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⚡ Cambridge Challenge Level

These questions feature tricky distractors, multi-step calculations, and subtle distinctions. Scoring A* (≥32) at this level shows genuine mastery. Don't worry if this feels harder — that's the point!

Paper 2 — Multiple Choice

Cambridge IGCSE Physics 0625 • Extended • 40 Questions • 45 Minutes • 40 Marks
Topic 6: Space Physics — Cambridge Challenge
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Section A: The Earth

Questions 1 – 7 • Orbital speed calculations, Earth’s tilt and seasons, sidereal vs synodic periods, satellite orbits, lunar eclipses

Question 1
A geostationary satellite orbits Earth at a radius of 42 200 km from the centre. Its orbital period is exactly 24 hours (86 400 s).

What is its orbital speed?
Question 2
At the December solstice, an observer at Greenwich would notice that the Sun:
Question 3
The Moon’s orbital period is 27.3 days, but the time between successive full Moons is 29.5 days. The difference is because:
Question 4
A satellite in a circular orbit has its orbital radius doubled. How does its orbital speed change?

(Assume the period increases as the radius increases.)
Question 5
During a lunar eclipse observed from the UK, the Moon passes through:
Question 6
If the Earth’s axis had zero tilt (were perpendicular to the orbital plane), what would happen to the seasons?
Question 7
A low-Earth orbit satellite has an orbital speed of 7.8 km/s and a period of 5500 s. What is its orbital radius?

Section B: The Solar System

Questions 8 – 16 • Planetary atmospheres, light travel time, orbital speed comparisons, gravitational field strength, Solar System formation, elliptical orbits

Question 8
A student claims that Venus is hotter than Mercury despite being further from the Sun. Which explanation is correct?
Question 9
Neptune is approximately 4.5 × 1012 m from the Sun. How long does light take to travel from the Sun to Neptune?

(Speed of light c = 3.0 × 108 m/s)
Question 10
The ESA JUICE mission is travelling to Jupiter’s icy moons. Jupiter’s orbital radius is 7.8 × 1011 m and its orbital period is 3.74 × 108 s.

What is Jupiter’s orbital speed around the Sun?
Question 11
Planet X has a surface gravitational field strength of 25 N/kg and Planet Y has 4.0 N/kg. An object weighs 500 N on Planet X.

What does it weigh on Planet Y?
Question 12
In the early Solar System, which process allowed small dust grains to grow into kilometre-sized planetesimals?
Question 13
A planet orbits a star in an elliptical path. At its closest point (perihelion) it is 1.0 × 1011 m from the star and at its farthest point (aphelion) it is 3.0 × 1011 m.

If its speed at perihelion is 45 km/s, which statement about its speed at aphelion is correct?
Question 14
Saturn is approximately 1.4 × 1012 m from the Sun and has an orbital period of 9.3 × 108 s. Mars is 2.3 × 1011 m from the Sun with a period of 5.9 × 107 s.

Which planet has the greater orbital speed?
Question 15
Two asteroids orbit the Sun. Asteroid A is at twice the distance of Asteroid B. Which statement is correct?
Question 16
During the formation of the Solar System, why did the inner planets form as rocky bodies while the outer planets formed as gas giants?

Section C: The Sun as a Star

Questions 17 – 21 • Hydrogen fusion, mass-energy conversion, peak emission wavelength, fusion vs combustion, Sun’s life cycle

Question 17
In the Sun’s core, hydrogen nuclei fuse to form helium. Approximately what percentage of the hydrogen mass is converted to energy in this process?
Question 18
The Sun’s surface temperature is about 5500°C. If you were to measure the peak wavelength of the Sun’s emission, in which part of the electromagnetic spectrum would it fall?
Question 19
A student says “The Sun burns hydrogen like a gas fire.”

Why is this statement incorrect?
Question 20
ESA’s Solar Orbiter mission studies the Sun from close range. Which statement about the Sun’s energy production is correct?
Question 21
The Sun will eventually leave the main sequence. What will happen to it?

Section D: Stars

Questions 22 – 30 • Luminosity and size, main sequence criteria, stellar remnants, light-year conversions, stellar size ordering, stellar lifetimes, supernovae, white dwarf properties

Question 22
Two stars have the same surface temperature. Star P is 100 times more luminous than Star Q.

What can be concluded?
Question 23
A protostar becomes a main sequence star when:
Question 24
Astronomers at Jodrell Bank detect radio signals from a rapidly spinning neutron star (pulsar). This neutron star could NOT have formed from:
Question 25
A galaxy observed by the Royal Astronomical Society is 2.0 × 1022 m away. Express this distance in light-years.

(1 ly = 9.5 × 1015 m)
Question 26
Which sequence correctly orders stellar objects from largest to smallest physical size?
Question 27
A star has a life span of 10 billion years on the main sequence. A star 10 times more massive would have a main sequence lifetime of approximately:
Question 28
During a supernova, elements heavier than iron are created. Why can’t these elements form by normal stellar fusion?
Question 29
The Crab Nebula, observed through the Lovell Telescope at Jodrell Bank, is a supernova remnant about 6500 light-years away.

How far is this in metres? (1 ly = 9.5 × 1015 m)
Question 30
A white dwarf has a mass similar to the Sun but a radius similar to Earth. Compared to the Sun, the white dwarf’s surface gravitational field strength is:

Section E: The Universe

Questions 31 – 40 • Hubble’s law calculations, redshift, cosmic microwave background, age of the Universe, expansion of space, measurement uncertainties

Question 31
Galaxy A is 5.0 × 1024 m away with a recession velocity of 1.1 × 107 m/s. Galaxy B is 2.5 × 1024 m away.

Using Hubble’s law, what is Galaxy B’s recession velocity?
Question 32
A student observes a galaxy whose light has been redshifted so that a spectral line normally at 500 nm appears at 510 nm. This means the galaxy is:
Question 33
The cosmic microwave background radiation is important evidence for the Big Bang because:
Question 34
The Hubble constant is measured as 2.2 × 10−18 s−1.

How old is the Universe in years? (1 year ≈ 3.15 × 107 s)
Question 35
If the Hubble constant were found to be larger than currently estimated, the estimated age of the Universe would:
Question 36
Two galaxies, P and Q, are observed from Earth. P has a redshift 3 times greater than Q. Galaxy Q is 1.5 × 1024 m from Earth.

How far away is Galaxy P?
Question 37
A galaxy is 3.0 × 1024 m away and has a recession velocity of 6.6 × 106 m/s.

How long would it take light to travel from this galaxy to Earth? (1 year ≈ 3.15 × 107 s)
Question 38
The expansion of the Universe means that:
Question 39
A student calculates the age of the Universe using two different galaxies and gets slightly different values of H₀. This is most likely because:
Question 40
If the Universe has been expanding since the Big Bang, and we observe CMBR at a temperature of 2.7 K today, what can we conclude about the Universe at the time the CMBR was emitted?