Trigonometric motion refers to the movement described by trigonometric functions such as sine and cosine. In our example, the object's displacement over time is given by the function \(d(t) = 4 + 3 \, \text{sin}(\pi t)\). Here, the sine function represents the oscillatory motion typical in trigonometry.
Essentially, trigonometric motion is periodic, meaning it repeats at regular intervals. This can often be visualized as an object moving back and forth, like a pendulum. The displacement function tells us the position of the object at any given time, factoring in both a constant term and a sinusoidal term.
- Constant term (4): Shifts the entire motion vertically by 4 units.
- Sinusoidal term (3 \, \text{sin}(\pi t)): Creates the oscillations around the central line defined by the constant term.
Understanding these components helps explain the overall motion, which in this case, means the object oscillates around the line \(d = 4\).