School13 min read

Physics Numericals Practice with Step-by-Step Solutions

By the QUFF Team

Most students who struggle with physics numericals do not have a concept problem - they have a process problem. They read the question, hunt for a formula that contains the given symbols, and substitute. That works until the numbers get awkward and then it fails silently. This set works the other way: a fixed four-step method, then solved numericals across the major chapters, each with the reasoning made explicit. The units and sign conventions get their own section, because that is where marks actually disappear.

An atom diagram, a molecule model, a compass and a stack of books with a graduation cap, representing physics problem practice

The four-step method

Every numerical, at every level, yields to the same sequence. Write it out fully even when the problem looks easy - the habit is what saves you when the problem is not.

  • Step 1 - List what is given, with units, and what is asked. Convert everything to SI now.
  • Step 2 - Name the concept, not the formula. 'This is conservation of energy' or 'this is a series circuit' narrows the formula choice to one or two.
  • Step 3 - Write the formula symbolically, then rearrange for the unknown before substituting numbers. Rearranging with numbers in place is where algebra errors creep in.
  • Step 4 - Substitute with units, compute, and sanity-check the magnitude and sign. A car accelerating at 400 m/s² is a wrong answer regardless of the arithmetic.

Kinematics and Newton's laws

A car starting from rest reaches 20 m/s in 5 s. Find its acceleration and the distance covered.

Given u = 0, v = 20 m/s, t = 5 s. From v = u + at, a = 20/5 = 4 m/s². Then s = ut + ½at² = 0 + ½ × 4 × 25 = 50 m. You could also use s = (u+v)t/2 = 10 × 5 = 50 m as a check.

A force of 10 N acts on a 5 kg body at rest on a frictionless surface. Find the acceleration and the velocity after 3 s.

From F = ma, a = 10/5 = 2 m/s². Then v = u + at = 0 + 2 × 3 = 6 m/s. Note that Newton's second law gives acceleration, never velocity directly - a step students often skip.

A ball is projected at 20 m/s at 30° to the horizontal. Find its maximum height and horizontal range (g = 10 m/s²).

H = u²sin²θ/2g = 400 × 0.25 / 20 = 5 m. R = u²sin2θ/g = 400 × sin60° / 10 = 400 × 0.866 / 10 ≈ 34.6 m. Note that sin2θ uses the doubled angle - substituting sinθ here is the standard error.

A 2 kg body moving at 5 m/s is brought to rest in 4 s. Find the retarding force.

a = (v − u)/t = (0 − 5)/4 = −1.25 m/s², so F = ma = 2 × (−1.25) = −2.5 N. The negative sign means the force opposes the motion, and stating that is worth a mark.

Work, energy, power and circular motion

A force of 10 N moves a body 5 m along a direction at 60° to the force. Find the work done.

W = Fs cosθ = 10 × 5 × cos60° = 10 × 5 × 0.5 = 25 J. Only the component of force along the displacement does work, which is why a force perpendicular to motion - like the centripetal force in uniform circular motion - does none.

Find the kinetic energy of a 2 kg body moving at 10 m/s, and the work needed to double its speed.

KE = ½mv² = ½ × 2 × 100 = 100 J. Doubling the speed quadruples the kinetic energy to 400 J, so the extra work required is 300 J. Kinetic energy scales with the square of speed - the source of many wrong intuitions.

A body of mass 1 kg falls freely from a height of 20 m. Find its speed on reaching the ground (g = 10 m/s²).

By conservation of energy, mgh = ½mv², so v = √(2gh) = √400 = 20 m/s. The mass cancels, which is why all bodies fall alike in the absence of air resistance.

A stone moves in a circle of radius 5 m at 10 m/s. Find its centripetal acceleration.

a_c = v²/r = 100/5 = 20 m/s², directed towards the centre. The speed may be constant while the velocity is not, since the direction keeps changing - which is precisely why there is an acceleration at all.

A pump raises 100 kg of water through 10 m in 20 s. Find its power output (g = 10 m/s²).

Work = mgh = 100 × 10 × 10 = 10,000 J, so power = W/t = 10,000/20 = 500 W. Power is always work divided by time, and mixing up the two is a common one-mark loss.

Electricity

Three resistors of 2 Ω, 3 Ω and 6 Ω are connected in parallel across a 6 V battery. Find the equivalent resistance and total current.

1/R = 1/2 + 1/3 + 1/6 = (3 + 2 + 1)/6 = 1, so R = 1 Ω. Then I = V/R = 6/1 = 6 A. Sanity check: the parallel equivalent must be smaller than the smallest resistor, and 1 Ω is.

A wire of resistance 4 Ω is stretched to twice its original length. Find its new resistance.

16 Ω. Volume is conserved, so doubling the length halves the area, and R = ρl/A therefore increases by a factor of 2 × 2 = 4. Stretching questions always turn on this simultaneous change in both l and A.

An electric heater draws 5 A from a 220 V supply. Find its power and the energy consumed in 2 hours.

P = VI = 220 × 5 = 1100 W = 1.1 kW. Energy = 1.1 × 2 = 2.2 kWh, or 2.2 units. Convert watts to kilowatts before multiplying by hours, or the unit count comes out a thousand times too large.

Find the heat produced when a current of 2 A flows through a 5 Ω resistor for 30 s.

H = I²Rt = 4 × 5 × 30 = 600 J. Note that heat depends on the square of the current, which is why a small increase in current causes a disproportionate rise in heating - the basis of both fuses and transmission losses.

Optics: get the signs right first

Optics numericals are the most mechanical in physics and the most error-prone, for one reason: the sign convention. Fix it before you write the formula. Distances are measured from the pole or optical centre, positive along the direction of incident light and negative against it - so a real object always has a negative u.

An object is placed 20 cm from a concave mirror of focal length 15 cm. Find the image distance and magnification.

With u = −20 cm and f = −15 cm: 1/v = 1/f − 1/u = −1/15 + 1/20 = (−4 + 3)/60 = −1/60, so v = −60 cm - a real image 60 cm in front. m = −v/u = −(−60)/(−20) = −3: inverted and three times larger.

A concave lens of focal length 20 cm has an object 30 cm away. Find the image position.

With u = −30 cm and f = −20 cm: 1/v = 1/f + 1/u = −1/20 − 1/30 = (−3 − 2)/60 = −1/12, so v = −12 cm. A concave lens always forms a virtual, diminished image on the same side as the object, whatever the object distance - a useful check on your answer.

Two lenses of power +3 D and −5 D are placed in contact. Find the power and focal length of the combination.

Powers in contact simply add: P = 3 + (−5) = −2 D. Then f = 1/P = −0.5 m = −50 cm, so the combination behaves as a diverging lens.

Light passes from air into glass of refractive index 1.5 at an angle of incidence of 30°. Find the angle of refraction.

From Snell's law, sin r = sin i / n = 0.5/1.5 = 0.333, so r ≈ 19.5°. The ray bends towards the normal on entering a denser medium, which the smaller angle confirms.

Modern physics

The work function of a metal is 2 eV. Light of energy 5 eV falls on it. Find the maximum kinetic energy of the emitted photoelectrons.

By Einstein's photoelectric equation, KE_max = hν − φ = 5 − 2 = 3 eV. Photons below the work function eject no electrons regardless of how intense the light is - the observation that established the particle nature of light.

Find the energy of an electron in the second orbit of a hydrogen atom.

E_n = −13.6/n² eV, so E₂ = −13.6/4 = −3.4 eV. The negative sign indicates a bound state, and its magnitude is the energy needed to remove the electron from that orbit.

A radioactive sample has a half-life of 10 days. What fraction remains after 40 days?

1/16. Forty days is four half-lives, and each halves the remaining quantity: 1/2, 1/4, 1/8, 1/16. Count half-lives rather than reaching for the exponential formula when the time is a whole multiple.

Where the marks actually go

  • Unit conversion done late or not at all - km/h left unconverted, centimetres in a formula expecting metres, grams where kilograms belong.
  • Sign convention errors in optics, which flip the nature of the image and lose every subsequent mark.
  • Substituting before rearranging, which turns a clean algebra step into an arithmetic mess.
  • Not writing the formula. Marking schemes usually award a separate mark for it, so a correct formula with a wrong final answer still scores.
  • Skipping the sanity check. Physically absurd magnitudes are the cheapest errors to catch and the most embarrassing to leave.
  • Practising untimed, so speed never develops. Solve in sets against a clock once the method is secure.

The bottom line

Now go test yourself

Physics numericals become reliable when the process becomes automatic: givens with units, name the concept, formula symbolically, substitute and sanity-check. Almost every mark lost in this subject goes to a unit left unconverted, a sign convention assumed rather than fixed, or an answer never checked against physical sense - and all three are process failures, not knowledge failures.

So drill the process, not just the problems. Work these solutions with the page covered, then move to timed physics quizzes on QUFF and read the explanation on every miss to see which step of the four broke down.

FAQs

Frequently asked questions

How do I get better at physics numericals?

Use one fixed process every time: list givens with units, name the concept, write the formula symbolically and rearrange, then substitute and sanity-check. Most difficulty comes from formula-hunting rather than from weak concepts.

Why do I keep getting optics numericals wrong?

Almost always the sign convention. Fix it before substituting - distances against the direction of incident light are negative, so a real object has a negative u. A single sign error propagates through the whole answer.

Should I memorise physics formulas or derive them?

Memorise the standard set for instant recall, since the clock is unforgiving, but understand each derivation well enough to reconstruct it. Recall gets you started; understanding tells you whether the formula applies to this situation.

How many numericals should I practise a day?

Ten to fifteen worked properly beats fifty rushed. Write every step, and after finishing check which step failed on each miss - that diagnosis is where the improvement comes from.

Why does resistance increase when a wire is stretched?

Because volume is conserved, so increasing the length reduces the cross-sectional area proportionally. Since R = ρl/A, doubling the length quadruples the resistance - both factors change at once.

What is the most common mistake in projectile motion questions?

Using sinθ instead of sin2θ in the range formula, R = u²sin2θ/g. Maximum height uses sin²θ and range uses sin2θ, and confusing the two is the standard error.

How do I check whether my numerical answer is reasonable?

Compare the magnitude with everyday physical values and check the sign against expectation. An acceleration of hundreds of metres per second squared for a car, or a real image behind a concave lens, means something went wrong regardless of the arithmetic.

Where can I practise physics questions online for free?

QUFF has free adaptive physics quizzes with no sign-up, covering both conceptual and numerical questions with an explanation on every answer - useful for finding which step of your method is failing.

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