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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。
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
$$L = m v r = 2.0(3.0)(0.50) = 3.0~\mathrm{kg \cdot m^2/s}$$
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。
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。
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 $I_\text{disk} = \tfrac{1}{2}MR^2$,$I_\text{hoop} = MR^2$:
$$\frac{K_\text{disk}}{K_\text{hoop}} = \frac{I_\text{disk}}{I_\text{hoop}} = \tfrac{1}{2}$$
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。
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,动能守恒。
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($\sqrt{4gh/3}$)。
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 $T_2/T_1 = (r_2/r_1)^{3/2} = 2^{3/2} = 2\sqrt{2}$。
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 $= \Delta L$:
$$\tau\,\Delta t = I\,\omega \;\Longrightarrow\; \omega = \frac{4.0(3.0)}{2.0} = 6.0~\mathrm{rad/s}$$
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 $\tfrac{2}{7}$。
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,$I_\text{tot} = \tfrac{1}{3}ML^2 + mL^2 = L^2(M/3 + m)$。
$$m v L = L^2\!\left(\tfrac{M}{3} + m\right)\,\omega \;\Longrightarrow\; \omega = \frac{m v}{L\bigl(M/3 + m\bigr)}$$
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)
$$|W| = |\Delta K_\text{rot}| = \tfrac{1}{2}I\omega^2 = \tfrac{1}{2}(0.50)(16) = 4.0~\mathrm{J}$$
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)。
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($r - R_\mathrm{E}$)。
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。
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。
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。
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)。
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 $f_s \le \mu_s\,M g\cos\theta$:
$$\mu_s \ge \tfrac{2}{7}\tan\theta = \tfrac{2}{7}\tan 30^\circ \approx 0.165$$
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。
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)。