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A car starts with a velocity of 10 m/s and decelerates at 2.5 m/s2. Calculate its velocity, distance, and time to stop.

Physics

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b)

i) Determine its velocity after 1.5 seconds.

  1. Identify the given values and the formula.

    Initial velocity u=10 m/su = 10 \, \text{m/s}.
    Acceleration a=−2.5 m/s2a = -2.5 \, \text{m/s}^2 (deceleration).
    Time t=1.5 st = 1.5 \, \text{s}.
    We use the kinematic equation: v=u+atv = u + at.

  2. Substitute the values into the formula and calculate the final velocity.

    v=10 m/s+(−2.5 m/s2)(1.5 s)v = 10 \, \text{m/s} + (-2.5 \, \text{m/s}^2)(1.5 \, \text{s}) v=10 m/s−3.75 m/sv = 10 \, \text{m/s} - 3.75 \, \text{m/s} v=6.25 m/sv = 6.25 \, \text{m/s}

    The velocity after 1.5 seconds is 6.25 m/s\boxed{\text{6.25 m/s}}.

    ii) The distance travelled in 1.5 seconds.

  3. Identify the given values and the formula.

    Initial velocity u=10 m/su = 10 \, \text{m/s}.
    Acceleration a=−2.5 m/s2a = -2.5 \, \text{m/s}^2.
    Time t=1.5 st = 1.5 \, \text{s}.
    We use the kinematic equation: s=ut+12at2s = ut + \frac{1}{2}at^2.

  4. Substitute the values into the formula and calculate the distance.

    s=(10 m/s)(1.5 s)+12(−2.5 m/s2)(1.5 s)2s = (10 \, \text{m/s})(1.5 \, \text{s}) + \frac{1}{2}(-2.5 \, \text{m/s}^2)(1.5 \, \text{s})^2 s=15 m+12(−2.5 m/s2)(2.25 s2)s = 15 \, \text{m} + \frac{1}{2}(-2.5 \, \text{m/s}^2)(2.25 \, \text{s}^2) s=15 m−(1.25 m/s2)(2.25 s2)s = 15 \, \text{m} - (1.25 \, \text{m/s}^2)(2.25 \, \text{s}^2) s=15 m−2.8125 ms = 15 \, \text{m} - 2.8125 \, \text{m} s=12.1875 ms = 12.1875 \, \text{m}

    The distance travelled in 1.5 seconds is 12.19 m\boxed{\text{12.19 m}}.

    iii) The time taken by the car to stop.

  5. Identify the given values and the formula.

    Initial velocity u=10 m/su = 10 \, \text{m/s}.
    Final velocity v=0 m/sv = 0 \, \text{m/s} (when the car stops).
    Acceleration a=−2.5 m/s2a = -2.5 \, \text{m/s}^2.
    We use the kinematic equation: v=u+atv = u + at.

  6. Substitute the values into the formula and solve for time tt.

    0 m/s=10 m/s+(−2.5 m/s2)t0 \, \text{m/s} = 10 \, \text{m/s} + (-2.5 \, \text{m/s}^2)t −10 m/s=(−2.5 m/s2)t-10 \, \text{m/s} = (-2.5 \, \text{m/s}^2)t t=−10 m/s−2.5 m/s2t = \frac{-10 \, \text{m/s}}{-2.5 \, \text{m/s}^2} t=4 st = 4 \, \text{s}

    The time taken by the car to stop is 4 s\boxed{\text{4 s}}.

    iv) Sketch the velocity-time graph for the motion of the car up to the time the car stopped.

    The velocity-time graph will be a straight line.

    • The initial velocity at t=0 st=0 \, \text{s} is 10 m/s10 \, \text{m/s}.
    • The final velocity at t=4 st=4 \, \text{s} (from part iii) is 0 m/s0 \, \text{m/s}.
    • The graph starts at (0,10)(0, 10) and ends at (4,0)(4, 0).
    • The slope of the line represents the acceleration, which is −2.5 m/s2-2.5 \, \text{m/s}^2.

    v) From the graph determine the distance covered by the car before it stopped.

  7. The distance covered is the area under the velocity-time graph.

    The graph forms a triangle with the time axis.
    Base of the triangle = time taken to stop = 4 s4 \, \text{s} (from part iii).
    Height of the triangle = initial velocity = 10 m/s10 \, \text{m/s}.

  8. Calculate the area of the triangle.

    Distance=12×base×height\text{Distance} = \frac{1}{2} \times \text{base} \times \text{height} Distance=12×(4 s)×(10 m/s)\text{Distance} = \frac{1}{2} \times (4 \, \text{s}) \times (10 \, \text{m/s}) Distance=20 m\text{Distance} = 20 \, \text{m}

    The distance covered by the car before it stopped is 20 m\boxed{\text{20 m}}.

    1. a)

    i) Determine the acceleration of gravity on the planet.

  9. Identify the given values and the formula for the frequency of a simple pendulum.

    Length of pendulum L=0.5 mL = 0.5 \, \text{m}.
    Frequency f=0.29 Hzf = 0.29 \, \text{Hz}.
    The mass of the body (50 g50 \, \text{g}) is not needed for this calculation.
    The formula for the frequency of a simple pendulum is: f=12πgLf = \frac{1}{2\pi} \sqrt{\frac{g}{L}}.

  10. Rearrange the formula to solve for gg.

    2πf=gL2\pi f = \sqrt{\frac{g}{L}} (2πf)2=gL(2\pi f)^2 = \frac{g}{L} g=L(2πf)2g = L(2\pi f)^2
  11. Substitute the values and calculate gg.

    g=(0.5 m)(2π×0.29 Hz)2g = (0.5 \, \text{m})(2\pi \times 0.29 \, \text{Hz})^2 g=(0.5 m)(1.8221237 s−1)2g = (0.5 \, \text{m})(1.8221237 \, \text{s}^{-1})^2 g=(0.5 m)(3.32014 s−2)g = (0.5 \, \text{m})(3.32014 \, \text{s}^{-2}) g=1.66007 m/s2g = 1.66007 \, \text{m/s}^2

    Rounding to two significant figures:

    g≈1.7 m/s2g \approx 1.7 \, \text{m/s}^2

    The acceleration of gravity on the planet is 1.7 m/s2\boxed{\text{1.7 m/s}^2}.

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