Kinematic equations are mathematical formulas used to describe the motion of a body under constant acceleration, like our projectile here. When dealing with projectiles, we often use the kinematic equation:
\[ R = v_0 t - \frac{1}{2} g t^2 \]
This formula helps in calculating displacement for a body moving under the influence of gravity, assuming the initial position is zero.
Here’s how the equation works:
- \(R\) is the displacement or change in position.
- The term \(v_0 t\) calculates the distance covered by the initial velocity over time \(t\).
- The subtraction \(-\frac{1}{2} g t^2\) accounts for the deceleration due to gravity.
This equation becomes particularly important when solving for the time it takes for a projectile to reach its maximum height and then fall back to a certain point.