OCR MEI Further Mechanics Major 2021 November — Question 6 11 marks

Exam BoardOCR MEI
ModuleFurther Mechanics Major (Further Mechanics Major)
Year2021
SessionNovember
Marks11
PaperDownload PDF ↗
Mark schemeDownload PDF ↗
TopicDimensional Analysis
TypeDerive dimensions from formula
DifficultyModerate -0.8 This is a straightforward dimensional analysis question with routine steps: recalling F=MLT^-2, rearranging a formula to find dimensions of G, converting units using given conversion factors, checking dimensional consistency (algebraic manipulation), and a final numerical calculation. All parts are standard textbook exercises requiring only methodical application of techniques with no problem-solving insight or novel reasoning.
Spec6.01a Dimensions: M, L, T notation6.01b Units vs dimensions: relationship6.01c Dimensional analysis: error checking6.01d Unknown indices: using dimensions6.01e Formulate models: dimensional arguments

6
  1. Write down the dimensions of force. The force \(F\) of gravitational attraction between two objects with masses \(m _ { 1 }\) and \(m _ { 2 }\), at a distance \(d\) apart, is given by $$F = \frac { G m _ { 1 } m _ { 2 } } { d ^ { 2 } }$$ where \(G\) is the universal gravitational constant.
    In SI units the value of \(G\) is \(6.67 \times 10 ^ { - 11 } \mathrm {~kg} ^ { - 1 } \mathrm {~m} ^ { 3 } \mathrm {~s} ^ { - 2 }\).
  2. Write down the dimensions of \(G\).
  3. Determine the value of \(G\) in imperial units based on pounds, feet, and seconds. Use the facts that 1 pound \(= 0.454 \mathrm {~kg}\) and 1 foot \(= 0.305 \mathrm {~m}\). For a planet of mass \(M\) and radius \(r\), it is suggested that the velocity \(v\) needed for an object to escape the gravitational pull of the planet, the 'escape velocity', is given by the following formula. \(\mathrm { v } = \sqrt { \frac { \mathrm { kGM } } { \mathrm { r } } }\),
    where \(k\) is a dimensionless constant.
  4. Show that this formula is dimensionally consistent. Information regarding the planets Earth and Mars can be found in the table below.
    EarthMars
    Radius (m)63710003389500
    Mass (kg)\(5.97 \times 10 ^ { 24 }\)\(6.39 \times 10 ^ { 23 }\)
    Escape velocity ( \(\mathrm { m } \mathrm { s } ^ { - 1 }\) )11186
  5. Using the formula \(\mathrm { v } = \sqrt { \frac { \mathrm { kGM } } { \mathrm { r } } }\), determine the escape velocity for planet Mars.

Question 6:
AnswerMarks Guidance
6(a) [ F ] = MLT−2
[1]1.2
6(b) [ G ] = M −1 L 3 T −2
[1]Gm m
May use F = 1 2 to obtain the
d 2
dimensions of G
AnswerMarks Guidance
6(c) ( ) 1
G = 6.67 ×10−11 × 0.454 ×
(0.305)3
AnswerMarks
G =1.07×10−9 (lb–1 ft3 s–2)M1
A1
AnswerMarks
[2]3.1a
1.1SC B1 for
G = ( 6.67 ×10−11 ) × 1 ×(0.305)3
0.454
= 4.17×10−12
awrt 1.07×10−9
AnswerMarks Guidance
6(d) ( −1L3T −2 )
 kGM  M M
=
 
 r  L
 kGM 
= LT −1
 
r
 
AnswerMarks
[ v ] = LT−1 so the formula is dimensionally consistentM1
A1
A1
AnswerMarks
[3]2.1
1.1
AnswerMarks
2.2aAttempt to calculate the dimension of
kGM
either or its square root with
r
[ k ] = 1 and two other terms correct
 kGM 
Or = L2T−2
 
 r 
Or allow showing consistency for
kGM
v2 =
r
AnswerMarks Guidance
6(e) ( )( )
k 6.67 ×10−11 5.97 ×1024
11186 =
6 371000
k ≈ 2
( )( )
2 6.67 ×10−11 6.39 ×1023
v =
3 389 500
AnswerMarks
v = 5015 (m s-1)M1
A1
M1
A1
AnswerMarks
[4]3.4
1.1
1.1
AnswerMarks
2.2aAllow to 3 sf or better (allow 5015 to
5017 inclusive)k = 2.0019677...
If using
k = 2.0019677...
expect to see
5017.346122…
Question 6:
6 | (a) | [ F ] = MLT−2 | B1
[1] | 1.2
6 | (b) | [ G ] = M −1 L 3 T −2 | B1
[1] | Gm m
May use F = 1 2 to obtain the
d 2
dimensions of G
6 | (c) | ( ) 1
G = 6.67 ×10−11 × 0.454 ×
(0.305)3
G =1.07×10−9 (lb–1 ft3 s–2) | M1
A1
[2] | 3.1a
1.1 | SC B1 for
G = ( 6.67 ×10−11 ) × 1 ×(0.305)3
0.454
= 4.17×10−12
awrt 1.07×10−9
6 | (d) | ( −1L3T −2 )
 kGM  M M
=
 
 r  L
 kGM 
= LT −1
 
r
 
[ v ] = LT−1 so the formula is dimensionally consistent | M1
A1
A1
[3] | 2.1
1.1
2.2a | Attempt to calculate the dimension of
kGM
either or its square root with
r
[ k ] = 1 and two other terms correct
 kGM 
Or = L2T−2
 
 r 
Or allow showing consistency for
kGM
v2 =
r
6 | (e) | ( )( )
k 6.67 ×10−11 5.97 ×1024
11186 =
6 371000
k ≈ 2
( )( )
2 6.67 ×10−11 6.39 ×1023
v =
3 389 500
v = 5015 (m s-1) | M1
A1
M1
A1
[4] | 3.4
1.1
1.1
2.2a | Allow to 3 sf or better (allow 5015 to
5017 inclusive) | k = 2.0019677...
If using
k = 2.0019677...
expect to see
5017.346122…
6
\begin{enumerate}[label=(\alph*)]
\item Write down the dimensions of force.

The force $F$ of gravitational attraction between two objects with masses $m _ { 1 }$ and $m _ { 2 }$, at a distance $d$ apart, is given by

$$F = \frac { G m _ { 1 } m _ { 2 } } { d ^ { 2 } }$$

where $G$ is the universal gravitational constant.\\
In SI units the value of $G$ is $6.67 \times 10 ^ { - 11 } \mathrm {~kg} ^ { - 1 } \mathrm {~m} ^ { 3 } \mathrm {~s} ^ { - 2 }$.
\item Write down the dimensions of $G$.
\item Determine the value of $G$ in imperial units based on pounds, feet, and seconds.

Use the facts that 1 pound $= 0.454 \mathrm {~kg}$ and 1 foot $= 0.305 \mathrm {~m}$.

For a planet of mass $M$ and radius $r$, it is suggested that the velocity $v$ needed for an object to escape the gravitational pull of the planet, the 'escape velocity', is given by the following formula.\\
$\mathrm { v } = \sqrt { \frac { \mathrm { kGM } } { \mathrm { r } } }$,\\
where $k$ is a dimensionless constant.
\item Show that this formula is dimensionally consistent.

Information regarding the planets Earth and Mars can be found in the table below.

\begin{center}
\begin{tabular}{|l|l|l|}
\hline
 & Earth & Mars \\
\hline
Radius (m) & 6371000 & 3389500 \\
\hline
Mass (kg) & $5.97 \times 10 ^ { 24 }$ & $6.39 \times 10 ^ { 23 }$ \\
\hline
Escape velocity ( $\mathrm { m } \mathrm { s } ^ { - 1 }$ ) & 11186 &  \\
\hline
\end{tabular}
\end{center}
\item Using the formula $\mathrm { v } = \sqrt { \frac { \mathrm { kGM } } { \mathrm { r } } }$, determine the escape velocity for planet Mars.
\end{enumerate}

\hfill \mbox{\textit{OCR MEI Further Mechanics Major 2021 Q6 [11]}}