If the tide-producing force is proportional to G × M/R3, then the Moon exerts a greater tide-raising force than the Sun due to the difference in their masses rather than a difference in their distances from the Earth.
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Q28: The _ tide component tends to make
Q31: Diurnal tide cycles occur
A) once a day.
B)
Q32: The center of mass of the Earth-Moon
Q32: To navigate swift tidal currents safely, small
Q36: Lunar tides are larger than solar tides.
Q37: Open ocean tides can be monitored and
Q37: The terms "ebb" and "low" pertain to
Q39: The combination of diurnal and semidiurnal tides
Q40: Rotary currents progress in a clockwise direction
Q45: Tides of large amplitude occurring every two
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