Physics 9702/54 — May/June 2025
Cambridge A-Level · Planning, Analysis and Evaluation · worked solutions for every part, with the mark scheme
Topics Analysis, Conclusions and Evaluation · Planning
A ball is dropped on to an inclined thin metal sheet, as shown in Fig. 1.1.
The angle between the sheet and the horizontal bench is . The height of the point of contact of the ball and the sheet is . The horizontal distance travelled by the ball between its points of contact with the sheet and the bench is , as shown in Fig. 1.1.
It is suggested that is related to by the relationship
where is the speed of the ball as it makes contact with the sheet, is the acceleration of free fall, and and are constants.
Plan a laboratory experiment to test the relationship between and .
Draw a diagram showing the arrangement of your equipment.
Explain how the results could be used to determine values for and .
In your plan you should include:
- the procedure to be followed
- the measurements to be taken
- the control of variables
- the analysis of the data
- any safety precautions to be taken.
Diagram
Variables
- Independent variable: .
- Dependent variable: .
- Control variables: (by keeping drop height constant), (keep point of impact fixed in space), same ball, same sheet/surface condition, same release method (no push/spin).
Diagram / arrangement
Procedure and measurements
- Fix a thin metal sheet so it can rotate about a pivot at the chosen impact point (so the impact point stays at constant height above the bench). Adjust the lower end on the bench to set different angles.
- Measure (vertical height of the impact point above the bench) with a metre rule/set square; keep it constant throughout.
- Set up a vertical guide tube (or electromagnet release) directly above the impact point and release the same ball from rest from a fixed height. Measure the vertical drop distance from release point to the impact point; keep constant.
- For a chosen (measure with protractor/inclinometer), release the ball so it strikes the marked point on the sheet.
- Mark the landing point on the bench using paper/carbon paper. Measure the horizontal distance from the vertical line through the impact point to the landing mark using a metre rule.
- Repeat at least 3 times for each and take the mean .
- Repeat for at least 6 different values of over a suitable range (e.g. to ) so that varies substantially.
Analysis (to find and )
Calculate using free-fall:
From
with and constant, plot a graph of (y-axis) against (x-axis).
- Gradient so
- Intercept so
A straight line confirms the suggested relationship (within experimental uncertainty).
Safety
- Prevent the ball from bouncing into walkways: use a catch tray/side barriers and keep the area clear.
- Ensure the sheet and clamp stand are stable/weighted so they cannot tip when struck.
- Keep fingers/feet clear of the landing region; eye protection is advisable.
See working
Background Concept
The suggested relationship is
This has the structure
where
If we can keep and constant while varying , then and are constants and a plot of against should be a straight line.
The speed as the ball reaches the sheet can be made known and constant by dropping it from rest through a fixed vertical height above the impact point. Neglecting air resistance,
Understanding the Question
You are asked to plan an experiment that tests whether depends on according to the given equation, and then to explain how to use the data to find numerical values for the constants and .
So you must:
- vary systematically,
- measure for each ,
- keep other quantities in the equation under control (especially and ),
- choose a graph/analysis that turns the equation into a straight-line form so that gradient and intercept give and .
Approach
- Choose as the independent variable and as the dependent variable.
- Make constant by using the same ball and the same release height above the impact point (a guide tube helps ensure no sideways launch speed).
- Make constant by ensuring the point where the ball hits the sheet stays at the same height above the bench even when the sheet angle changes. The simplest way is to pivot/hinge the sheet about the impact point.
- For each , measure and compute .
- Plot against ; use gradient and intercept to determine and .
Step-by-Step Reasoning
(1) Setting the geometry and keeping constant
A common pitfall is that if you simply raise one end of the sheet, the impact point moves up/down and changes with . That would change the term and destroy the simple linear test.
To avoid this, fix the sheet so it rotates about a pivot located exactly at the chosen impact point. Then, when you change , the impact point stays at the same position in space, so remains constant.
Measure once (vertical height from bench to the impact point). You can use a set square with a metre rule to measure vertical height reliably.
(2) Making known and constant
Release the ball from rest from a fixed vertical height above the impact point. Using a tube ensures the ball falls vertically and hits the same point each time.
Measure and use
Since is fixed, is fixed for all trials.
(3) Measuring reliably
For each :
- measure with a protractor/inclinometer (repeat or check for parallax),
- drop the ball and mark the first contact point on the bench (paper/carbon paper helps),
- measure horizontal distance from the vertical line under the impact point to the landing mark.
Repeat the drop several times at each and take the mean to reduce random effects (slightly different bounces, small changes in impact point, etc.).
(4) Linear graph and extracting and
With and constant, rewrite the equation as
So if you define
you have
with
From the graph:
- Determine the gradient using a large triangle, then calculate
- Read the y-intercept , then calculate
A straight line (within scatter) supports the proposed relationship.
Key Takeaways
- In planning questions, success depends on choosing the correct independent variable and controlling everything else in the given equation.
- To test a relationship efficiently, convert it to a straight-line form and choose a graph where gradient/intercept directly yield the constants.
- A practical plan must include repeat readings, a clear method for measuring each quantity, and explicit control of variables.
Common Mistakes
- Letting change when changing (then the intercept term is not constant and the graph may curve).
- Not stating how is kept constant/known (it is in the equation, so it must be controlled or measured).
- Plotting against instead of (does not linearise the relationship).
- Using too small a range of so hardly changes, giving a very uncertain gradient.
- Not repeating measurements or not stating averaging.
Things to Be Careful About
- Ensure the ball hits the same point on the sheet each time (mark the point and use a guide tube); otherwise and the effective bounce conditions can vary.
- Choose values where varies smoothly and avoids extreme sensitivity near where the slope of changes rapidly.
- Measure horizontally (not along the sheet or along the projectile path) and define the reference line (vertical below impact point) clearly.
- Keep the apparatus stable: an unsecured sheet changes angle on impact, changing during the bounce.
- Record units consistently (e.g. in , and in ) before using the formulas.
A student investigates the relationship between the luminosity of a star and its mass.
The student obtains data of relative luminosity and relative mass for six stars, where
and
It is suggested that and are related by the equation
where and are constants.
A graph is plotted of on the -axis against on the -axis.
Determine expressions for the gradient and -intercept.
gradient = ______
-intercept = ______
Take (\lg) of
So for a graph of (y=\lg\lambda) against (x=\lg\mu):
Answer
Gradient (= n)
(y)-intercept (= \lg k)
gradient = n, y-intercept = lg k
Background Concept
A power law
can be tested using a straight-line graph by taking logarithms (base 10 here). Using log laws:
This converts the power law into the straight-line form
where the gradient (m) and intercept (c) can be read from the graph.
Understanding the Question
You are told the suggested relationship between relative luminosity (\lambda) and relative mass (\mu) is (\lambda = k\mu^n). A graph is plotted of (\lg \lambda) (vertical axis) against (\lg \mu) (horizontal axis). You must state what the gradient and the (y)-intercept represent in terms of (k) and (n).
Approach
- Take (\lg) of both sides of (\lambda = k\mu^n).
- Use log laws to separate into a sum.
- Compare with (y = mx + c) where (y = \lg\lambda) and (x = \lg\mu).
Step-by-Step Reasoning
Start with
Take (\lg) of both sides:
Use (\lg(AB)=\lg A + \lg B) and (\lg(A^n)=n\lg A):
Now identify the straight-line form:
- (y = \lg\lambda)
- (x = \lg\mu)
- gradient (m = n)
- intercept (c = \lg k)
Key Takeaways
- Taking logarithms linearises power laws.
- On a (\lg y) vs (\lg x) plot, the gradient gives the power (n) and the intercept gives (\lg k).
Common Mistakes
- Writing the intercept as (k) instead of (\lg k).
- Forgetting that the plotted variables are (\lg \lambda) and (\lg \mu), not (\lambda) and (\mu).
Things to Be Careful About
- The base of the logarithm matters: (\lg) means base 10, so the intercept corresponds to (\lg k), and later (k) is found using (k = 10^{\text{intercept}}).
Values of and are given in Table 2.1.
Table 2.1
Calculate and record values of and in Table 2.1.
Include the absolute uncertainties in .
For (x=\lg \mu), absolute uncertainty:
Calculated values (3 d.p.):
| (\mu) | (\lambda) | (\lg\mu) | (\Delta(\lg\mu)) | (\lg\lambda) |
|---|---|---|---|---|
| 4.6 (\pm 0.4) | 500 | 0.663 | 0.038 | 2.699 |
| 5.4 (\pm 0.4) | 800 | 0.732 | 0.032 | 2.903 |
| 8.4 (\pm 0.4) | 3200 | 0.924 | 0.021 | 3.505 |
| 11 (\pm 1) | 7000 | 1.041 | 0.039 | 3.845 |
| 16 (\pm 1) | 25000 | 1.204 | 0.027 | 4.398 |
| 18 (\pm 1) | 38000 | 1.255 | 0.024 | 4.580 |
lgμ and lgλ values with Δ(lgμ) as in table
Background Concept
When you transform data using a function (here (\lg)), uncertainties also transform.
For a small uncertainty (\Delta\mu), the uncertainty in (\lg\mu) can be found using differentials:
Since
we have
So
This is why horizontal error bars on a (\lg\mu) axis are based on the fractional uncertainty in (\mu).
Understanding the Question
You are given six values of relative mass (\mu) with uncertainties, and six values of relative luminosity (\lambda) (no uncertainties given). You must:
- compute (\lg\mu) for each star,
- compute (\lg\lambda) for each star,
- and include the absolute uncertainty in (\lg\mu) (so you can later draw error bars in (x)).
Approach
For each row:
- Calculate (\lg\mu) using a calculator.
- Calculate (\lg\lambda).
- Convert (\Delta\mu) to (\Delta(\lg\mu)) using
- Record values to consistent decimal places (typically 3 d.p. for logs here, since the uncertainties are a few (\times 10^{-2})).
Step-by-Step Reasoning
Example (first row): (\mu = 4.6 \pm 0.4).
- Log value:
- Uncertainty:
- For (\lambda=500):
Repeat the same process for each row. Notice that as (\mu) increases, the fractional uncertainty (\Delta\mu/\mu) generally decreases, so (\Delta(\lg\mu)) decreases.
Key Takeaways
- (\lg) values should be recorded consistently (same d.p. across a column).
- For logs, absolute uncertainty depends on fractional uncertainty: (\Delta(\lg\mu)\propto \Delta\mu/\mu).
Common Mistakes
- Using (\Delta(\lg\mu)=\lg(\Delta\mu)) (wrong).
- Forgetting the factor (1/\ln 10) (i.e. using (\Delta\mu/\mu) directly).
- Writing uncertainties to too many decimal places or inconsistent d.p.
Things to Be Careful About
- Use (\ln) (natural log) in the uncertainty formula even though the graph uses (\lg): the conversion factor (1/\ln 10) is essential.
- Keep an appropriate number of significant figures: uncertainties like (0.038) justify giving (\lg\mu) to 3 d.p. rather than 2 d.p.
Plot the points ((x=\lg\mu,, y=\lg\lambda)) (from part (b)):
((0.663,,2.699)), ((0.732,,2.903)), ((0.924,,3.505)), ((1.041,,3.845)), ((1.204,,4.398)), ((1.255,,4.580)).
Add horizontal error bars of (\pm\Delta(\lg\mu)): (\pm0.038,\pm0.032,\pm0.021,\pm0.039,\pm0.027,\pm0.024) respectively.
Answer
Graph of (\lg\lambda) against (\lg\mu) with correct points and (x)-error bars plotted.
Correct plot with x-error bars
Background Concept
To test (\lambda = k\mu^n), we plot
so a straight-line trend supports the power law. Uncertainties in (\mu) become uncertainties in (x=\lg\mu), shown as horizontal error bars of size (\pm\Delta(\lg\mu)).
Understanding the Question
You must place six points on a grid where:
- the horizontal axis is (x=\lg\mu),
- the vertical axis is (y=\lg\lambda),
- and each point has a horizontal error bar only (because only (\mu) has uncertainty).
Approach
- Use the calculated coordinates from part (b).
- Plot each point accurately.
- For each point, draw a horizontal error bar from (x-\Delta x) to (x+\Delta x) where (\Delta x = \Delta(\lg\mu)).
- Ensure axes labels include the correct quantities ((\lg\lambda) and (\lg\mu)).
Step-by-Step Reasoning
The coordinates come directly from the log table. For example, the first star has
- (x = \lg\mu = 0.663)
- (y = \lg\lambda = 2.699)
- (\Delta x = 0.038)
So you plot the point at ((0.663, 2.699)) and draw an error bar from (0.663-0.038) to (0.663+0.038), i.e. from (0.625) to (0.701), at the same height (y=2.699).
Repeat for each of the six points.
Key Takeaways
- A log-log plot turns a power law into a straight line.
- Only draw error bars for quantities that have stated uncertainties.
Common Mistakes
- Plotting (\lambda) against (\mu) instead of logs.
- Drawing vertical error bars for (\lg\lambda) when no uncertainty in (\lambda) is given.
- Misplacing points by reading the axis scale wrongly.
Things to Be Careful About
- Error bars are centred on the plotted (x)-value.
- Use the full resolution of the grid: choose/read values to the nearest small square where possible.
Draw the straight line of best fit and a worst acceptable straight line on your graph. Label both lines.
Draw a straight line of best fit through the plotted points.
Draw a worst acceptable straight line (steepest or shallowest line consistent with all horizontal error bars).
Answer
Both lines drawn and labelled (e.g. “best fit” and “worst acceptable”).
Best-fit line and labelled worst acceptable line drawn
Background Concept
A best-fit line represents the overall trend of the data. When error bars are present, there is a family of lines that could reasonably fit the data; a “worst acceptable” line is an extreme member of this family (either steepest or shallowest) that still passes through all the error bars.
This is used to estimate uncertainty in the gradient and intercept:
Understanding the Question
You have already plotted (\lg\lambda) vs (\lg\mu) with horizontal error bars. Now you must:
- draw one straight line that best represents the trend,
- and another straight line that is still consistent with the error bars but gives an extreme slope.
Approach
- Best fit: balance the scatter (roughly equal number of points above and below, not necessarily passing through every point).
- Worst acceptable: choose either the steepest or shallowest straight line that can still be considered consistent with the data given the error bars.
- Label both lines clearly so you can use them later.
Step-by-Step Reasoning
- Draw the best-fit line through the central trend of the points.
- For the worst acceptable line, imagine “sliding” a ruler to get the maximum or minimum slope while still intersecting the horizontal error bars of all points (it does not have to go through the central dots; passing through the error bars is enough).
Key Takeaways
- “Worst acceptable” means extreme but still consistent with uncertainties.
- Clear labelling prevents confusion when extracting gradients/intercepts.
Common Mistakes
- Drawing the worst line through the points rather than through the error bars.
- Choosing a line that misses one or more error bars (not acceptable).
- Not labelling which line is which.
Things to Be Careful About
- With only horizontal error bars, consistency is judged horizontally: your line should pass within the x-range of each bar at the appropriate y-value.
- Use a long ruler stroke: extend the line across the full graph to make intercept reading more accurate.
Determine the gradient of the line of best fit. Include the absolute uncertainty in your answer.
gradient = ______
Working
Using two points on the best-fit line (widely spaced), e.g.
From worst acceptable line, e.g. (m_{\text{worst}}\approx 3.5).
Answer
(m = 3.2 \pm 0.4)
3.2 ± 0.4
Background Concept
For a straight-line graph, the gradient is
To reduce percentage reading error, you should use two points that are far apart on the drawn line (not necessarily the original data points). When uncertainties are shown by error bars, the uncertainty in the gradient can be estimated by comparing the gradient of the best-fit line with that of a worst acceptable line.
Understanding the Question
You need the gradient of the best-fit line from your log-log plot, and you must give an absolute uncertainty. The uncertainty is found from the difference between the gradients of the best-fit and worst acceptable lines.
Approach
- Choose two well-separated points on the best-fit line and calculate (m_{\text{best}}).
- Choose two well-separated points on the worst acceptable line and calculate (m_{\text{worst}}).
- Take
Step-by-Step Reasoning
- Suppose the best-fit line passes near ((0.66,2.70)) and ((1.26,4.58)).
Then
so
-
Repeat the same process for the worst acceptable line, giving an extreme slope (for example around (3.5) for a steeper line).
-
The absolute uncertainty is the difference:
Key Takeaways
- Use a large triangle on the line to find gradient accurately.
- Uncertainty in gradient comes from comparing best and worst acceptable lines.
Common Mistakes
- Using two data points instead of two points on the drawn best-fit line (more scatter).
- Calculating (\Delta x/\Delta y) instead of (\Delta y/\Delta x).
- Quoting uncertainty as half the range without reference to best vs worst line.
Things to Be Careful About
- Read coordinates carefully from the axes scales.
- Ensure the two points used are far apart (spanning much of the graph width/height) to minimise reading error.
- The uncertainty should be absolute (e.g. (\pm 0.4)), not percentage, unless asked.
Determine the -intercept of the line of best fit. Include the absolute uncertainty in your answer.
-intercept = ______
Working
Using (y = mx + c) with (m_{\text{best}}\approx 3.2) and a point on the best-fit line, e.g. ((x,y)\approx(0.97,3.66)):
From worst acceptable line, e.g. (c_{\text{worst}}\approx 0.2) or (0.9), so
Answer
(y\text{-intercept } = 0.6 \pm 0.4)
0.6 ± 0.4
Background Concept
For a straight line
the (y)-intercept (c) is the value of (y) when (x=0). On a plotted graph, it can be found by extending the best-fit line to cross the (y)-axis, or calculated using a point ((x,y)) on the line:
When uncertainties are present, you compare best-fit and worst acceptable lines to estimate (\Delta c).
Understanding the Question
You must find the (y)-intercept of the best-fit line on the (\lg\lambda) vs (\lg\mu) graph and include an absolute uncertainty using your worst acceptable line.
Approach
- Obtain (c_{\text{best}}) by reading intercept directly or using (c=y-mx).
- Obtain (c_{\text{worst}}) from the worst acceptable line in the same way.
- Take
Step-by-Step Reasoning
- If the best-fit gradient is about (m=3.2) and a point on the best-fit line is around ((0.97,3.66)), then
- If the worst acceptable line gives a noticeably different intercept (for example around (0.2) or (0.9)), then the difference from the best estimate is around (0.4), so
Thus quote (c = 0.6 \pm 0.4).
Key Takeaways
- Intercept can be read from the graph or computed from (c=y-mx).
- Uncertainty comes from comparing best and worst acceptable lines.
Common Mistakes
- Confusing the intercept with (k) (the intercept here is (\lg k), not (k)).
- Using a point that is not actually on the best-fit line.
- Forgetting to include the uncertainty.
Things to Be Careful About
- Extend the drawn line fully to the (y)-axis for a more reliable intercept reading.
- Keep consistency: if you use (c=y-mx) for the best line, do the same for the worst line.
Using your answers to (a), (c)(iii) and (c)(iv), determine the values of and . Include the absolute uncertainties in your values. You need not be concerned with units.
= ______
= ______
From (a):
So
Using (c)(iii) (m = 3.2 \pm 0.4):
Using (c)(iv) (c = 0.6 \pm 0.4):
Uncertainty in (k):
Answer
(k = 4.0 \pm 3.7)
(n = 3.2 \pm 0.4)
k = 4.0 ± 3.7, n = 3.2 ± 0.4
Background Concept
From the linearised relationship
a plot of (y=\lg\lambda) against (x=\lg\mu) has:
- gradient (m = n)
- intercept (c = \lg k)
So (k) is found by antilog:
If (c) has an uncertainty (\Delta c), then for (k = 10^c):
(using differentiation), so
Understanding the Question
You have already found the gradient (with uncertainty) and intercept (with uncertainty) from the best-fit line. You must convert these into values of (n) and (k), again with absolute uncertainties.
Approach
- Set (n) equal to the best-fit gradient, and (\Delta n) equal to the gradient uncertainty.
- Set (c) equal to the intercept (\lg k). Convert to (k) using (10^c).
- Convert (\Delta c) into (\Delta k) using
Step-by-Step Reasoning
- From the graph, suppose
Then
- Since (c = \lg k),
- Uncertainty in (k):
So
(Your numbers may differ slightly depending on your exact graph readings; method is what matters.)
Key Takeaways
- On a log-log plot: gradient gives the exponent (n), intercept gives (\lg k).
- Antilog is needed to get (k).
- Uncertainty propagation through (10^c) uses fractional uncertainty (\ln 10,\Delta c).
Common Mistakes
- Taking (k=c) instead of (k=10^c).
- Using (\Delta k = 10^{\Delta c}) (wrong approach for small uncertainties).
- Forgetting to carry the uncertainties into (k) and (n).
Things to Be Careful About
- The uncertainty in (k) can be large if (\Delta c) is large; quote an absolute uncertainty as requested.
- Keep rounding sensible: do not over-round (c) before taking antilogs, or you can shift (k) noticeably.
The mass of the Sun is . The star Alpha Centauri B has a value of of .
Determine the mass of Alpha Centauri B.
= ______
Using (\lambda = k\mu^n) with (\lambda = 0.46), (k\approx 4.0), (n\approx 3.2):
Mass of Sun (= 2.0\times 10^{30}\ \text{kg}), so
Answer
(M \approx 1.0 \times 10^{30}\ \text{kg})
1.0 × 10^30 kg
Background Concept
Relative mass is defined as
So once you have (\mu), the star’s mass is
The model relating luminosity and mass is
To find (\mu), rearrange:
Understanding the Question
You are told:
- (M_{\odot} = 2.0\times 10^{30}\ \text{kg})
- Alpha Centauri B has (\lambda = 0.46)
- From earlier parts you have constants (k) and (n)
You must calculate the mass (M) of Alpha Centauri B.
Approach
- Use (\lambda = k\mu^n) to solve for (\mu).
- Multiply (\mu) by (M_{\odot}) to get (M) in kg.
Step-by-Step Reasoning
Start with
Rearrange:
Substitute (\lambda=0.46), and your values of (k) and (n) (using best estimates, e.g. (k\approx 4.0), (n\approx 3.2)):
Then convert from relative to actual mass:
Key Takeaways
- Relative quantities convert to absolute quantities by multiplying by the Sun’s value.
- Solving a power law often involves raising to the reciprocal power ((1/n)).
Common Mistakes
- Using (\mu = (\lambda/k)^n) instead of ((\lambda/k)^{1/n}).
- Forgetting to multiply by (2.0\times 10^{30}\ \text{kg}) at the end.
- Mixing up (\lambda) and (\mu).
Things to Be Careful About
- Use the best-estimate values of (k) and (n) (not their logarithms).
- Give the final mass in kg and in standard form, matching the significant figures implied by the data (typically 2 s.f. here).






