Speed and direction remain constant unless acted upon by an external force
Free fall motion
Object falls under the influence of gravity without any other forces acting on it
Acceleration of free fall near the Earth's surface is approximately 9.81 m/s² downward
Projectile motion
Motion of an object projected into the air under the influence of gravity
Involves both horizontal and vertical components of motion, resulting in a curved trajectory
Uniform circular motion
Object moves in a circular path at a constant speed
Object experiences a centripetalforce directed towards the center of the circle to maintain its circular motion
Newton'sUniversalLawofGravitation
Every particle in the universe attracts every other particle with a force that is directlyproportional to the product of their masses and inverselyproportional to the square of the distance between their centers
Newton's Laws of Motion
Newton's First Law (Law of Inertia)
Newton's Second Law (Law of Acceleration)
Newton's Third Law (Action-Reaction Law)
Newton'sFirstLaw (Law of Inertia)
An object at rest will remain at rest, and an object in motion will continue moving in a straight line at a constant velocity unless acted upon by an external force
Newton'sSecondLaw (Law of Acceleration)
The acceleration of an object is directly proportional to the net force acting on it and inversely proportional to its mass
Newton'sThirdLaw (Action-Reaction Law)
For every action, there is an equal and opposite reaction
Normal force
The force exerted by a surface on an object in contact with it, perpendicular to the surface
Friction
The force that opposes the relative motion or tendency of motion between two surfaces in contact
Types of friction
Static friction
Kinetic friction
Tension
The pulling force transmitted through a string, rope, cable, or any other similar object when it is pulled tight by forces acting from opposite ends
Kepler's Laws of Planetary Motion
Kepler's First Law (Law of Ellipses)
Kepler's Second Law (Law of Equal Areas)
Kepler's Third Law (Law of Harmonies)
Kepler's First Law (Law of Ellipses)
The orbit of a planet around the Sun is an ellipse with the Sun at one of the two foci
An ellipse is a geometric shape resembling a stretched circle, where the distance between the center and the edges varies
Kepler'sSecondLaw (Law of Equal Areas)
A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time
A planet moves faster when it is closer to the Sun and slower when it is farther away, maintaining a consistent rate of change in the area it sweeps out
Work
When a force acts on an object to move it over a distance in the direction of the force
Power
The rate at which work is done or energy is transferred
Energy
The capacity to do work, classified into potential energy and kinetic energy
Momentum
A vector quantity that describes the motion of an object, calculated as the product of its mass and velocity
Impulse
The change in momentum of an object when a force is applied over a time interval