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Chapter 6 · Mechanics · Solutions第 6 章 · 力学 · 解答

Energy & Momentum of Rotating Systems, Solutions转动系统的能量与动量, 解答

Companion to the AP-Style Practice Set配套 AP 风格练习题集

EASY MEDIUM HARD

Topics主题 6.1 - 6.6MECH



PART IMultiple Choice · Topics 6.1 - 6.6选择题 · 主题 6.1 - 6.6

Multiple Choice, Worked Answers选择题, 详解

Each item restates the prompt and choices, marks the correct letter, and gives a brief justification. Numbers use $g = 9.8~\mathrm{m/s^2}$, $G = 6.67 \times 10^{-11}~\mathrm{N \cdot m^2/kg^2}$.每道题均重申题目和选项,标注正确答案字母,并给出简要说明。数值取 $g = 9.8~\mathrm{m/s^2}$,$G = 6.67 \times 10^{-11}~\mathrm{N \cdot m^2/kg^2}$。

Q1EASY6.1 Rotational Kinetic Energy6.1 转动动能No Calculator

A flywheel of moment of inertia $I = 2.0~\mathrm{kg \cdot m^2}$ spins about its axis at $\omega = 3.0~\mathrm{rad/s}$. Its rotational kinetic energy is一个转动惯量为 $I = 2.0~\mathrm{kg \cdot m^2}$ 的飞轮以 $\omega = 3.0~\mathrm{rad/s}$ 绕轴旋转。其转动动能为

Answer:答案: (C)
$$K_\text{rot} = \tfrac{1}{2} I \omega^2 = \tfrac{1}{2}(2.0)(3.0)^2 = 9~\mathrm{J}$$
Trap (D) drops the $\tfrac{1}{2}$; (B) forgets to square $\omega$.干扰项 (D) 遗漏了 $\tfrac{1}{2}$;(B) 忘记对 $\omega$ 平方。
Insight.要点。 Rotational kinetic energy is $\tfrac12 I\omega^2$, the direct analogue of $\tfrac12 mv^2$. Both the one half and the square on $\omega$ are required.转动动能是 $\tfrac12 I\omega^2$,与 $\tfrac12 mv^2$ 直接对应。二分之一和 $\omega$ 的平方都不可少。
Q2EASY6.3 Angular Momentum6.3 角动量No Calculator

A particle of mass $2.0~\mathrm{kg}$ moves at $3.0~\mathrm{m/s}$ in a circle of radius $0.50~\mathrm{m}$. The magnitude of its angular momentum about the center of the circle is一个质量为 $2.0~\mathrm{kg}$ 的质点以 $3.0~\mathrm{m/s}$ 的速度在半径 $0.50~\mathrm{m}$ 的圆形轨道上运动。其相对于圆心的角动量大小为

Answer:答案: (B)
For circular motion $\vec v \perp \vec r$, so圆周运动中 $\vec v \perp \vec r$,故
$$L = m v r = 2.0(3.0)(0.50) = 3.0~\mathrm{kg \cdot m^2/s}$$
Insight.要点。 For a particle in circular motion, $\vec r$ and $\vec p$ are perpendicular, so $L=mvr$. Angular momentum has units $kg\cdot m^2/s$, distinct from linear momentum.圆周运动中 $\vec r$ 与 $\vec p$ 垂直,故 $L=mvr$。角动量的单位是 $kg\cdot m^2/s$,与线动量不同。
Q3EASY6.4 Conservation of L6.4 角动量守恒No Calculator

A spinning ice skater pulls her arms in toward her body. With no external torques acting on her, her angular speed一位旋转的花样滑冰运动员将手臂向身体收拢。在没有外力矩作用的情况下,她的角速度

Answer:答案: (A)
$L = I\omega$ is conserved with no external torque. Pulling arms in decreases $I$ (mass closer to the axis), so $\omega$ must increase to compensate. The skater's KE actually goes up, work is done by the arm muscles pulling the mass inward.无外力矩时 $L = I\omega$ 守恒。收拢手臂使 $I$ 减小(质量更靠近轴),故 $\omega$ 必须增大以补偿。运动员的动能实际上增加了,这是手臂肌肉向内拉动质量所做的功。
Insight.要点。 With no external torque, $L=I\omega$ is conserved. Pulling mass inward lowers $I$, so $\omega$ rises; the added kinetic energy comes from the internal work done by the skater's muscles.无外力矩时 $L=I\omega$ 守恒。质量向内收拢使 $I$ 减小,故 $\omega$ 增大;增加的动能来自运动员肌肉所做的内力功。
Q4EASY6.6 Orbital Speed6.6 轨道速度No Calculator

A satellite is in a circular orbit around Earth. As the orbital radius is increased, the satellite's orbital speed一颗卫星围绕地球做圆轨道运动。随着轨道半径增大,卫星的轨道速度

Answer:答案: (B)
Newton's 2nd law in centripetal form gives向心力形式的牛顿第二定律给出
$$v_\text{orb} = \sqrt{\frac{G M}{r}}$$
so $v \propto 1/\sqrt{r}$, larger $r$, smaller speed. Mass-independent.故 $v \propto 1/\sqrt{r}$,轨道半径越大,速度越小,且与卫星质量无关。
Insight.要点。 Circular orbital speed is $v=\sqrt{GM/r}$, so larger orbits are slower. Mass cancels from the satellite side; only the central body's mass and radius matter.圆轨道速度为 $v=\sqrt{GM/r}$,故轨道越大速度越慢。卫星质量会消去;只有中心天体质量和轨道半径起作用。
Q5MEDIUM6.1 Disk vs. Hoop KE6.1 圆盘与圆环转动动能比较No Calculator

A solid disk and a thin hoop have the same mass $M$ and the same radius $R$, and rotate about their central axes at the same angular speed $\omega$. The ratio of the disk's rotational kinetic energy to the hoop's rotational kinetic energy is一个实心圆盘和一个细圆环质量均为 $M$,半径均为 $R$,以相同的角速度 $\omega$ 绕各自的中心轴旋转。圆盘的转动动能与圆环的转动动能之比为

Answer:答案: (B)
$K_\text{rot} \propto I$ at fixed $\omega$. With $I_\text{disk} = \tfrac{1}{2}MR^2$ and $I_\text{hoop} = MR^2$:固定 $\omega$ 时,$K_\text{rot} \propto I$。其中 $I_\text{disk} = \tfrac{1}{2}MR^2$,$I_\text{hoop} = MR^2$:
$$\frac{K_\text{disk}}{K_\text{hoop}} = \frac{I_\text{disk}}{I_\text{hoop}} = \tfrac{1}{2}$$
Insight.要点。 At fixed angular speed, rotational kinetic energy is proportional to moment of inertia. Comparing disk and hoop therefore reduces to comparing $\tfrac12MR^2$ with $MR^2$.角速度相同时,转动动能与转动惯量成正比。比较圆盘与圆环因此归结为比较 $\tfrac12MR^2$ 与 $MR^2$。
Q6MEDIUM6.2 Rotational Work6.2 转动做功No Calculator

A constant torque of $5.0~\mathrm{N \cdot m}$ rotates a wheel through an angular displacement of $4.0~\mathrm{rad}$. The work done on the wheel by the torque is一个大小为 $5.0~\mathrm{N \cdot m}$ 的恒定力矩使一个轮子转过 $4.0~\mathrm{rad}$ 的角位移。该力矩对轮子做的功为

Answer:答案: (C)
$$W = \tau\,\Delta\theta = 5.0(4.0) = 20~\mathrm{J}$$
The rotational analogue of $W = F\,\Delta x$.这是 $W = F\,\Delta x$ 的转动类比。
Insight.要点。 Rotational work is torque times angular displacement: $W=\tau\Delta\theta$. It is the exact analogue of $W=F\Delta x$ for a constant force over a straight displacement.转动功等于力矩乘角位移:$W=\tau\Delta\theta$。它是恒力沿直线位移做功 $W=F\Delta x$ 的精确类比。
Q7MEDIUM6.4 Disk-Drop Collision6.4 圆盘叠落碰撞No Calculator

A disk of moment of inertia $I$ spins about a vertical axis at angular speed $\omega_0$. A second disk of moment of inertia $2I$, initially at rest, is gently dropped onto the first disk and sticks to it. The final angular speed of the combined disks is一个转动惯量为 $I$ 的圆盘以角速度 $\omega_0$ 绕竖直轴旋转。另一个转动惯量为 $2I$ 的圆盘从静止开始轻轻叠落在第一个圆盘上并与之粘合。两圆盘合并后的最终角速度为

Answer:答案: (B)
Angular momentum about the vertical axis is conserved (no external torque):绕竖直轴的角动量守恒(无外力矩):
$$I\,\omega_0 = (I + 2I)\,\omega_f \;\Longrightarrow\; \omega_f = \frac{\omega_0}{3}$$
This is the rotational analogue of a perfectly inelastic collision, KE is not conserved.这是完全非弹性碰撞的转动类比,动能不守恒。
Insight.要点。 Disk-drop collisions conserve angular momentum but not kinetic energy, just like perfectly inelastic linear collisions. The final angular speed follows from the total moment of inertia.圆盘叠落碰撞守恒角动量但不守恒动能,正如完全非弹性线碰撞。最终角速度由总转动惯量决定。
Q8MEDIUM6.5 Sphere Rolling Down Incline6.5 实心球沿斜面滚动No Calculator

A uniform solid sphere is released from rest at the top of an incline of vertical height $h$ and rolls without slipping to the bottom. Its speed at the bottom is一个均匀实心球从高度为 $h$ 的斜面顶端由静止开始释放,无滑动地滚到底部。到达底部时的速度为

Answer:答案: (B)
For rolling without slipping ($\omega = v/R$) with $I_\text{sphere} = \tfrac{2}{5}MR^2$:无滑动滚动时($\omega = v/R$),球的转动惯量 $I_\text{sphere} = \tfrac{2}{5}MR^2$:
$$Mgh = \tfrac{1}{2}M v^2 + \tfrac{1}{2}\bigl(\tfrac{2}{5}MR^2\bigr)\!\left(\tfrac{v}{R}\right)^2 = \tfrac{7}{10} M v^2$$
$$v = \sqrt{\frac{10 g h}{7}}$$
Trap (A) is the frictionless slide; (C) is the answer for a disk ($\sqrt{4gh/3}$).干扰项 (A) 为无摩擦滑动的结果;(C) 为圆盘的结果($\sqrt{4gh/3}$)。
Insight.要点。 Rolling converts height into both translational and rotational kinetic energy. For a solid sphere, $v=\sqrt{10gh/7}$, slower than the frictionless slide $\sqrt{2gh}$.滚动把高度同时转化为平动和转动动能。实心球 $v=\sqrt{10gh/7}$,比无摩擦滑动的 $\sqrt{2gh}$ 慢。
Q9MEDIUM6.6 Kepler's 3rd Law6.6 开普勒第三定律No Calculator

Two satellites orbit the same planet in circular orbits. The orbital radius of satellite 2 is twice that of satellite 1. The ratio $T_2/T_1$ of their orbital periods is两颗卫星在同一行星的圆形轨道上运行。卫星 2 的轨道半径是卫星 1 的两倍。它们的轨道周期之比 $T_2/T_1$ 为

Answer:答案: (B)
$T^2 \propto r^3$, so $T_2/T_1 = (r_2/r_1)^{3/2} = 2^{3/2} = 2\sqrt{2}$.$T^2 \propto r^3$,故 $T_2/T_1 = (r_2/r_1)^{3/2} = 2^{3/2} = 2\sqrt{2}$。
Insight.要点。 Kepler's third law gives $T\propto r^{3/2}$ for circular orbits. A doubled radius multiplies the period by $2^{3/2}=2\sqrt2$, not by two.圆轨道的开普勒第三定律给出 $T\propto r^{3/2}$。半径翻倍使周期变为 $2^{3/2}=2\sqrt2$ 倍,而不是两倍。
Q10MEDIUM6.3 Angular Impulse6.3 角冲量No Calculator

A constant net torque of $4.0~\mathrm{N \cdot m}$ acts on a wheel of moment of inertia $2.0~\mathrm{kg \cdot m^2}$, initially at rest, for $3.0~\mathrm{s}$. The wheel's final angular speed is一个大小为 $4.0~\mathrm{N \cdot m}$ 的恒定合力矩作用在转动惯量为 $2.0~\mathrm{kg \cdot m^2}$ 的轮子上,持续时间 $3.0~\mathrm{s}$,轮子初始静止。轮子的最终角速度为

Answer:答案: (C)
Angular impulse $= \Delta L$:角冲量 $= \Delta L$:
$$\tau\,\Delta t = I\,\omega \;\Longrightarrow\; \omega = \frac{4.0(3.0)}{2.0} = 6.0~\mathrm{rad/s}$$
Insight.要点。 Angular impulse equals change in angular momentum: $\tau\Delta t=I\omega$. It is the rotational version of $F\Delta t=\Delta p$.角冲量等于角动量变化:$\tau\Delta t=I\omega$。它是 $F\Delta t=\Delta p$ 的转动版本。
Q11MEDIUM6.5 Rolling KE Fraction6.5 滚动动能占比No Calculator

A uniform solid disk rolls without slipping along a horizontal surface with center-of-mass speed $v$. The fraction of its total kinetic energy that is rotational is一个均匀实心圆盘以质心速度 $v$ 在水平面上无滑动地滚动。其总动能中转动动能所占的比例为

Answer:答案: (B)
With $I = \tfrac{1}{2}MR^2$ and $\omega = v/R$:利用 $I = \tfrac{1}{2}MR^2$,$\omega = v/R$:
$$K_\text{trans} = \tfrac{1}{2}M v^2,\qquad K_\text{rot} = \tfrac{1}{2}I\omega^2 = \tfrac{1}{4}M v^2$$
$$\frac{K_\text{rot}}{K_\text{total}} = \frac{1/4}{1/2 + 1/4} = \frac{1/4}{3/4} = \tfrac{1}{3}$$
For a hoop, this fraction is $\tfrac{1}{2}$; for a sphere, $\tfrac{2}{7}$.对于圆环,该比例为 $\tfrac{1}{2}$;对于实心球,为 $\tfrac{2}{7}$。
Insight.要点。 Rolling energy splits by shape. For a disk, rotational energy is one third of the total; for a hoop it is one half; for a sphere it is two sevenths. The no-slip condition fixes the split.滚动能量的分配取决于形状。圆盘转动能占总能三分之一,圆环占二分之一,实心球占七分之二。不打滑条件固定了这一分配。
Q12MEDIUM6.4 Bullet-into-Pivoted-Rod6.4 子弹射入转动杆No Calculator

A uniform rod of mass $M$ and length $L$, pivoted at one end and initially at rest, is struck and embedded by a bullet of mass $m$ moving with speed $v$ at the rod's free end (perpendicular to the rod). The angular speed of the rod-plus-bullet system just after the collision is一根质量为 $M$、长度为 $L$ 的均匀细杆,一端铰支,初始静止,被质量为 $m$、速度为 $v$ 的子弹垂直射入其自由端并嵌入其中。碰撞后,杆与子弹组合体的角速度为

Answer:答案: (B)
Conserve angular momentum about the pivot. Bullet's $L_\text{before} = m v L$ (perpendicular at distance $L$). After collision, $I_\text{tot} = \tfrac{1}{3}ML^2 + mL^2 = L^2(M/3 + m)$.对铰支点应用角动量守恒。子弹的初始角动量 $L_\text{before} = m v L$(在距铰支点 $L$ 处垂直射入)。碰撞后,$I_\text{tot} = \tfrac{1}{3}ML^2 + mL^2 = L^2(M/3 + m)$。
$$m v L = L^2\!\left(\tfrac{M}{3} + m\right)\,\omega \;\Longrightarrow\; \omega = \frac{m v}{L\bigl(M/3 + m\bigr)}$$
Insight.要点。 For a bullet embedding in a pivoted rod, conserve angular momentum about the pivot, not linear momentum: the pivot exerts an external force. The bullet's initial angular momentum is $mvL$.子弹嵌入绕轴杆时,应绕转轴守恒角动量,而不是线动量,因为转轴提供外力。子弹初始角动量为 $mvL$。
Q13MEDIUM6.1 Work to Stop Wheel6.1 使轮子停转所做的功No Calculator

A wheel of moment of inertia $0.50~\mathrm{kg \cdot m^2}$ spins at $4.0~\mathrm{rad/s}$. The magnitude of the work that must be done on the wheel to bring it to rest is一个转动惯量为 $0.50~\mathrm{kg \cdot m^2}$ 的轮子以 $4.0~\mathrm{rad/s}$ 旋转。使轮子停止旋转所需做的功的大小为

Answer:答案: (C)
$$|W| = |\Delta K_\text{rot}| = \tfrac{1}{2}I\omega^2 = \tfrac{1}{2}(0.50)(16) = 4.0~\mathrm{J}$$
Insight.要点。 The work needed to stop a rotating object equals its initial rotational kinetic energy. Compute $\tfrac12 I\omega^2$; no distance or torque history is needed.使旋转物体停下所需功等于其初始转动动能。直接计算 $\tfrac12 I\omega^2$,无需知道距离或力矩历程。
Q14HARD6.4 Person on Rotating Platform6.4 人站在旋转台上Calculator

A horizontal turntable of moment of inertia $I_p = 100~\mathrm{kg \cdot m^2}$ rotates freely about a vertical axis at $\omega_0 = 1.0~\mathrm{rad/s}$. A person of mass $50~\mathrm{kg}$ stands at rest on the turntable at $r = 1.0~\mathrm{m}$ from the axis. The person then walks to the axis (treat the person as a point mass throughout). The new angular speed of the turntable is一个转动惯量为 $I_p = 100~\mathrm{kg \cdot m^2}$ 的水平转台以 $\omega_0 = 1.0~\mathrm{rad/s}$ 绕竖直轴自由旋转。一个质量为 $50~\mathrm{kg}$ 的人静止站在距轴 $r = 1.0~\mathrm{m}$ 处。该人随后走向轴心(全程将人视为质点)。转台的新角速度为

Answer:答案: (C)
Angular momentum about the axis is conserved. With person on the platform, person and platform share $\omega$.绕轴的角动量守恒。人站在转台上时,人与转台共享同一 $\omega$。
$$\bigl(I_p + m r^2\bigr)\,\omega_0 = I_p\,\omega_f$$
$$\omega_f = \frac{(100 + 50)(1.0)}{100} = 1.5~\mathrm{rad/s}$$
Moving inward reduces the system's $I$, so $\omega$ rises (same idea as the skater).向内移动减小了系统的 $I$,故 $\omega$ 增大(与花样滑冰运动员原理相同)。
Insight.要点。 A person walking inward on a turntable changes the system's moment of inertia, so the platform speeds up. Angular momentum conservation relates the initial and final $I\omega$ values.人在转台上向内走动会改变系统转动惯量,转台因此加速。角动量守恒联系前后 $I\omega$。
Q15HARD6.6 Geosynchronous Orbit6.6 地球同步轨道Calculator

A satellite is placed in a circular orbit such that its orbital period equals one Earth day. Take $GM_\mathrm{E} = 4.0 \times 10^{14}~\mathrm{m^3/s^2}$ and $T_\mathrm{day} = 8.64 \times 10^4~\mathrm{s}$. The orbital radius (measured from Earth's center) is closest to一颗卫星被置于圆形轨道上,使其轨道周期等于地球自转一天。取 $GM_\mathrm{E} = 4.0 \times 10^{14}~\mathrm{m^3/s^2}$,$T_\mathrm{day} = 8.64 \times 10^4~\mathrm{s}$。轨道半径(从地心算起)最接近

Answer:答案: (C)
Kepler's 3rd law: $T^2 = \dfrac{4\pi^2}{GM_\mathrm{E}}\,r^3$.开普勒第三定律:$T^2 = \dfrac{4\pi^2}{GM_\mathrm{E}}\,r^3$。
$$r^3 = \frac{G M_\mathrm{E}\,T^2}{4\pi^2} = \frac{(4.0 \times 10^{14})(8.64 \times 10^4)^2}{4\pi^2}$$
$$r^3 \approx \frac{2.99 \times 10^{24}}{39.5} \approx 7.56 \times 10^{22}~\mathrm{m^3}$$
$$r \approx 4.22 \times 10^7~\mathrm{m} = 4.2 \times 10^4~\mathrm{km}$$
Trap (D) is roughly the lunar orbital radius; (B) is the altitude above Earth's surface ($r - R_\mathrm{E}$).干扰项 (D) 约为月球轨道半径;(B) 为高于地球表面的轨道高度($r - R_\mathrm{E}$)。
Insight.要点。 Geosynchronous radius follows from setting $T$ equal to one sidereal day in Kepler's law. Distinguish orbital radius from altitude: altitude is radius minus Earth's radius.地球同步轨道半径由开普勒定律中令 $T$ 等于一个恒星日求得。要区分轨道半径与高度:高度等于半径减地球半径。
Q16HARD6.5 Race Down the Incline6.5 斜面竞速No Calculator

A solid sphere, a uniform solid disk, and a thin hoop, all of mass $M$ and radius $R$, are released simultaneously from rest at the top of the same incline and roll without slipping to the bottom. Which arrives first?一个实心球、一个均匀实心圆盘和一个细圆环,质量均为 $M$,半径均为 $R$,同时从同一斜面顶端由静止释放,无滑动地滚到底部。哪个最先到达?

Answer:答案: (A)
For rolling-without-slipping, energy conservation gives无滑动滚动时,能量守恒给出
$$v_\text{bottom} = \sqrt{\frac{2 g h}{1 + I/(MR^2)}}$$
Smaller $I/(MR^2)$ $\Rightarrow$ larger $v$. With $\tfrac{2}{5}, \tfrac{1}{2}, 1$ for sphere/disk/hoop, the sphere wins. Mass and radius drop out, only the shape's $I/(MR^2)$ ratio matters.$I/(MR^2)$ 越小,$v$ 越大。球、圆盘、圆环对应的值分别为 $\tfrac{2}{5}$、$\tfrac{1}{2}$、$1$,故实心球最先到达。质量和半径消去,只有形状的 $I/(MR^2)$ 比值起作用。
Insight.要点。 Rolling race outcomes depend only on the dimensionless shape factor $I/(MR^2)$. The sphere wins over the disk, which wins over the hoop; mass and radius cancel.滚动竞速结果只取决于无量纲形状因子 $I/(MR^2)$。实心球快于圆盘,圆盘快于圆环;质量和半径均消去。
Q17HARD6.3 Direction of Angular Momentum6.3 角动量的方向No Calculator

A particle moves in a circular path in the $xy$-plane, traveling counter-clockwise as viewed from the $+z$ axis. Its angular momentum about the center of the circle points in the一个质点在 $xy$ 平面内沿圆形轨道运动,从 $+z$ 轴方向俯视为逆时针。其相对于圆心的角动量指向

Answer:答案: (C)
$\vec L = \vec r \times \vec p$. Right-hand rule with $\vec r$ in the $xy$-plane and $\vec p$ tangent to the circle (also in the $xy$-plane) gives $\vec L$ perpendicular to the plane, along $+\hat k$ for counter-clockwise motion viewed from $+z$ (the "spin direction of the angular-velocity vector"). Trap (D) reverses the sense.$\vec L = \vec r \times \vec p$。$\vec r$ 在 $xy$ 平面内,$\vec p$ 与圆相切(也在 $xy$ 平面内),右手定则给出 $\vec L$ 垂直于该平面,从 $+z$ 方向观察逆时针运动时沿 $+\hat k$ 方向(即角速度矢量的方向)。干扰项 (D) 方向相反。
Insight.要点。 Angular momentum direction comes from the right-hand rule for $\vec r\times\vec p$. Counterclockwise motion viewed from $+z$ points along $+\hat k$, independent of the particle's mass.角动量方向由 $\vec r\times\vec p$ 的右手定则确定。从 $+z$ 俯视逆时针运动时指向 $+\hat k$,与粒子质量无关。
Q18HARD6.6 Total Orbital Energy6.6 轨道总机械能No Calculator

A satellite of mass $m$ orbits a planet of mass $M$ in a circular orbit of radius $r$. The total mechanical energy of the satellite is质量为 $m$ 的卫星在质量为 $M$ 的行星的半径为 $r$ 的圆形轨道上运行。卫星的总机械能为

Answer:答案: (B)
For a circular orbit, $v^2 = GM/r$, so $K = \tfrac{1}{2}m v^2 = \tfrac{GMm}{2r}$. With $U = -GMm/r$:圆轨道上 $v^2 = GM/r$,故 $K = \tfrac{1}{2}m v^2 = \tfrac{GMm}{2r}$。其中 $U = -GMm/r$:
$$E = K + U = \frac{G M m}{2r} - \frac{G M m}{r} = -\frac{G M m}{2r}$$
The negative sign signals a bound state. Note $E = -K$ and $U = 2E$, the "virial" relations.负号表明这是束缚态。注意 $E = -K$,$U = 2E$,即"维里定理"关系。
Insight.要点。 A bound circular orbit has negative total energy $E=-GMm/(2r)$. The kinetic energy is positive and half the magnitude of the potential energy, a virial relation for inverse-square forces.束缚圆轨道总能量为负:$E=-GMm/(2r)$。动能是正的,大小为势能绝对值的一半,这是平方反比力的维里关系。
PART IIFree-Response · Topics 6.1 - 6.6自由回答题 · 主题 6.1 - 6.6

Free-Response, Worked Solutions自由回答题, 完整解答

Each FRQ walks every part in the canonical setup → execute → evaluate structure.每道自由回答题均按照"建立模型 → 执行计算 → 评估结果"的标准结构逐步讲解。

FRQ 1MEDIUM6.4 Disk-on-Disk Collision6.4 圆盘叠落碰撞Calculator

$M = 2.0~\mathrm{kg}$, $R = 0.30~\mathrm{m}$ disk spinning at $\omega_0 = 6.0~\mathrm{rad/s}$; identical disk dropped from rest and sticks.$M = 2.0~\mathrm{kg}$,$R = 0.30~\mathrm{m}$ 的圆盘以 $\omega_0 = 6.0~\mathrm{rad/s}$ 旋转;相同圆盘从静止叠落并粘合。

(a) Per disk: $I = \tfrac{1}{2}MR^2 = \tfrac{1}{2}(2.0)(0.30)^2 = 0.090~\mathrm{kg \cdot m^2}$.每个圆盘:$I = \tfrac{1}{2}MR^2 = \tfrac{1}{2}(2.0)(0.30)^2 = 0.090~\mathrm{kg \cdot m^2}$。
(b) Angular momentum conserved about the vertical axis (the friction between the disks is an internal torque):绕竖直轴的角动量守恒(两圆盘之间的摩擦力是内力矩):
$$I\,\omega_0 = (2I)\,\omega_f \;\Longrightarrow\; \omega_f = \frac{\omega_0}{2} = 3.0~\mathrm{rad/s}$$
(c) Rotational KE before and after:合并前后的转动动能:
$$K_i = \tfrac{1}{2} I \omega_0^2 = \tfrac{1}{2}(0.090)(36) = 1.62~\mathrm{J}$$
$$K_f = \tfrac{1}{2}(2I) \omega_f^2 = \tfrac{1}{2}(0.180)(9) = 0.81~\mathrm{J}$$
(d) Fraction of $K_i$ lost: $(1.62 - 0.81)/1.62 = 0.50$, exactly half. The missing $0.81~\mathrm{J}$ is dissipated as heat / sound / surface deformation during the brief slip between the two disks as they reach a common $\omega$. This is the rotational analogue of a perfectly inelastic linear collision (KE not conserved).$K_i$ 的损失比例:$(1.62 - 0.81)/1.62 = 0.50$,恰好一半。缺失的 $0.81~\mathrm{J}$ 在两圆盘达到共同 $\omega$ 过程中通过短暂滑动以热能、声音和表面形变的形式耗散。这是完全非弹性线性碰撞的转动类比(动能不守恒)。
Insight.要点。 Two disks reaching a common angular speed conserve angular momentum but lose kinetic energy to internal friction. For equal disks, the final speed halves and exactly half the initial energy is dissipated.两个圆盘达到共同角速度时角动量守恒,但动能因内摩擦损失。对相同圆盘,末角速度减半,恰好损失一半初始能量。
FRQ 2MEDIUM6.5 Sphere Rolling Down Incline6.5 实心球沿斜面滚动Calculator

$M = 0.50~\mathrm{kg}$, $R = 0.10~\mathrm{m}$ solid sphere, released from rest at vertical height $h = 0.80~\mathrm{m}$ on an incline of $\theta = 30^\circ$, rolls without slipping.$M = 0.50~\mathrm{kg}$,$R = 0.10~\mathrm{m}$ 的实心球,从倾角 $\theta = 30^\circ$、竖直高度 $h = 0.80~\mathrm{m}$ 处由静止释放,无滑动地滚动。

(a) Energy conservation with $I = \tfrac{2}{5}MR^2$ and $\omega = v/R$:利用 $I = \tfrac{2}{5}MR^2$,$\omega = v/R$ 进行能量守恒:
$$M g h = \tfrac{1}{2} M v^2 + \tfrac{1}{2}\bigl(\tfrac{2}{5}MR^2\bigr)\!\left(\tfrac{v}{R}\right)^2 = \tfrac{7}{10} M v^2$$
$$v = \sqrt{\frac{10 g h}{7}}$$
(b) Numerical value:数值结果:
$$v = \sqrt{\frac{10(9.8)(0.80)}{7}} = \sqrt{11.2} \approx 3.35~\mathrm{m/s}$$
(c) Newton's 2nd law. Translation: $M g\sin\theta - f_s = M a$. Rotation about CM: $f_s R = I\alpha = \tfrac{2}{5}MR^2\alpha$, and $a = R\alpha$ gives $f_s = \tfrac{2}{5}M a$. Substitute:牛顿第二定律。平动:$M g\sin\theta - f_s = M a$。绕质心转动:$f_s R = I\alpha = \tfrac{2}{5}MR^2\alpha$,$a = R\alpha$ 给出 $f_s = \tfrac{2}{5}M a$。代入:
$$M g\sin\theta - \tfrac{2}{5} M a = M a \;\Longrightarrow\; a = \tfrac{5}{7}\,g\sin\theta$$
(d) Static-friction force is $f_s = \tfrac{2}{5}M a = \tfrac{2}{7} M g\sin\theta$. Constraint $f_s \le \mu_s\,M g\cos\theta$:静摩擦力 $f_s = \tfrac{2}{5}M a = \tfrac{2}{7} M g\sin\theta$。约束条件 $f_s \le \mu_s\,M g\cos\theta$:
$$\mu_s \ge \tfrac{2}{7}\tan\theta = \tfrac{2}{7}\tan 30^\circ \approx 0.165$$
Insight.要点。 For a rolling sphere, the no-slip constraint $a=R\alpha$ gives the friction force and hence the minimum $\mu_s$ for rolling. Without enough friction, the object slides instead of rolling cleanly.对滚动球体,不打滑约束 $a=R\alpha$ 给出摩擦力,从而得到无滑动滚动所需的最小 $\mu_s$。摩擦不足时物体会滑动而非纯滚动。
FRQ 3HARD6.3 / 6.4 Bullet-into-Rod (Ballistic)6.3 / 6.4 子弹射入杆(弹道实验)Calculator

Rod $M = 0.50~\mathrm{kg}$, $L = 0.80~\mathrm{m}$, pivoted at one end, hanging vertically. Bullet $m = 0.020~\mathrm{kg}$ at $v_0 = 200~\mathrm{m/s}$ strikes the free end horizontally and embeds.杆 $M = 0.50~\mathrm{kg}$,$L = 0.80~\mathrm{m}$,一端铰支,竖直悬挂。子弹 $m = 0.020~\mathrm{kg}$,以 $v_0 = 200~\mathrm{m/s}$ 水平射入自由端并嵌入。

(a) Moment of inertia about the pivot:绕铰支点的转动惯量:
$$I = \tfrac{1}{3}ML^2 + mL^2 = \tfrac{1}{3}(0.50)(0.64) + (0.020)(0.64) \approx 0.1195~\mathrm{kg \cdot m^2}$$
(b) Angular momentum about the pivot is conserved through the collision. Bullet's incoming $L = m v_0 L$:碰撞过程中绕铰支点的角动量守恒。子弹的初始角动量 $L = m v_0 L$:
$$m v_0 L = I\,\omega \;\Longrightarrow\; \omega = \frac{m v_0 L}{I} = \frac{(0.020)(200)(0.80)}{0.1195} \approx 26.8~\mathrm{rad/s}$$
(c) Center of mass of rod-plus-bullet, measured from the pivot:杆与子弹组合体的质心,从铰支点量起:
$$x_\text{cm} = \frac{M(L/2) + m L}{M + m} = \frac{0.50(0.40) + 0.020(0.80)}{0.520} \approx 0.415~\mathrm{m}$$
Energy after the collision is $K_\text{rot} = \tfrac{1}{2}I\omega^2 \approx 42.9~\mathrm{J}$. To swing up by angle $\theta$ from vertical, the CM rises by $x_\text{cm}(1 - \cos\theta)$. Setting $K_\text{rot} = (M+m) g\,x_\text{cm}(1 - \cos\theta)$:碰撞后的转动动能为 $K_\text{rot} = \tfrac{1}{2}I\omega^2 \approx 42.9~\mathrm{J}$。摆动至偏离竖直方向 $\theta$ 时,质心上升 $x_\text{cm}(1 - \cos\theta)$。令 $K_\text{rot} = (M+m) g\,x_\text{cm}(1 - \cos\theta)$:
$$1 - \cos\theta = \frac{42.9}{(0.520)(9.8)(0.415)} \approx 20.3$$
⚠ This implies $\cos\theta \approx -19.3$, which is impossible. The post-collision rotational KE ($42.9~\mathrm{J}$) exceeds the maximum gravitational PE barrier ($2(M+m)g\,x_\text{cm} \approx 4.23~\mathrm{J}$) by nearly 10×, so the system passes over the top and continues to rotate. There is no momentary stop with the given parameters; the rod-plus-bullet executes full rotations. For a finite swing-up angle, $v_0$ would need to be roughly $10\times$ smaller (e.g. $\sim 20~\mathrm{m/s}$ gives $\theta \approx 37^\circ$).⚠ 这意味着 $\cos\theta \approx -19.3$,这在物理上不可能。碰撞后的转动动能($42.9~\mathrm{J}$)是最大重力势能壁垒($2(M+m)g\,x_\text{cm} \approx 4.23~\mathrm{J}$)的近 10 倍,因此系统越过最高点并继续旋转。在给定参数下不存在瞬间停止,杆与子弹组合体做完整圆周运动。若要得到有限摆角,$v_0$ 需约减小 10 倍(例如 $\sim 20~\mathrm{m/s}$ 时 $\theta \approx 37^\circ$)。
(d) KE accounting:动能核算:
$$K_\text{bullet, initial} = \tfrac{1}{2}m v_0^2 = \tfrac{1}{2}(0.020)(200)^2 = 400~\mathrm{J}$$
$$\frac{\Delta K}{K_i} = \frac{400 - 42.9}{400} \approx 0.893~~(89\%~\text{lost})$$
Even though angular momentum is conserved, most of the bullet's KE is dissipated into the rod's deformation as the bullet embeds.尽管角动量守恒,子弹大部分动能在嵌入过程中以杆的形变方式耗散。
Insight.要点。 A ballistic rod collision conserves angular momentum during impact but not kinetic energy. After impact, mechanical energy is conserved during the swing, so the two stages use different laws.弹道杆碰撞在撞击瞬间守恒角动量但不守恒动能。撞击后摆动阶段机械能守恒,因此两个阶段使用不同定律。
FRQ 4HARD6.6 Orbital Mechanics6.6 轨道力学Calculator

$m = 500~\mathrm{kg}$ satellite at $r_1 = 1.5\,R_\mathrm{E}$ ($R_\mathrm{E} = 6.4 \times 10^6~\mathrm{m}$, $M_\mathrm{E} = 6.0 \times 10^{24}~\mathrm{kg}$).$m = 500~\mathrm{kg}$ 的卫星位于 $r_1 = 1.5\,R_\mathrm{E}$ 轨道($R_\mathrm{E} = 6.4 \times 10^6~\mathrm{m}$,$M_\mathrm{E} = 6.0 \times 10^{24}~\mathrm{kg}$)。

(a) Centripetal: $\dfrac{G M_\mathrm{E} m}{r_1^2} = \dfrac{m v_1^2}{r_1}$, so $v_1 = \sqrt{G M_\mathrm{E}/r_1}$. With $r_1 = 9.6 \times 10^6~\mathrm{m}$:向心力:$\dfrac{G M_\mathrm{E} m}{r_1^2} = \dfrac{m v_1^2}{r_1}$,故 $v_1 = \sqrt{G M_\mathrm{E}/r_1}$。取 $r_1 = 9.6 \times 10^6~\mathrm{m}$:
$$v_1 = \sqrt{\frac{(6.67 \times 10^{-11})(6.0 \times 10^{24})}{9.6 \times 10^6}} = \sqrt{4.17 \times 10^7} \approx 6.46 \times 10^3~\mathrm{m/s}$$
(b) Period: $T_1 = 2\pi r_1 / v_1$.周期:$T_1 = 2\pi r_1 / v_1$。
$$T_1 = \frac{2\pi(9.6 \times 10^6)}{6.46 \times 10^3} \approx 9.34 \times 10^3~\mathrm{s} \approx 2.6~\mathrm{h}$$
(c) Total mechanical energy:总机械能:
$$E_1 = -\frac{G M_\mathrm{E} m}{2 r_1} = -\frac{(6.67 \times 10^{-11})(6.0 \times 10^{24})(500)}{2(9.6 \times 10^6)} \approx -1.04 \times 10^{10}~\mathrm{J}$$
(d) Higher orbit at $r_2 = 2.0\,R_\mathrm{E} = 1.28 \times 10^7~\mathrm{m}$:更高轨道 $r_2 = 2.0\,R_\mathrm{E} = 1.28 \times 10^7~\mathrm{m}$:
$$E_2 = -\frac{G M_\mathrm{E} m}{2 r_2} \approx -7.82 \times 10^9~\mathrm{J}$$
Work an external agent must do:外力需做的功:
$$W_\text{ext} = E_2 - E_1 \approx -7.82 \times 10^9 - (-1.04 \times 10^{10}) \approx +2.6 \times 10^9~\mathrm{J}$$
Positive, raising the orbit costs energy (the satellite ends with more total mechanical energy, even though it moves slower; the PE rise outweighs the KE drop).结果为正,说明升高轨道需要输入能量(卫星的总机械能增大,尽管速度降低,势能的增加超过了动能的减少)。
Insight.要点。 Orbital energy is negative for a bound orbit and becomes less negative at larger radius. Raising an orbit requires positive external work even though the satellite slows down, because potential energy increases more than kinetic energy decreases.束缚轨道的轨道能量为负,轨道越大负得越少。抬高轨道需要正的功,即使卫星速度变慢,因为势能增加量超过动能减少量。