Inertia. The pendulum will continue in the same motion until an outside force changes it's direction. The earth turns underneath it, it is not connected to the earth except a the connection of the wire, the rotation of the earth has not effect on the pendulum.
Newton's laws of motion
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For other uses, see
Laws of motion.

Newton's First and Second laws, in Latin, from the original 1687
Principia Mathematica.
Classical mechanics
{\displaystyle {\vec {F}}=m{\vec {a}}}
Second law of motion
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Newton's laws of motion are three
physical laws that, together, laid the foundation for
classical mechanics. They describe the relationship between a body and the
forces acting upon it, and its
motion in response to those forces. They have been expressed in several different ways, over nearly three centuries,
[1] and can be summarised as follows.
First law: When viewed in an
inertial reference frame, an object either remains at rest or continues to move at a constant
velocity, unless acted upon by a
net force.
[2][3]
Second law: In an inertial reference frame, the
vector sum of the
forces F on an object is equal to the
mass m of that object multiplied by the
acceleration vector
a of the object:
F =
ma.
Third law: When one body exerts a force on a second body, the second body simultaneously exerts a force equal in magnitude and opposite in direction on the first body.
Newton's laws of motion - Wikipedia, the free encyclopedia