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5.3.3.6 The shape of orbital trajectories in solar system

The shape of the orbital trajectory was in general considered by physicists as circular, elliptical or, not differring much from elliptical so far. The trajectories calculated in accordance with this spaceflow theory varies from the circular through egg-like to pear-like shape, along with the increasing excentricity.
We can see on the following images how the shape of the trajectories with the same aphelion and different perihelion varies. For our example the single aphelion was choosen rk=1,52*1012 m (the aphelion of the planet Saturn).

Fig13d-1

Trajectory
e=0,063620		 Trajectory
e=0,304444
image
Parameters
rk=1,52*1012 m
voodk=8,752046*103 m/sec
rf=1,33816*1012 m
e=0,063620
To=9,296020*108 secs
DeltaAlpha=1,613383*10-2 grade 		image
Parameters
rk=1,52*1012 m
voodk=6,504840*103 m/sec
rf=8,104947*1011 m
e=0,304444
To=6,495800*108 secs
DeltaAlpha=1,066802*10-2 grade

Trajectory
e=0,67903		 Trajectory
e=0,893049
image
Parameters
rk=1,52*1012 m
voodk=3,003776*103 m/sec
rf=2,905724*1011 m
e=0,67903
To=3,335930*108 secs
DeltaAlpha=-6,211542*10-2 grade 		image
Parameters
rk=1,52*1012 m
voodk=1,001461*103 m/sec
rf=8,587478*1010 m
e=0,893049
To=1,650563*108 secs
DeltaAlpha=-4,174293*10-1 grade


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