Knowing your physics formulas is a must, but they’re
useless if you don’t know how to apply them. You will probably
never be asked to calculate the force acting on an object given
its mass and acceleration. Far more likely, you will be asked
for the acceleration given its mass and the force acting on it.
Knowing that F = ma is useless unless you can also sort out that a = F⁄m.
The ETS people don’t want to test your ability to memorize
formulas; they want to test your understanding of formulas and
your ability to use formulas. To this end, they will word questions
in unfamiliar ways and expect you to manipulate familiar equations
in order to get the right answer. Let’s look at an example.
A satellite orbits the Earth at a speed of 1000 m⁄s. Given that the mass of the
Earth is 6.0 × 10 24kg and the universal gravitational constant is
6.67 × 10-11
N · m2 ⁄ kg2,what
is the best approximation for the radius of the satellite’s orbit?
(A) 4 ×10-2m
(B) 4 ×108m
(C) 4 ×1012m
(D) 2.25 ×104m
(E) 2.25 ×1010m
What’s the universal gravitational constant?
Some people will know that this is the G in the equation for
Newton’s Law of Gravitation:F=G(m1)G(m2)/r2.
Other people won’t know that G is called the “universal gravitational constant,”
and ETS will have successfully separated the wheat from the chaff. It’s not
good enough to know some formulas: you have to know what they mean as well.
Given that we know what the universal gravitational constant is,
how do we solve this problem? Well, we know the satellite is moving in
a circular orbit, and we know that the force holding it in this circular
orbit is the force of gravity. If we not only know our formulas, but
also understand them, we will know that the gravitational force must
be equal to the formula for centripetal force,F=mv2/r. If we know
to equate these two formulas, it’s a simple matter of plugging in numbers and solving for r.
Knowing formulas, however, is a small part of getting the right answer. More
important, you need to know how to put these two equations together and solve
for r. On their own, without
understanding how to use them, the equations are useless.
But there are two slightly underhanded ways of getting close to an answer
without knowing any physics equations. These aren’t foolproof methods, but they
might help in a pinch.