Edexcel M3 2014 June — Question 2 9 marks

Exam BoardEdexcel
ModuleM3 (Mechanics 3)
Year2014
SessionJune
Marks9
PaperDownload PDF ↗
Mark schemeDownload PDF ↗
TopicAdvanced work-energy problems
TypeInverse-square gravitational force
DifficultyStandard +0.3 Part (a) is straightforward substitution using F=mg at Earth's surface. Part (b) requires energy conservation with inverse-square gravity, which is a standard M3 technique but involves algebraic manipulation of the energy equation. This is a typical textbook-style M3 question with clear structure and standard methods, making it slightly easier than average overall.
Spec6.02d 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 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 magnitude \(\frac { k } { x ^ { 2 } }\), where \(k\) is a constant. 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 \(k = m g R ^ { 2 }\). When \(P\) is at a height \(\frac { R } { 4 }\) above the surface of the Earth, the speed of \(P\) is \(\sqrt { \frac { g R } { 2 } }\) Given that air resistance can be ignored,
  2. find, in terms of \(R\), the greatest distance from the centre of the Earth reached by \(P\).

(a)
AnswerMarks Guidance
(At surface) \(\frac{k}{R^2} = mg \Rightarrow k = mgR^2\)M1A1 (2)
Notes for Question 2(a):
AnswerMarks
M1for \(\frac{k}{R^2} = mg\). If not made clear that this applies at the surface of the Earth award M0 or \(\frac{k}{x^2} = mg\) and \(x = R\)
A1 csofor \(k = mgR^2\) *
(b)
AnswerMarks Guidance
\(m\ddot{x} = -\frac{mgR^2}{x^2}\)
\(v\frac{dv}{dx} = -\frac{gR^2}{x^2}\)M1
\(\int v \frac{dv}{dx} dx = -gR^2 \int \frac{1}{x^2} dx\) or \(\int d\left(\frac{1}{2}v^2\right) dx\)DM1A1
\(\frac{1}{2}v^2 = \frac{gR^2}{x} (+c)\)DM1A1
\(x = \frac{5R}{4}, v = \sqrt{\frac{gR}{2}} \Rightarrow c = -\frac{11gR}{20}\)DM1A1
\(v = 0 \Rightarrow \frac{gR^2}{x} - \frac{11gR}{20}\)DM1
\(x = \frac{20R}{11}\)A1 (7)
[9]
Alternative for Question 2:
Using \(F = \frac{GM_1 M_2}{x^2}\) with \(x = R\) and one mass as mass of Earth:
\(mg = \frac{GmM_E}{R^2}\)
AnswerMarks
\(GM_E = gR^2 \Rightarrow F = \frac{mgR^2}{x^2} \Rightarrow F = \frac{k}{x^2}\) with \(k = mgR^2\) *M1 Complete method A1 Correct answer
By conservation of energy:
AnswerMarks
Work done against gravity \(= \int_R^x \frac{mgR^2}{x^2} dx = \int_x mgR x^{-2} dx\)M1
\(= \frac{4mgR}{5} - \frac{mgR^2}{z}\)DM1(integration)A1(correct)
Work-energy equation: \(\frac{mgR}{4} = \frac{4mgR}{5} - \frac{mgR^2}{z}\)DM1A1
\(z = \frac{20R}{11}\)DM1A1
Notes for Question 2(b):
AnswerMarks
M1for using accel \(= v\frac{dv}{dx}\) oe in NL2 with or w/o m. Minus sign not required.
M1 depfor attempting to integrate both sides - minus not needed
A1for fully correct integration, with or w/o the constant. Must have included the minus sign from the start.
M1 depfor using \(x = \frac{5R}{4}\), \(v = \sqrt{\frac{gR}{2}}\) to obtain a value for the constant. Use of \(x = \frac{R}{4}\) scores M0. Depends on both previous M marks
A1for \(c = -\frac{11gR}{20}\)
M1 depfor setting \(v = 0\) and solving for \(x\). Depends on 1st and 2nd M marks, but not 3rd
A1 csofor \(x = \frac{20R}{11}\)
ALT: By definite integration
First 3 marks as above, then
AnswerMarks
DM1Using limits \(x = \frac{5R}{4}\), \(v = \sqrt{\frac{gR}{2}}\)
DM1Using limit \(v = 0\)
A1Correct substitution
A1 csofor \(x = \frac{20R}{11}\)
NB: The penultimate A mark has changed position, but must be entered on e-pen in its original position.
**(a)**

(At surface) $\frac{k}{R^2} = mg \Rightarrow k = mgR^2$ | M1A1 | (2)

**Notes for Question 2(a):**

M1 | for $\frac{k}{R^2} = mg$. If not made clear that this applies at the surface of the Earth award M0 or $\frac{k}{x^2} = mg$ and $x = R$ |

A1 cso | for $k = mgR^2$ * |

**(b)**

$m\ddot{x} = -\frac{mgR^2}{x^2}$ |  |

$v\frac{dv}{dx} = -\frac{gR^2}{x^2}$ | M1 |

$\int v \frac{dv}{dx} dx = -gR^2 \int \frac{1}{x^2} dx$ or $\int d\left(\frac{1}{2}v^2\right) dx$ | DM1A1 |

$\frac{1}{2}v^2 = \frac{gR^2}{x} (+c)$ | DM1A1 |

$x = \frac{5R}{4}, v = \sqrt{\frac{gR}{2}} \Rightarrow c = -\frac{11gR}{20}$ | DM1A1 |

$v = 0 \Rightarrow \frac{gR^2}{x} - \frac{11gR}{20}$ | DM1 |

$x = \frac{20R}{11}$ | A1 | (7)

[9]

**Alternative for Question 2:**

Using $F = \frac{GM_1 M_2}{x^2}$ with $x = R$ and one mass as mass of Earth:

$mg = \frac{GmM_E}{R^2}$

$GM_E = gR^2 \Rightarrow F = \frac{mgR^2}{x^2} \Rightarrow F = \frac{k}{x^2}$ with $k = mgR^2$ * | M1 Complete method A1 Correct answer |

By conservation of energy:

Work done against gravity $= \int_R^x \frac{mgR^2}{x^2} dx = \int_x mgR x^{-2} dx$ | M1 |

$= \frac{4mgR}{5} - \frac{mgR^2}{z}$ | DM1(integration)A1(correct) |

Work-energy equation: $\frac{mgR}{4} = \frac{4mgR}{5} - \frac{mgR^2}{z}$ | DM1A1 |

$z = \frac{20R}{11}$ | DM1A1 |

**Notes for Question 2(b):**

M1 | for using accel $= v\frac{dv}{dx}$ oe in NL2 with or w/o m. Minus sign not required. |

M1 dep | for attempting to integrate both sides - minus not needed |

A1 | for fully correct integration, with or w/o the constant. Must have included the minus sign from the start. |

M1 dep | for using $x = \frac{5R}{4}$, $v = \sqrt{\frac{gR}{2}}$ to obtain a value for the constant. Use of $x = \frac{R}{4}$ scores M0. Depends on both previous M marks |

A1 | for $c = -\frac{11gR}{20}$ |

M1 dep | for setting $v = 0$ and solving for $x$. Depends on 1st and 2nd M marks, but not 3rd |

A1 cso | for $x = \frac{20R}{11}$ |

**ALT:** By definite integration
First 3 marks as above, then

DM1 | Using limits $x = \frac{5R}{4}$, $v = \sqrt{\frac{gR}{2}}$ |

DM1 | Using limit $v = 0$ |
A1 | Correct substitution |

A1 cso | for $x = \frac{20R}{11}$ |

NB: The penultimate A mark has changed position, but must be entered on e-pen in its original position.

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2. 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 magnitude $\frac { k } { x ^ { 2 } }$, where $k$ is a constant.

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 $k = m g R ^ { 2 }$.

When $P$ is at a height $\frac { R } { 4 }$ above the surface of the Earth, the speed of $P$ is $\sqrt { \frac { g R } { 2 } }$ Given that air resistance can be ignored,
\item find, in terms of $R$, the greatest distance from the centre of the Earth reached by $P$.
\end{enumerate}

\hfill \mbox{\textit{Edexcel M3 2014 Q2 [9]}}