Basic Math: Problem Solving

This is a "recipe" for solving word problems. Slightly rewritten, it can be a guide to solving ANY problem. You've been following this procedure for years, probably unconsciously. While this is not "the only way," if you stick to this procedure, solving problems should become steadily easier.

  1. Write down what is given in the problem. Yes, yes, I know it's right there, but writing it all down on your own sheet of paper helps you focus more.

  2. Determine and write down what you are expected to find. Sometimes this can be the hardest part...

  3. Make a sketch of the problem, labeling all quantities. Sometimes, this may not be necessary.

  4. Find a way to relate what you've been given to what you need to find. Often this involves a formula or equation, which must occasionally be rearranged to suit our needs.

  5. Make sure the units of the data are compatible with the formula and with each other. This is a VITAL step and MUST NOT be omitted!

  6. Perform the calculations and get the answer. Always check your answer to make sure it makes sense!

 

Here's an example of this procedure:

The average distance between the Earth and the Moon is 384,000 km. The Moon takes 27.3 days to orbit the Earth once. What is the Moon's orbital velocity, in km/sec? Assume the Moon's orbit is circular.

 

  1. Our information is all in the problem: Distance between Earth and Moon = 384,000 kilometers and Travel time = 27.3 days.

  2. We want to find v, the orbital velocity, so v = ?

  3. No sketch needed, but we should bear in mind that the Moon travels in a near-circle around the Earth.

  4. The formula for velocity is v = D / T, where D is the distance the object travels, and T is the amount of time it takes to travel. Now the distance the Moon travels in its orbit is not the radius of the orbit; it's the distance around the orbit, called the circumference. The formula for circumference is C = 2(pi)R.

  5. We're asked for the velocity in km/sec, and the distance is in kilometers, so we're halfway there. We must convert the orbital period from days into seconds:
    T = 27.3 days X ( 24 hrs / day ) X ( 60 min / hr ) X ( 60 sec / min )

    T= 2,358,720 seconds
  6. Plug in the values into the formula v = D/T = 2(pi)R/T:
  1.  
    V = 2 (pi) (384,000) / (2,358,720) = 2,412,743 km / 2,358,720 sec

    V = 1.023 km/sec

 

So the velocity of the moon in its orbit is a little over 1 kilometer per second. Pretty fast!
 

Updated 8/25/99
By James E. Heath
  
 
 
Copyright Ó 1999 Austin Community College