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Pearson Edexcel International GCSE (9–1) PHYSICS UNIT: 4PH1 PAPER: 2P QUESTION PAPER+MARK SCHEME JUNE 2025

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Pearson Edexcel International GCSE (9–1) PHYSICS UNIT: 4PH1 PAPER: 2P QUESTION PAPER+MARK SCHEME JUNE 2025

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Pearson Edexcel International GCSE PHYSICS
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Pearson Edexcel International GCSE PHYSICS











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Institution
Pearson Edexcel International GCSE PHYSICS
Course
Pearson Edexcel International GCSE PHYSICS

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October 5, 2025
Number of pages
50
Written in
2025/2026
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Pearson Edexcel International GCSE (9–1) PHYSICS
UNIT: 4PH1 PAPER: 2P QUESTION PAPER+MARK SCHEME
JUNE 2025
Please check the examination details below before entering your candidate information
Candidate surname Other names


Centre Number Candidate Number




Pearson Edexcel International GCSE (9–1)
Monday 16 June 2025
Morning (Time: 1 hour 15 minutes) Paper
reference 4PH1/2P
Physics 🟐 🟐


UNIT: 4PH1
PAPER: 2P

You must have: Total Marks
Ruler, calculator, Equation Booklet (enclosed)



Instructions
•• Use black ink or ball‑point pen.
If pencil is used for diagrams/sketches/graphs it must be dark (HB or B).
• Fill in the
centre boxesand
number at the top of this
candidate page with your name,
number.

•• Answer
Answer all
thequestions.
questions in the spaces provided
– there may be more space than you need.
• Show all the steps in any calculations and state the units.
Information

•• The total mark for this paper is 70.
The marks for each question are shown in brackets
– use this as a guide as to how much time to spend on each question.

Advice

•• Read each question carefully before you start to answer it.
Write your answers neatly and in good English.
•• Try to answer every question.
Check your answers if you have time at the end.


Turn over

,P78955A
©2025 Pearson Education Ltd.
Y:1/1/1/1/1/

,
, FORMULAE

You may find the following formulae useful.




DO NOT WRITE IN THIS AREA
energy transferred = current × voltage × time E = I×V×t

1 1
frequency = f=
time period T
work done W
power = P=
time taken t
energy transferred E
power = P=
time taken t
2π  orbital radius 2πr
orbital speed = v=
time period T

(final speed)2 = (initial speed)2 + (2 × acceleration × distance moved)
v2 = u2 + (2 × a × s)




DO NOT WRITE IN THIS AREA
pressure × volume = constant p1 × V1 = p2 × V2

pressure p1 p2
= constant 
temperature T1 T2

change in momentum (mv  mu)
force = F=
time taken t

change of wavelength velocity of a galaxy λ  λ0 Δ λ v
  
wavelength speed of light λ0 λ0 c

change in thermal energy = mass × specific heat capacity × change in temperature
ΔQ = m × c × ΔT

Where necessary, assume the acceleration of free fall, g = 10 m/ s2. DO NOT WRITE IN THIS AREA




2
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