25.1.1 A Gravitational Analogy

Gravity, like electricity, is a long-range force. Much as we defined the electric field E⃗=F⃗on q/q, we can also define a gravitational field—the agent that exerts gravitational forces on masses—as F⃗on m/m. But F⃗on m=mg⃗ near the earth’s surface; thus the familiar g⃗=(9.80 N/kg, down) is really the gravitational field! Notice how we’ve written the units of g⃗ as N/kg, but you can easily show that N/kg=m/s2. The gravitational field near the earth’s surface is a uniform field in the downward direction.

FIGURE 25.2 shows a particle of mass m falling in the gravitational field. The gravitational force is in the same direction as the particle’s displacement, so the gravitational field does a positive amount of work on the particle. The gravitational force is constant, hence the work done by the gravitational field is

WG=FG Δr cos 0°=mg|yf−yi|=mgyi−mgyf  (25.5)

We have to be careful with signs because Δr, the magnitude of the displacement vector, must be a positive number.

FIGURE 25.2 Potential energy is transformed into kinetic energy as a particle moves in a gravitational field.

The figure illustrates the transformation of a particle's potential energy into kinetic energy as the particle moves in a gravitational field.
FIGURE 25.2 Full Alternative Text

Now we can see how the definition of ΔU in Equation 25.2 makes sense. The change in gravitational potential energy is

ΔUG=Uf−Ui=−WG(i→f)=mgyf−mgyi  (25.6)

Comparing the initial and final terms on the two sides of the equation, we see that the gravitational potential energy near the earth is the familiar quantity

UG=mgy (25.7)

We could add a constant to UG, but we’ve made the customary choice that UG=0 at y=0.