FRQ: Gravitational Potential Energy in Free Fall — The Sentinel Payload Drop
Solution▸ earns credit ⚠︎ common error, partial credit ✗ common error, no credit
- Sketch and label a line or curve that represents the gravitational potential energy U of the Earth–payload system as a function of r.
- Sketch and label a line or curve that represents the total mechanical energy E of the Earth–payload system as a function of r during the drop.
- Sketch and label a line or curve that represents the kinetic energy K of the payload as a function of r during the drop.
Part C — Model Answer
The gravitational potential energy of the Earth–payload system is U = −GM_E m/r. With GM_E m/R_E = 2.50 × 10¹⁰ J,
U = −(2.50 × 10¹⁰ J)(R_E/r)
r = R_E: U = −2.50 × 10¹⁰ J
r = 2R_E: U = −1.25 × 10¹⁰ J
r = 4R_E: U = −0.625 × 10¹⁰ J
U is negative at every finite r because its zero is at infinite separation and gravity is attractive: moving the payload outward toward that zero takes energy. Doubling r halves the magnitude of U, so the curve rises steeply near Earth and flattens as r increases, approaching zero without reaching it (−0.417 × 10¹⁰ J at r = 6R_E). U depends only on the separation, so it is defined at every r in the range.
The system’s mechanical energy is constant (part B) and is fixed at release, where K = 0:
E = K + U = 0 + (−0.625 × 10¹⁰ J) = −0.625 × 10¹⁰ J
so E is a horizontal line at −0.625 × 10¹⁰ J. The kinetic energy at each r is K = E − U, the vertical gap from the U curve up to the E line: zero at r = 4R_E, 0.625 × 10¹⁰ J at r = 2R_E, which is ½mv_2² from part B, and 1.875 × 10¹⁰ J at r = R_E.
The kinetic energy at each r is the gap between the E line and the U curve, so the payload can only be where the E line lies on or above the U curve. For r > 4R_E, U is greater than E, and K = E − U would be negative, which is impossible: the payload, released from rest and falling inward, never reaches those separations, so K is not defined there.
Scoring (4 points):
▸C1 — 1 point: For sketching a line or curve, labelled as the gravitational potential energy, that is negative from r = R_E to r = 6R_E, increases as r increases, and becomes less steep as r increases without reaching zero.
▸C2 — 1 point: For a U curve at −2.50 × 10¹⁰ J at r = R_E, −1.25 × 10¹⁰ J at r = 2R_E and −0.625 × 10¹⁰ J at r = 4R_E.
▸C3 — 1 point: For sketching a horizontal line, labelled as the total mechanical energy, at −0.625 × 10¹⁰ J or at the value of the response’s own U curve at r = 4R_E, continuous from r = R_E to at least r = 4R_E.
▸C4 — 1 point: For sketching a line or curve, labelled as the kinetic energy, that is zero at r = 4R_E, increases as r decreases, and is not drawn for r > 4R_E, with values of 0.625 × 10¹⁰ J at r = 2R_E and 1.875 × 10¹⁰ J at r = R_E, or with values equal at each r to the vertical distance from the response’s own U curve up to its own E line.
⚠︎Common error (partial credit): Joins −2.50 × 10¹⁰ J at r = R_E and −0.625 × 10¹⁰ J at r = 4R_E with a straight line, as if U changed by the same amount for each metre of the fall, with E and K consistent with it — earns 2 of 4 points, C3 and C4. That line gives −1.875 × 10¹⁰ J at r = 2R_E, not −1.25 × 10¹⁰ J, and reaches zero at r = 5R_E; the field weakens with distance from Earth.