Here is a sketch of the Jupiter/Saturn rotation/revolution situation:
In Figure A is shown :
#1, Planet,
#2 North pole,
#3 Orbital velocity in
green, prograde motion,
#4 Points on equator,
#5 Rotational velocity in
red, prograde motion,
#6 telescopes measuring transit of points 4, looking in ( on top), -toward, and - out to planet (on bottom),
#7 stationary area of surface facing directly toward sun, and
#8 fasted area facing away from sun,
Planet #1 is rotating about North Pole #2 , giving points #4
rotational direction #5. Planet#1 has
orbital motion #3. Telescopes 6 are viewing close and far points #4 near the equator of planet 1.
In area #7, the two motions: the #3, prograde orbit revolution of the planet (green) and its rotation #5 (red) are seen to
subtract, ~ cancelled, resulting in a near zero proper motion of the area #7 closest to the sun.
In area # 8 these two motions are seen to
add, arrows shown in concert, giving the points #4 there
twice the orbital velocity.
This leads points #4 to transit the field of view of inner telescope #6 very slowly (area#7), , but causes a fast passage, only a short time appearance, in the outer instrument #6, aiming at area #8.
Theses situations prevails despite the points #4 having the constant rotational velocity# 5. so:
prolonged/shortened exposure?, really?
A similar situation would have occurred had a supersonic plane remained in the shadow of last years' eclipse, ( did not happen, no bang heard) .
Questions: prolonged, exposure, shortened exposure possible with a far away ~5 AU, ~10 AU point source? does it matter? of course
Total solar energy impinging on the total area does not change, but duration/ intensity might vary from equator to poles, point to point, with effects.