\(\mathbf{T} / \mathbf{F}:\) When an object falls to Earth, Earth also falls up to the object.

Gravitational force is one of the fundamental forces of nature. It is the force of attraction that exists between any two masses. This means that every object with mass exerts a gravitational pull on every other object with mass.

The strength of this pull depends on two main factors:

• The masses of the objects.
• The distance between them.

When an object falls to Earth, gravity pulls it towards the ground. This force is described by Newton's Law of Universal Gravitation: \[ F = G \frac{m1 \cdot m2}{r^2} \] Here, \[ F \] is the gravitational force, \[ G \] is the gravitational constant, \[ m1 \] and \[ m2 \] are the masses of the two objects, and \[ r \] is the distance between their centers.

Understanding gravitational force helps us make sense of why objects fall towards Earth and why planets orbit stars.

Newton's Third Law of Motion states that for every action, there is an equal and opposite reaction. This means forces always come in pairs. When you push on something, it pushes back on you with the same amount of force.

In the context of an object falling to Earth, the action is the gravitational pull of Earth on the object, pulling it downward. The reaction is the gravitational pull of the object on Earth, pulling Earth upwards. Even though the forces are equal, the effects are different because of the vast difference in mass between Earth and the falling object.

• Action: Object falls towards Earth due to Earth's gravity.
• Reaction: Earth moves slightly upwards towards the object.

The mass of Earth is so large that its movement is tiny and almost imperceptible. This principle is crucial in understanding how forces interact in our world.

Mass plays a crucial role in the movement caused by gravitational forces. Mass is the measure of the amount of matter in an object, and it directly influences how objects respond to forces.

• More mass means more gravitational pull.
• More mass also means more inertia, making it harder to move.

When an object falls, the Earth's gravitational force acts on it, making it accelerate towards the ground. According to Newton's Second Law of Motion, \[ F = ma \] where \[ F \] is force, \[ m \] is mass, and \[ a \] is acceleration.

Although the object also exerts a gravitational force on Earth, Earth's massive size means the acceleration it experiences is extremely small. This is why we do not notice Earth moving towards a falling object.

Understanding mass and movement helps clarify why large objects like Earth seem immovable compared to smaller objects that we see falling every day.