Edexcel M3 2015 June — Question 2 9 marks

Exam BoardEdexcel
ModuleM3 (Mechanics 3)
Year2015
SessionJune
Marks9
PaperDownload PDF ↗
Mark schemeDownload PDF ↗
TopicAdvanced work-energy problems
TypeInverse-square gravitational force
DifficultyStandard +0.3 This is a standard M3 gravitational force problem requiring students to (a) equate the given force law to weight at Earth's surface (straightforward substitution), and (b) apply conservation of energy with the inverse-square force law. Part (b) involves integrating F = K/x² to find work done, which is a routine M3 technique. While it requires understanding of variable force and energy conservation, it follows a well-established method taught explicitly in M3 courses.
Spec6.02c Work by variable force: using integration6.02d Mechanical energy: KE and PE concepts6.02i Conservation of energy: mechanical energy principle6.06a Variable force: dv/dt or v*dv/dx methods

2. A spacecraft \(S\) of mass \(m\) moves in a straight line towards the centre of the Earth. The Earth is modelled as a sphere of radius \(R\) and \(S\) is modelled as a particle. When \(S\) is at a distance \(x , x \geqslant R\), from the centre of the Earth, the force exerted by the Earth on \(S\) is directed towards the centre of the Earth. The force has magnitude \(\frac { K } { x ^ { 2 } }\), where \(K\) is a constant.
  1. Show that \(K = m g R ^ { 2 }\) (2) When \(S\) is at a distance \(3 R\) from the centre of the Earth, the speed of \(S\) is \(V\). Assuming that air resistance can be ignored,
  2. find, in terms of \(g , R\) and \(V\), the speed of \(S\) as it hits the surface of the Earth.

Question 2(a):
AnswerMarks Guidance
Working/AnswerMarks Guidance
\(x = R \Rightarrow F = mg \therefore mg = \frac{K}{R^2}\)M1 Setting \(F = mg\) and \(x = R\)
\(K = mgR^2\)A1 Deducing the given answer
Total: (2)
Question 2(b):
AnswerMarks Guidance
Working/AnswerMarks Guidance
\(\frac{mgR^2}{x^2} = -mv\frac{dv}{dx}\)M1 Acceleration in form \(v\frac{dv}{dx}\); minus sign may be missing
\(g\int\frac{R^2}{x^2}dx = -\int v\,dv\)
\(-g\frac{R^2}{x} = -\frac{1}{2}v^2\ (+c)\)DM1A1ft Attempting integration; correct integration (ft on missing minus sign)
\(x = 3R,\, v = V \Rightarrow -g\frac{R^2}{3R} = -\frac{1}{2}V^2 + c\)M1 Substituting \(x=3R, v=V\) to obtain equation for \(c\)
\(c = -\frac{Rg}{3} + \frac{1}{2}V^2\)A1 Correct expression for \(c\)
\(x = R \Rightarrow \frac{1}{2}v^2 = -\frac{Rg}{3} + \frac{1}{2}V^2 + \frac{gR^2}{R}\)M1 Substituting \(x = R\) and their expression for \(c\)
\(v^2 = V^2 + \frac{4Rg}{3}\)
\(v = \sqrt{V^2 + \frac{4Rg}{3}}\)A1 cso Correct expression for \(v\), any equivalent form
Total: (7) [9]
## Question 2(a):

| Working/Answer | Marks | Guidance |
|---|---|---|
| $x = R \Rightarrow F = mg \therefore mg = \frac{K}{R^2}$ | M1 | Setting $F = mg$ and $x = R$ |
| $K = mgR^2$ | A1 | Deducing the given answer |

**Total: (2)**

## Question 2(b):

| Working/Answer | Marks | Guidance |
|---|---|---|
| $\frac{mgR^2}{x^2} = -mv\frac{dv}{dx}$ | M1 | Acceleration in form $v\frac{dv}{dx}$; minus sign may be missing |
| $g\int\frac{R^2}{x^2}dx = -\int v\,dv$ | | |
| $-g\frac{R^2}{x} = -\frac{1}{2}v^2\ (+c)$ | DM1A1ft | Attempting integration; correct integration (ft on missing minus sign) |
| $x = 3R,\, v = V \Rightarrow -g\frac{R^2}{3R} = -\frac{1}{2}V^2 + c$ | M1 | Substituting $x=3R, v=V$ to obtain equation for $c$ |
| $c = -\frac{Rg}{3} + \frac{1}{2}V^2$ | A1 | Correct expression for $c$ |
| $x = R \Rightarrow \frac{1}{2}v^2 = -\frac{Rg}{3} + \frac{1}{2}V^2 + \frac{gR^2}{R}$ | M1 | Substituting $x = R$ and their expression for $c$ |
| $v^2 = V^2 + \frac{4Rg}{3}$ | | |
| $v = \sqrt{V^2 + \frac{4Rg}{3}}$ | A1 cso | Correct expression for $v$, any equivalent form |

**Total: (7) [9]**

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2. A spacecraft $S$ of mass $m$ moves in a straight line towards the centre of the Earth. The Earth is modelled as a sphere of radius $R$ and $S$ is modelled as a particle. When $S$ is at a distance $x , x \geqslant R$, from the centre of the Earth, the force exerted by the Earth on $S$ is directed towards the centre of the Earth. The force has magnitude $\frac { K } { x ^ { 2 } }$, where $K$ is a constant.
\begin{enumerate}[label=(\alph*)]
\item Show that $K = m g R ^ { 2 }$\\
(2)

When $S$ is at a distance $3 R$ from the centre of the Earth, the speed of $S$ is $V$. Assuming that air resistance can be ignored,
\item find, in terms of $g , R$ and $V$, the speed of $S$ as it hits the surface of the Earth.
\end{enumerate}

\hfill \mbox{\textit{Edexcel M3 2015 Q2 [9]}}