In physics and mathematics, equations of motion describe how an object moves through space over time. For the paper airplane exercise, these are given by the parametric equations \( x = t - 2 \sin t \) and \( y = 3 - 2 \cos t \). Parametric equations are particularly useful when examining motion, as they allow each coordinate (horizontal and vertical, in this case) to be expressed as a function of a third variable, typically time \( t \).
This setup permits simultaneous consideration of both the trajectory's shape and the timing of the moving object at any given instance. Here, \( x(t) \) tells us where the airplane is horizontally, and \( y(t) \) provides its vertical position. By adjusting the parameter \( t \), the airplane's precise position at any moment during its flight can be determined.
- \( x = t - 2 \sin t \): Horizontal movement depends on time and the sinusoidal component.
- \( y = 3 - 2 \cos t \): Vertical position oscillates, reaching peaks and troughs based on the cosmological value.
The role of the trigonometric functions in these equations (\( \sin \) and \( \cos \)) introduces periodic motion characteristics—often essential for studying repetitive or cyclical motion patterns such as the path a thrown object follows.