
properties as the moons of Uranus insofar as it should be easy to
discriminate the axial trajectories of the moons from the change in
orbital orientation as a location slowly turns through 360 degrees
with respect to the Sun as seperate to axial rotation.

The proximity of the Earth's axial orientation with the change in
orbital orientation does not lend itself to a clear seperation of
axial and orbital components however artificial means can be employed
to gauge the actual change in orbital orientation and specifically the
GPS system.
 




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