CAIE IGCSE Physics 6. Space physics Question Bank
Practise space physics through Solar System data, orbit descriptions, light-speed calculations and evidence for stars and galaxies.
- Syllabus
- 2026–2028
- Course
- Physics 0625
Practise space physics through Solar System data, orbit descriptions, light-speed calculations and evidence for stars and galaxies.
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
The Sun is a medium-sized star powered by nuclear fusion reactions which release energy.
State two regions of the electromagnetic spectrum by which the Sun radiates most of its energy.
Any two from:
- infrared
- visible
- ultraviolet
B2
Describe what happens to a star when most of the fuel in its centre has been converted to helium.
(the star) expands
B1
Any one from:
- (smaller star) forms a red giant
- (more massive star) forms a red supergiant
B1
The Milky Way is the galaxy in which the Solar System is located.
State what a galaxy is.
group / collection of (billions of) stars
B1
The Milky Way has a diameter that is approximately equal to 100000 light-years.
Determine this distance in kilometres (km).
9.5×1017( km)
A2
(1 light-year =) 9.5×1015( m) OR (1 light-year =) 3×108×365×24×3600
C1
Astronomers determine the speed and distance from the Earth of a far galaxy that is moving away from the Earth.
State one observation that allows the speed at which a galaxy is moving away to be determined.
increase in wavelength (of light from far galaxy) OR (amount of) redshift
B1
State one different observation that is used to determine the distance to a far galaxy.
brightness of a supernova
B1
State how the speeds of galaxies and their distances from the Earth are related.
(their) speeds are (directly) proportional to distances (from Earth) OR H0=v/d
B1
The best estimate for the Hubble constant H0 is 2.2×10−18 per second.
Use this value to calculate an estimate for the age of the Universe.
> age of the Universe = s [2]
[Total: 8]
4.5×1017( s)
A2
(age of Universe =) 1/H0 OR 1/(2.2×10−18)
C1
What is the approximate diameter of the Milky Way?
100000 kilometres
1000000 kilometres
100000 light-years
1000000 light-years
C