| Exam Board | OCR |
|---|---|
| Module | Further Mechanics AS (Further Mechanics AS) |
| Year | 2019 |
| Session | June |
| Marks | 14 |
| Paper | Download PDF ↗ |
| Mark scheme | Download PDF ↗ |
| Topic | Circular Motion 1 |
| Type | Multiple particles on string |
| Difficulty | Standard +0.8 This is a multi-part coupled particles problem requiring force analysis, circular motion equations, algebraic manipulation to show given results, limiting case analysis, and energy calculations. While systematic, it demands careful coordination of multiple concepts (tension forces, centripetal acceleration, equilibrium, energy) across several steps with specific numerical values to show, placing it moderately above average difficulty. |
| Spec | 6.02d Mechanical energy: KE and PE concepts6.02e Calculate KE and PE: using formulae6.05a Angular velocity: definitions6.05b Circular motion: v=r*omega and a=v^2/r |
| Answer | Marks | Guidance |
|---|---|---|
| Answer/Working | Mark | Guidance |
| \(T_2\cos\theta = m_2g\) | M1 | 1.1a – Resolving \(T_2\) vertically and balancing forces on \(R\); do not allow extra forces present. In this solution \(\theta\) is the angle between \(RP\) and \(RA\); sin may be seen instead if \(\theta\) is measured horizontally. |
| \(T_2 = \frac{m_2 \times 9.8}{0.8} = 12.25m_2\) | A1 | 1.1 – Allow use of g, e.g. \(\frac{5}{4}gm_2\); do not allow incomplete expressions e.g. \(\frac{m_2 g}{\sin 53.13}\) |
| [2] |
| Answer | Marks | Guidance |
|---|---|---|
| Answer/Working | Mark | Guidance |
| \(T_2\cos\theta + m_1g = T_1\cos\theta\) | M1 | 3.1b – Vertical forces on \(P\); 3 terms including resolving of \(T_1\); allow sign error. Or \(T_1\cos\theta = m_1g + m_2g\) (equation for the system as a whole) |
| \(T_1 = T_2 + \frac{9.8m_1}{0.8} =\) | A1 | 2.1 – AG Dividing by \(\cos\theta\) (= 0.8), substituting their \(T_2\) and rearranging. Allow 12.25 instead of \(\frac{49}{4}\). At least one intermediate step must be seen. |
| [2] |
| Answer | Marks | Guidance |
|---|---|---|
| Answer/Working | Mark | Guidance |
| \(T_1\sin\theta + T_2\sin\theta = m_1 a\) | M1 | 3.1b – NII horizontally for \(P\); 3 terms including resolving of tensions; allow sign error. Could see \(a\) or \(0.6\omega^2\) or \(\frac{v^2}{0.6}\) or \(\omega^2 r\) or \(\frac{v^2}{r}\) |
| \(12.25(m_1+m_2)\times 0.6 + 12.25m_2\times 0.6 = m_1\times 0.6\omega^2\) | M1 | 1.1 – Substituting for \(T_1\), their \(T_2\), \(\sin\theta\) and \(a\). \(\sin\theta = 0.6\); must be \(a = 0.6\omega^2\) |
| \(\omega^2 = \frac{7.35m_1 + 14.7m_2}{0.6m_1} = \frac{49(m_1+2m_2)}{4m_1}\) | A1 | 2.1 – AG Must see an intermediate step |
| [3] |
| Answer | Marks | Guidance |
|---|---|---|
| Answer/Working | Mark | Guidance |
| E.g. \(m_1 \gg m_2 \Rightarrow \frac{2m_2}{m_1} \approx 0\) or \(\frac{49m_2}{4m_1} \approx 0\) | M1 | 1.1 – Allow argument such as if \(m_1 \gg m_2\) then \(m_1 + 2m_2 \approx m_1\). Do not allow the assumption that \(m_2 = 0\) |
| \(\omega \approx \sqrt{\frac{49m}{4m}} = 3.5\) | A1 | 1.1 – AG \(m\) may be missing. SC1 for result following argument that \(m_2\) is negligible (by comparison with \(m_1\)) without justification, or using trial values of \(m_1\) and \(m_2\) with \(m_1 \gg m_2\). If using trial values, \(m_1\) must be at least \(70 \times m_2\) to give \(\omega = 3.5\) to 1dp. |
| [2] |
| Answer | Marks | Guidance |
|---|---|---|
| Answer/Working | Mark | Guidance |
| \(v = r\omega = 0.6\sqrt{\frac{49\times2.5+98\times2.8}{4\times2.5}}\) | M1 | 1.2 – Use of \(v = r\omega\) with values for \(m_1\) and \(m_2\). (\(v = 3.78\), \(v^2 = 14.2884\)). NB \(\omega = 6.3\) |
| Final energy \(= 2.5\times g\times 1\) | B1 | 1.1 – Assuming zero PE level at 2m below \(A\); other values possible. (24.5) |
| Initial KE \(= \frac{1}{2}\times 2.5\times 0.6^2\times\frac{49\times2.5+98\times2.8}{4\times2.5}\) | M1 | 1.1 – Do not allow use of \(\omega = 3.5\). (17.8605) |
| Initial PE \(= 2.5\times g\times 1.2 + 2.8\times g\times 0.4\) | M1 | 1.1 – oe with different zero PE level. (40.376) |
| Energy loss \(= 17.8605 + 40.376 - 24.5 = 33.7365\) | A1 | 3.2a – awrt 33.7 |
| Alternate method: | ||
| \(v = r\omega = 0.6\sqrt{\frac{49\times2.5+98\times2.8}{4\times2.5}}\) | M1 | Use of \(v = r\omega\) with values for \(m_1\) and \(m_2\). (\(v=3.78\), \(v^2=14.2884\)). NB \(\omega=6.3\) |
| Initial KE \(= \frac{1}{2}\times2.5\times0.6^2\times\frac{49\times2.5+98\times2.8}{4\times2.5}\) | M1 | (17.8605) |
| \(\Delta PE\) for \(m_1 = \pm2.5\times9.8\times(0.8-1)\) | M1 | (\(\pm4.9\)) |
| \(\Delta PE\) for \(m_2 = \pm2.8\times9.8(1.6-2)\) | M1 | (\(\pm10.976\)). Or \(-\Delta PE = 2.5\times9.8\times0.2 + 2.8\times9.8\times0.4\) (\(\pm15.876\)) |
| Energy loss \(= 17.8605 + 4.9 + 10.976\) | A1 | awrt 33.7. Or \(15.876 + 17.8605\) |
| [5] |
## Question 5:
### Part (a):
| Answer/Working | Mark | Guidance |
|---|---|---|
| $T_2\cos\theta = m_2g$ | M1 | 1.1a – Resolving $T_2$ vertically and balancing forces on $R$; do not allow extra forces present. In this solution $\theta$ is the angle between $RP$ and $RA$; sin may be seen instead if $\theta$ is measured horizontally. |
| $T_2 = \frac{m_2 \times 9.8}{0.8} = 12.25m_2$ | A1 | 1.1 – Allow use of g, e.g. $\frac{5}{4}gm_2$; do not allow incomplete expressions e.g. $\frac{m_2 g}{\sin 53.13}$ |
| **[2]** | | |
### Part (b)(i):
| Answer/Working | Mark | Guidance |
|---|---|---|
| $T_2\cos\theta + m_1g = T_1\cos\theta$ | M1 | 3.1b – Vertical forces on $P$; 3 terms including resolving of $T_1$; allow sign error. Or $T_1\cos\theta = m_1g + m_2g$ (equation for the system as a whole) |
| $T_1 = T_2 + \frac{9.8m_1}{0.8} =$ | A1 | 2.1 – **AG** Dividing by $\cos\theta$ (= 0.8), substituting their $T_2$ and rearranging. Allow 12.25 instead of $\frac{49}{4}$. At least one intermediate step must be seen. |
| **[2]** | | |
### Part (b)(ii):
| Answer/Working | Mark | Guidance |
|---|---|---|
| $T_1\sin\theta + T_2\sin\theta = m_1 a$ | M1 | 3.1b – NII horizontally for $P$; 3 terms including resolving of tensions; allow sign error. Could see $a$ or $0.6\omega^2$ or $\frac{v^2}{0.6}$ or $\omega^2 r$ or $\frac{v^2}{r}$ |
| $12.25(m_1+m_2)\times 0.6 + 12.25m_2\times 0.6 = m_1\times 0.6\omega^2$ | M1 | 1.1 – Substituting for $T_1$, their $T_2$, $\sin\theta$ and $a$. $\sin\theta = 0.6$; must be $a = 0.6\omega^2$ |
| $\omega^2 = \frac{7.35m_1 + 14.7m_2}{0.6m_1} = \frac{49(m_1+2m_2)}{4m_1}$ | A1 | 2.1 – **AG** Must see an intermediate step |
| **[3]** | | |
### Part (c):
| Answer/Working | Mark | Guidance |
|---|---|---|
| E.g. $m_1 \gg m_2 \Rightarrow \frac{2m_2}{m_1} \approx 0$ or $\frac{49m_2}{4m_1} \approx 0$ | M1 | 1.1 – Allow argument such as if $m_1 \gg m_2$ then $m_1 + 2m_2 \approx m_1$. Do not allow the assumption that $m_2 = 0$ |
| $\omega \approx \sqrt{\frac{49m}{4m}} = 3.5$ | A1 | 1.1 – **AG** $m$ may be missing. SC1 for result following argument that $m_2$ is negligible (by comparison with $m_1$) without justification, or using trial values of $m_1$ and $m_2$ with $m_1 \gg m_2$. If using trial values, $m_1$ must be at least $70 \times m_2$ to give $\omega = 3.5$ to 1dp. |
| **[2]** | | |
### Part (d):
| Answer/Working | Mark | Guidance |
|---|---|---|
| $v = r\omega = 0.6\sqrt{\frac{49\times2.5+98\times2.8}{4\times2.5}}$ | M1 | 1.2 – Use of $v = r\omega$ with values for $m_1$ and $m_2$. ($v = 3.78$, $v^2 = 14.2884$). NB $\omega = 6.3$ |
| Final energy $= 2.5\times g\times 1$ | B1 | 1.1 – Assuming zero PE level at 2m below $A$; other values possible. (24.5) |
| Initial KE $= \frac{1}{2}\times 2.5\times 0.6^2\times\frac{49\times2.5+98\times2.8}{4\times2.5}$ | M1 | 1.1 – Do not allow use of $\omega = 3.5$. (17.8605) |
| Initial PE $= 2.5\times g\times 1.2 + 2.8\times g\times 0.4$ | M1 | 1.1 – oe with different zero PE level. (40.376) |
| Energy loss $= 17.8605 + 40.376 - 24.5 = 33.7365$ | A1 | 3.2a – awrt 33.7 |
| **Alternate method:** | | |
| $v = r\omega = 0.6\sqrt{\frac{49\times2.5+98\times2.8}{4\times2.5}}$ | M1 | Use of $v = r\omega$ with values for $m_1$ and $m_2$. ($v=3.78$, $v^2=14.2884$). NB $\omega=6.3$ |
| Initial KE $= \frac{1}{2}\times2.5\times0.6^2\times\frac{49\times2.5+98\times2.8}{4\times2.5}$ | M1 | (17.8605) |
| $\Delta PE$ for $m_1 = \pm2.5\times9.8\times(0.8-1)$ | M1 | ($\pm4.9$) |
| $\Delta PE$ for $m_2 = \pm2.8\times9.8(1.6-2)$ | M1 | ($\pm10.976$). Or $-\Delta PE = 2.5\times9.8\times0.2 + 2.8\times9.8\times0.4$ ($\pm15.876$) |
| Energy loss $= 17.8605 + 4.9 + 10.976$ | A1 | awrt 33.7. Or $15.876 + 17.8605$ |
| **[5]** | | |
---
\begin{enumerate}[label=(\alph*)]
\item By considering forces on $R$, express $T _ { 2 }$ in terms of $m _ { 2 }$.
\item Show that
\begin{enumerate}[label=(\roman*)]
\item $T _ { 1 } = \frac { 49 } { 4 } \left( m _ { 1 } + m _ { 2 } \right)$,
\item $\omega ^ { 2 } = \frac { 49 \left( m _ { 1 } + 2 m _ { 2 } \right) } { 4 m _ { 1 } }$.
\end{enumerate}\item Deduce that, in the case where $m _ { 1 }$ is much bigger than $m _ { 2 } , \omega \approx 3.5$.
In a different case, where $m _ { 1 } = 2.5$ and $m _ { 2 } = 2.8 , P$ slows down. Eventually the system comes to rest with $P$ and $R$ hanging in equilibrium.
\item Find the total energy lost by $P$ and $R$ as the angular velocity of $P$ changes from the initial value of $\omega \mathrm { rads } ^ { - 1 }$ to zero.
\end{enumerate}
\hfill \mbox{\textit{OCR Further Mechanics AS 2019 Q5 [14]}}