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CIE iGCSE Co-Ordinated Science P6.2.2 Life cycle of stars Exam Style Questions Paper 3

Question

(a) Table 10.1 shows information about the planets in the Solar System.
(i) Identify planet X.
(ii) The mass of the Sun is \( 2 \times 10^{30} \, \text{kg} \).
A student says that the Sun has 100 times the mass of planet X.
Use data from Table 10.1 to show that the student is incorrect.
(b)(i) The Sun is a stable star that formed as a protostar from two materials.
State the two materials from which protostars form.
(b)(ii) The Sun is a small mass star.
Use words or phrases from the list to describe the next stages of the life cycle of the Sun by filling in the gaps in the sequence below.
(c) Visible light travels \( 1.5 \times 10^{11} \, \text{m} \) from the Sun to the Earth at a speed of \( 3.0 \times 10^8 \, \text{m/s} \).
Show that the time for visible light to travel from the Sun to the Earth is approximately 8 minutes.
(d) On Fig. 10.1 complete the ray diagram to show how a lens is able to focus rays of light from the Sun onto some dry grass.

Topic codes (Cambridge IGCSE Co-ordinated Sciences 0654):

• Topic P6.1 — The Solar System
• Topic P6.2.1 — The Sun as a star
• Topic P6.2.2 — Life cycle of stars
• Topic P3.2.3 — Thin converging lens

▶️ Answer/Explanation

(a)(i) Planet X is Jupiter.
From Table 10.1, planet X has a mass of \(2 \times 10^{27}\,\text{kg}\), which closely matches Jupiter’s known mass of approximately \(1.9 \times 10^{27}\,\text{kg}\). Jupiter is the most massive planet in the Solar System, making it the only candidate consistent with the table data.

(a)(ii) The Sun is 1000 times the mass of planet X — the student is incorrect.
\(\dfrac{2 \times 10^{30}}{2 \times 10^{27}} = 10^3 = 1000\). Since the ratio is 1000 and not 100, the student has made an error, likely a mistake with powers of 10. The Sun is therefore ten times more massive relative to planet X than the student claimed.

(b)(i) The two materials are gas and dust.
Protostars form when vast interstellar clouds of gas (mainly hydrogen and helium) and dust are drawn together by gravity. As the cloud collapses, temperature and pressure at the centre rise steadily until nuclear fusion ignites, marking the birth of a stable star.

(b)(ii) Stable star → red giant → planetary nebula + white dwarf.
When the hydrogen fuel in the Sun’s core is exhausted, it will expand and cool into a red giant. The outer layers will then be expelled as a planetary nebula, leaving behind the hot, dense core as a white dwarf that gradually cools over billions of years.

(c) Calculation:
\(\text{time} = \dfrac{\text{distance}}{\text{speed}} = \dfrac{1.5 \times 10^{11}}{3.0 \times 10^{8}} = 500\,\text{s}\)
\(500\,\text{s} \div 60 = 8.3\,\text{minutes} \approx 8\,\text{minutes}\) 
Therefore, the time is approximately 8 minutes.

(d) Parallel rays from the Sun enter the converging lens and refract to meet at the principal focus on the dry grass.
Since the Sun is effectively at infinity, light rays arriving at the lens are parallel to the principal axis. The converging lens bends these rays inward so they all meet at a single focal point, concentrating light energy enough to raise the temperature of the grass and ignite it.

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