The Calculus of Motion
Imagine you are tracking a particle moving along a straight line. Its velocity isn't constant; it's changing every single second. The problem gives us the exact mathematical rule governing this velocity: v=αt+βt2. This is a quadratic equation, meaning if we were to graph velocity against time, we would see a beautiful parabolic curve sweeping upwards.
Our mission is to find the total distance this particle travels between the 1st and 2nd second.
The Master Equation
How do we extract distance from velocity? We must turn to the fundamental definitions of kinematics. Velocity is defined as the rate of change of displacement with respect to time. Mathematically, this is written as a derivative:
To find the small displacement ds over an infinitesimally small time interval dt, we rearrange the equation:
To find the total distance s over a macroscopic time interval, we must sum up all these tiny ds segments. In the language of calculus, this continuous summation is integration. Geometrically, this integral represents the exact area under the velocity-time graph between our two time limits.
Executing the Integral
Now, we substitute our specific velocity function into the integral and set our limits from t=1 to t=2:
Integrating this polynomial is straightforward. We apply the power rule of integration, ∫tndt=n+1tn+1. The constants α and β simply multiply the results.
Final Calculation
The final step is to evaluate this expression at the upper limit (t=2) and subtract the value at the lower limit (t=1). This is where we must be careful with our arithmetic to avoid silly mistakes.
s=(α222+β323)−(α212+β313)
Let's group the α and β terms together for cleaner algebra:
And there we have it! By applying the fundamental theorem of calculus to our kinematic definitions, we have successfully derived the exact distance travelled by the particle. The correct option is (b).