Study Guide

Unit Overview

Space Physics

CIE IGCSE Physics· 5 min read 📊 5-7% of total exam marks across MCQ and theory papers

1. Unit at a glance

We start with concrete, observable astronomical phenomena on our local scale, including day/night cycles, seasonal variation, and the structure of our solar system, before moving outwards to explore the life cycle of stars and cosmological models of the universe.

The learning sequence builds steadily from familiar real-world observations to more abstract physics principles, helping you connect everyday experiences to large-scale universal rules.

2. Common Pitfalls

Wrong move:

Confusing the cause of seasons with Earth's distance from the Sun

Why:

Seasons are caused by the 23.5° tilt of Earth's axis, not varying orbital distance from the Sun

Correct move:

Always link seasonal temperature changes to axial tilt affecting the angle and duration of incoming solar radiation

Wrong move:

Assuming all stars follow the same life cycle regardless of initial mass

Why:

High-mass stars end their lives in supernova explosions forming neutron stars or black holes, while low-mass stars become white dwarfs

Correct move:

Categorize star life cycles by initial mass when describing end-stage remnants

Wrong move:

Stating cosmological redshift is caused by stars moving through space towards/away from Earth

Why:

Cosmological redshift arises from the expansion of space itself stretching light wavelengths, not the local motion of individual galaxies

Correct move:

Distinguish between Doppler shift from local motion and cosmological redshift from universal expansion

3. Quick Reference Cheatsheet

Key Concept

Description/Formula

Relevant Sub-Topic

Orbital Speed

where = orbital radius, = orbital period

The Solar System

Axial Tilt

23.5° tilt of Earth's axis causes seasons, equinoxes, and solstices

Earth, Moon, Day/Night and Seasons

Low-Mass Star Lifecycle

Nebula → Protostar → Main Sequence → Red Giant → White Dwarf → Black Dwarf

Sun and Life Cycle of Stars

Hubble's Law

where = recessional speed, = galaxy distance, = Hubble constant

Universe: Redshift, Big Bang

Redshift

: longer observed wavelength of light from distant receding galaxies

Universe: Redshift, Big Bang

What's Next

You are now ready to start the first sub-topic in this unit, which covers the Earth-Moon system and the everyday observable phenomena of day, night, and seasonal variation. Work through all four sub-topics in sequence to build your knowledge from local astronomical systems to cosmological models of the universe. After completing this entire unit, you will progress to the next core unit covering electricity and magnetism for CIE IGCSE Physics 0625.