Dynamics of uniform circular motion

The average velocity is calculated by dividing the change in velocity by the change in time. An object’s average velocity tells us nothing about what happens to it between its starting and finishing points. The more detailed the input, the smaller the time intervals considered in a motion. We’re left with an infinitely small gap […]

Uniform motion is described in physics as motion in which the velocity of a body travelling in a straight line remains constant. A uniform motion occurs when the distance travelled by a moving object is the same at multiple time intervals, regardless of time length. As there is a constant velocity with regard to time,

Introduction In 1609, Johannes Kepler gave his first two laws of planetary motion after examining Tycho Brahe’s astronomical data. After a gap of 10 years, he reported his third law in 1619.  Before starting his research on planetary motion, he believed in the Copernican model of the solar system like many of his time. The

Instantaneous velocity refers to the rate at which a position changes in a very short time period (almost zero). Measuring in SI units m/s. The magnitude of the instantaneous velocity is instantaneous speed. It is the same as instantaneous velocity however without any direction. Simply put, it is the object’s velocity at that moment in time. Therefore the speed

Uniform motion is described in physics as motion in which the velocity of a body travelling in a straight line remains constant. A uniform motion occurs when the distance travelled by a moving object is the same at multiple time intervals, regardless of time length. As there is a constant velocity with regard to time,