Edexcel M3 2016 June — Question 4 9 marks

Exam BoardEdexcel
ModuleM3 (Mechanics 3)
Year2016
SessionJune
Marks9
PaperDownload PDF ↗
Mark schemeDownload PDF ↗
TopicVariable Force
TypeInverse power force - gravitational/escape velocity context
DifficultyStandard +0.8 Part (a) is a straightforward 2-mark 'show that' using proportionality and boundary conditions. Part (b) requires setting up and integrating F=ma with variable force (inverse square law), applying energy methods or chain rule integration v dv/dx, and careful algebraic manipulation with the given maximum height condition. This is a standard M3 variable force question but requires multiple sophisticated steps beyond typical A-level, making it moderately challenging.
Spec6.02i Conservation of energy: mechanical energy principle6.06a Variable force: dv/dt or v*dv/dx methods

A particle \(P\) of mass \(m\) is fired vertically upwards from a point on the surface of the Earth and initially moves in a straight line directly away from the centre of the Earth. When \(P\) is at a distance \(x\) from the centre of the Earth, the gravitational force exerted by the Earth on \(P\) is directed towards the centre of the Earth and has a magnitude which is inversely proportional to \(x^2\). At the surface of the Earth the acceleration due to gravity is \(g\). The Earth is modelled as a fixed sphere of radius \(R\).
  1. Show that the magnitude of the gravitational force acting on \(P\) is \(\frac{mgR^2}{x^2}\) [2]
The particle was fired with initial speed \(U\) and the greatest height above the surface of the Earth reached by \(P\) is \(\frac{R}{20}\). Given that air resistance can be ignored,
  1. find \(U\) in terms of \(g\) and \(R\). [7]

Part (a)
AnswerMarks Guidance
Answer/WorkingMarks Guidance
\(F = (-)\frac{k}{x^2}\)
\(x = R\) \(F = (-)mg\)
\(mg = (-){\frac{k}{R^2}}\)M1 Using NL2 at the surface of the Earth with the proportionality condition, force to be \(mg\). distance to be \(R\). Can use \(F = \frac{GMm}{x^2}\)
Mag of \(F = \frac{mgR^2}{x^2}\) *A1cso (2) Find the constant of proportionality and hence deduce the stated magnitude.
Part (b)
AnswerMarks Guidance
Answer/WorkingMarks Guidance
\((m)v\frac{dv}{dx} = -(m)\frac{gR^2}{x^2}\)M1 Using NL2 with acceleration in form \(v\frac{dv}{dx}\). Minus sign may be missing. \(m\) may be cancelled.
\(\int vdv = -\int gR^2 x^{-2}dx\)DM1A1ft Attempt integration of their expression. \(v^2\) or \(x^{-1}\) must be seen. Correct integration follow through a missing minus sign. Constant of integration may be missing.
\(\frac{1}{2}v^2 = gR^2 x^{-1} + (c)\)
\(x = R\) \(v = U\) \(\frac{1}{2}U^2 = gR + c\)M1
\(\frac{1}{2}v^2 = \frac{gR^2}{x} + \frac{1}{2}U^2 - gR\) oeA1
\(x = \frac{21}{20}R\) \(v = 0\) \(0 = \frac{gR^2}{\frac{21}{20}R} + \frac{1}{2}U^2 - gR\)M1 Using \(x = R\) \(v = U\) OR substitute \(x = \frac{21}{20}R\) \(v = 0\) in an equation containing \(c\)
\(\frac{1}{2}U^2 = gR - \frac{20}{21}gR\)
\(U = \sqrt{\frac{2gR}{21}}\) oeA1 (7)
Total: [9]
Key Notes:
- (a)M1: Using NL2 at the surface of the Earth with the proportionality condition, force to be \(mg\), distance to be \(R\). Can use \(F = \frac{GMm}{x^2}\)
- (a)A1cso: Find the constant of proportionality and hence deduce the stated magnitude.
- (b)M1: Using NL2 with acceleration in form \(v\frac{dv}{dx}\). Minus sign may be missing. \(m\) may be cancelled.
- (b)DM1: Attempt integration of their expression. \(v^2\) or \(x^{-1}\) must be seen.
- (b)A1ft: Correct integration follow through a missing minus sign. Constant of integration may be missing.
- (b)M1: Using \(x = R\) \(v = U\) OR substitute \(x = \frac{21}{20}R\) \(v = 0\) in an equation containing \(c\)
- (b)A1: Substituting a correct constant to obtain a correct expression for \(\frac{1}{2}v^2\)
- (b)M1: Substitute \(x = \frac{21}{20}R\) \(v = 0\) OR substitute \(x = R\) \(v = U\)
- (b)A1: Complete to a correct expression for \(U\).
Definite integration in (b):
AnswerMarks Guidance
Answer/WorkingMarks Guidance
\((m)v\frac{dv}{dx} = -(m)\frac{gR^2}{x^2}\)M1
\(\int_U^0 vdv = -\int_R^{\frac{21R}{20}} gR^2 x^{-2}dx\)
\(\left[\frac{1}{2}v^2\right] = \left[gR^2 x^{-1}\right]\)DM1A1ft (ft missing sign, as main scheme) Limits not needed
\(\left[\frac{1}{2}v^2\right]_U^0 = \left[gR^2 x^{-1}\right]_R^{\frac{21R}{20}}\)M1 limits seen, correct "values" but may be paired incorrectly
A1correct limits, \(0\) and \(\frac{21R}{20}\) at top or bottom on both integrals, \(U\) and \(R\) in the other positions
M1Substitute their limits A1
NB: It is possible to appear to omit the minus sign and reverse the limits on one integral. However, without some explanation this will be insufficient working and scores as a missing minus case.
### Part (a)

| Answer/Working | Marks | Guidance |
|---|---|---|
| $F = (-)\frac{k}{x^2}$ | | |
| $x = R$ $F = (-)mg$ | | |
| $mg = (-){\frac{k}{R^2}}$ | M1 | Using NL2 at the surface of the Earth with the proportionality condition, force to be $mg$. distance to be $R$. Can use $F = \frac{GMm}{x^2}$ |
| Mag of $F = \frac{mgR^2}{x^2}$ * | A1cso | (2) Find the constant of proportionality and hence deduce the stated magnitude. |

### Part (b)

| Answer/Working | Marks | Guidance |
|---|---|---|
| $(m)v\frac{dv}{dx} = -(m)\frac{gR^2}{x^2}$ | M1 | Using NL2 with acceleration in form $v\frac{dv}{dx}$. Minus sign may be missing. $m$ may be cancelled. |
| $\int vdv = -\int gR^2 x^{-2}dx$ | DM1A1ft | Attempt integration of their expression. $v^2$ or $x^{-1}$ must be seen. Correct integration follow through a missing minus sign. Constant of integration may be missing. |
| $\frac{1}{2}v^2 = gR^2 x^{-1} + (c)$ | | |
| $x = R$ $v = U$ $\frac{1}{2}U^2 = gR + c$ | M1 | |
| $\frac{1}{2}v^2 = \frac{gR^2}{x} + \frac{1}{2}U^2 - gR$ oe | A1 | |
| $x = \frac{21}{20}R$ $v = 0$ $0 = \frac{gR^2}{\frac{21}{20}R} + \frac{1}{2}U^2 - gR$ | M1 | Using $x = R$ $v = U$ OR substitute $x = \frac{21}{20}R$ $v = 0$ in an equation containing $c$ |
| $\frac{1}{2}U^2 = gR - \frac{20}{21}gR$ | | |
| $U = \sqrt{\frac{2gR}{21}}$ oe | A1 | (7) |

**Total: [9]**

**Key Notes:**
- (a)M1: Using NL2 at the surface of the Earth with the proportionality condition, force to be $mg$, distance to be $R$. Can use $F = \frac{GMm}{x^2}$
- (a)A1cso: Find the constant of proportionality and hence deduce the stated magnitude.
- (b)M1: Using NL2 with acceleration in form $v\frac{dv}{dx}$. Minus sign may be missing. $m$ may be cancelled.
- (b)DM1: Attempt integration of their expression. $v^2$ or $x^{-1}$ must be seen.
- (b)A1ft: Correct integration follow through a missing minus sign. Constant of integration may be missing.
- (b)M1: Using $x = R$ $v = U$ OR substitute $x = \frac{21}{20}R$ $v = 0$ in an equation containing $c$
- (b)A1: Substituting a correct constant to obtain a correct expression for $\frac{1}{2}v^2$
- (b)M1: Substitute $x = \frac{21}{20}R$ $v = 0$ OR substitute $x = R$ $v = U$
- (b)A1: Complete to a correct expression for $U$.

**Definite integration in (b):**

| Answer/Working | Marks | Guidance |
|---|---|---|
| $(m)v\frac{dv}{dx} = -(m)\frac{gR^2}{x^2}$ | M1 | |
| $\int_U^0 vdv = -\int_R^{\frac{21R}{20}} gR^2 x^{-2}dx$ | | |
| $\left[\frac{1}{2}v^2\right] = \left[gR^2 x^{-1}\right]$ | DM1A1ft | (ft missing sign, as main scheme) Limits not needed |
| $\left[\frac{1}{2}v^2\right]_U^0 = \left[gR^2 x^{-1}\right]_R^{\frac{21R}{20}}$ | M1 | limits seen, correct "values" but may be paired incorrectly |
| | A1 | correct limits, $0$ and $\frac{21R}{20}$ at top or bottom on both integrals, $U$ and $R$ in the other positions |
| M1 | Substitute their limits | A1 | correct answer. |

**NB:** It is possible to appear to omit the minus sign and reverse the limits on one integral. However, without some explanation this will be insufficient working and scores as a missing minus case.

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A particle $P$ of mass $m$ is fired vertically upwards from a point on the surface of the Earth and initially moves in a straight line directly away from the centre of the Earth. When $P$ is at a distance $x$ from the centre of the Earth, the gravitational force exerted by the Earth on $P$ is directed towards the centre of the Earth and has a magnitude which is inversely proportional to $x^2$. At the surface of the Earth the acceleration due to gravity is $g$. The Earth is modelled as a fixed sphere of radius $R$.

\begin{enumerate}[label=(\alph*)]
\item Show that the magnitude of the gravitational force acting on $P$ is $\frac{mgR^2}{x^2}$ [2]
\end{enumerate}

The particle was fired with initial speed $U$ and the greatest height above the surface of the Earth reached by $P$ is $\frac{R}{20}$.

Given that air resistance can be ignored,

\begin{enumerate}[label=(\alph*)]
\setcounter{enumi}{1}
\item find $U$ in terms of $g$ and $R$. [7]
\end{enumerate}

\hfill \mbox{\textit{Edexcel M3 2016 Q4 [9]}}