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Paper 2 — Multiple Choice

Cambridge IGCSE Physics 0625 • 40 Questions • 45 Minutes • 40 Marks
Topic 6: Space Physics — Mock 2
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Section A — 6.1.1 The Earth

Questions 1–7 • Rotation, seasons, Moon phases, orbital speed (v = 2πr/T)

Question 1
The Earth rotates on its axis once every 24 hours. In which direction does it rotate when viewed from above the North Pole?
Question 2
Seasons on Earth are caused by:
Question 3
A full Moon occurs when:
Question 4
The International Space Station (ISS), where Tim Peake conducted experiments, orbits at a radius of 6800 km from Earth's centre with a period of 5500 s. Calculate its orbital speed using v = 2πr/T.
Question 5
At the June solstice, the North Pole is tilted towards the Sun. What does this mean for the UK?
Question 6
During a first quarter Moon, approximately what fraction of the Moon's visible face is illuminated?
Question 7
A comet orbits the Sun with an orbital radius of 6.0 × 1012 m and a period of 9.5 × 108 s. What is its average orbital speed?

Section B — 6.1.2 The Solar System

Questions 8–16 • Planets, orbits, gravity, formation of the Solar System

Question 8
Which planet is the largest in the Solar System?
Question 9
The outer planets (Jupiter, Saturn, Uranus, Neptune) are called gas giants or ice giants. Which characteristic do they share?
Question 10
Mars is approximately 2.3 × 1011 m from the Sun. How long does it take light from the Sun to reach Mars?
Question 11
In the accretion model of Solar System formation, what role does gravity play?
Question 12
ESA's Rosetta mission studied Comet 67P. Why do comets speed up as they approach the Sun?
Question 13
A student at a Scottish Dark Sky Observatory measures the gravitational field strength on Earth's surface as 9.8 N/kg. On the Moon, g = 1.6 N/kg. A telescope weighing 49 N on Earth would weigh approximately what on the Moon?
Question 14
Which statement about planetary orbits is correct?
Question 15
Neptune is the most distant planet from the Sun. What can be said about its orbital period compared to Mercury's?
Question 16
The gravitational field strength at the surface of a planet depends on:

Section C — 6.2.1 The Sun as a Star

Questions 17–21 • Nuclear fusion, the Sun's classification, electromagnetic radiation

Question 17
The Sun produces energy by:
Question 18
Which statement about the Sun is correct?
Question 19
The Sun emits ultraviolet radiation. What is one effect of this on Earth?
Question 20
Nuclear fusion in the Sun requires extremely high temperatures because:
Question 21
Compared to the visible light it emits, the infrared radiation from the Sun has:

Section D — 6.2.2 Stars

Questions 22–30 • Stellar evolution, life cycles, light-years, the Milky Way

Question 22
Stars are born in:
Question 23
During the main sequence stage, a star is stable because:
Question 24
The Milky Way is best described as a:
Question 25
A star is 1.9 × 1017 m from Earth. Express this distance in light-years. (1 ly = 9.5 × 1015 m)
Question 26
After the red giant phase, a star with a mass similar to the Sun will:
Question 27
A supernova is:
Question 28
Which statement about neutron stars is correct?
Question 29
Light from a distant star observed at the Cambridge Institute of Astronomy takes 50 years to reach Earth. How far away is the star in metres? (1 ly = 9.5 × 1015 m)
Question 30
A black hole is formed when:

Section E — 6.2.3 The Universe

Questions 31–40 • Redshift, Hubble's law (v = H₀d), CMBR, Big Bang, age of the Universe

Question 31
The diameter of the Milky Way is approximately:
Question 32
Redshift in the light from a distant galaxy indicates that:
Question 33
Hubble's law states that:
Question 34
CMBR was first detected in 1965 by Penzias and Wilson. What temperature does this radiation correspond to?
Question 35
If the Hubble constant H₀ = 2.2 × 10−18 s−1, the estimated age of the Universe in seconds is:
Question 36
A galaxy has a recession velocity of 3.3 × 106 m/s. Using H₀ = 2.2 × 10−18 s−1, how far away is it?
Question 37
The Big Bang theory is supported by the observation that:
Question 38
Galaxy X has a recession velocity of 4.4 × 105 m/s and Galaxy Y has a recession velocity of 8.8 × 105 m/s. According to Hubble's law:
Question 39
If the Universe is expanding, what was it like in the distant past?
Question 40
A galaxy at a distance of 4.5 × 1024 m shows a recession velocity of 9.9 × 106 m/s. Calculate H₀.