Changes

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[[File:Sam_orbit_1.jpg|thumb|right|450px|Figure 00, exponent = 2.0]]

[[File:Sam_orbit_1.jpg|thumb|right|225px|Figure 00, exponent = 2.0]]

[[File:Sam_orbit_2.jpg|thumb|right|450px|Figure 03, exponent = 2.03]]

[[File:Sam_orbit_2.jpg|thumb|right|250px|Figure 03, exponent = 2.03]]

[[File:Sam_orbit_3.jpg|thumb|right|450px|Figure 2, exponent = 2.2]]

[[File:Sam_orbit_3.jpg|thumb|right|275px|Figure 2, exponent = 2.2]]

[[File:Sam_orbit_4.jpg|thumb|right|450px|Figure 4, exponent = 2.4]]

[[File:Sam_orbit_4.jpg|thumb|right|300px|Figure 4, exponent = 2.4]]

[[File:Sam_orbit_5.jpg|thumb|right|450px|Figure 436, exponent = 2.436]]

[[File:Sam_orbit_5.jpg|thumb|right|200px|Figure 436, exponent = 2.436]]

Figure 00 shows the familiar Kepler orbit with an exponent of exactly 2.  It is an ellipse, of course.  The parameters were set so that the eccentricity was about 2.  (Way more than the planets in the solar system, by the way.)

Figure 00 shows the familiar Kepler orbit with an exponent of exactly 2.  It is an ellipse, of course.  The parameters were set so that the eccentricity was about 2.  (Way more than the planets in the solar system, by the way.)