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CIE iGCSE Co-Ordinated Science P2.3.2 Convection Exam Style Questions Paper 4

Question

(a) The explosion of a supernova forms a nebula. State what may form from this nebula.
(b) (i) Describe how energy is released in a star such as the Sun.
(ii) Energy is released in the core of the Sun. Explain how thermal energy travels, by convection, through the outer gas layers of the surface of the Sun.
(iii) Energy from the Sun travels to Earth by radiation. Satellites in orbit around the Earth can be in direct sunshine for long periods of time. Suggest the colour and texture chosen for the outer surface of a satellite to limit the temperature of the satellite.
(c) Complete the sentences to describe the Big Bang Theory.
The Universe initially expanded from a place of high __________.
The Universe is still expanding.
The Universe is approximately __________ years old.

Most-appropriate topic codes (Cambridge IGCSE Co-ordinated Sciences 0654):

• Topic P6.2.2 — Life cycle of stars (Part (a))
• Topic P6.2.1 — The Sun as a star (Part (b)(i))
• Topic P2.3.2 — Convection (Part (b)(ii))
• Topic P2.3.3 — Radiation (Part (b)(iii))
• Topic P6.2.3 — Galaxies and the Universe (Part (c))

▶️ Answer/Explanation

(a) New stars, planets, or protostars may form from a nebula.
The material from a supernova explosion forms a nebula (cloud of gas and dust), which can collapse under gravity to form new stars and planetary systems.

(b)(i) Energy release in a star:
• Energy is released by nuclear fusion.
• Hydrogen nuclei fuse together to form helium nuclei.
• This process releases vast amounts of energy in the form of electromagnetic radiation (including light and heat).

(b)(ii) Convection in the Sun’s outer layers:
• Hot gas near the core becomes less dense and rises.
• As it rises, it cools and becomes more dense.
• The cooled gas sinks back down, creating convection currents that transfer energy outward.

(b)(iii) Surface design to limit temperature:
• Colour: White or silver (to reflect most incident radiation)
• Texture: Shiny or smooth (to reduce absorption of radiation)

Light colours reflect more radiation (poor absorbers), while shiny surfaces are poor emitters of thermal radiation.

(c) Completed sentences:
The Universe initially expanded from a place of high density (or temperature).
The Universe is still expanding.
The Universe is approximately 13.8 billion years old.

Question

(a) (i) Describe one similarity and two differences between boiling and evaporation.
(ii) State three factors which increase the rate of evaporation.
(b) Fig. 11.1 shows a beaker of water on a tripod and gauze.
The beaker of water is being heated.
Water at the bottom of the beaker is heated by conduction through the glass beaker.
Explain the process of convection which causes all the water in the beaker to increase in temperature.

Topic codes:

• Topic P2.2.2 — Melting, boiling and evaporation (Part (a))
• Topic P2.3.2 — Convection (Part (b))

▶️ Answer/Explanation

(a)(i) Similarity: Both boiling and evaporation are changes of state from liquid to gas.

Difference 1: Boiling occurs at the boiling point, while evaporation occurs below the boiling point.
Difference 2: Boiling occurs throughout the liquid (forms bubbles), while evaporation occurs only at the surface of the liquid.

(a)(ii) Three factors which increase the rate of evaporation:

1. Increased temperature (particles have more kinetic energy, more can escape)
2. Increased surface area (more particles at the surface can escape)
3. Increased air movement over the liquid surface (removes vapour, maintaining a steep concentration gradient)

(b) Convection in the beaker of water:

The heated water at the bottom becomes less dense (as it expands).
This less dense water rises to the top.
The cooler, more dense water sinks to the bottom, where it is heated and the cycle repeats, creating a convection current.
This circulation transfers thermal energy throughout the water, causing all the water in the beaker to increase in temperature.

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