CAIE IGCSE Physics Solar System Question Bank
Practise classifying Solar System objects, interpreting planetary data, calculating light travel and explaining elliptical-orbit speed through energy transfers.
- Syllabus
- 2026–2028
- Course
- Physics 0625
Practise classifying Solar System objects, interpreting planetary data, calculating light travel and explaining elliptical-orbit speed through energy transfers.
The Solar System includes the Sun and planets.
State two other types of natural object that orbit the Sun.
1
2
any two from:
- minor planets OR dwarf planets
- comets
- asteroids
B2
State the shape of the orbits of the planets.
elliptical
B1
Fig. 10.1 shows the orbit of an object around the Sun. At point A, the object is closest to the Sun. At point B, the object is furthest away from the Sun.

Fig. 10.1
State and explain the energy transfer as the object travels from point A to point B.
statement
explanation
kinetic energy (store) decreases AND potential energy (store) increases (as object moves from A to B)
B1
energy is conserved
B1
Jupiter is 7.8×1011 m from the Sun. The speed of light in a vacuum is 3.0×108 m/s.
Calculate the time taken for light from the Sun to reach Jupiter.
time =
2.6×103 s
A2
v=s/tOR(t=)s/vOR7.8×1011/3.0×108
C1
Jupiter and the Earth are planets in our Solar System.
Describe the composition of Jupiter and the Earth.
Jupiter
the Earth
Jupiter is gaseous
B1
Earth is rocky
B1
The gravitational field strength at the surface of the Earth is approximately 9.8 N/kg. The gravitational field strength at the surface of Jupiter is approximately 23 N/kg.
State one factor which causes the difference between the gravitational field strength at the surface of Jupiter and the gravitational field strength at the surface of the Earth.
mass
B1
State and explain the difference between the orbital speed of Jupiter and the orbital speed of the Earth.
statement
explanation
(orbital speed of) Jupiter is slower ORA
B1
Jupiter is further from the Sun ORA OR orbital speeds of planets decrease as distance from the Sun increases ORA
B1
gravitational field (strength) of Sun decreases with distance (from Sun) ORA
B1