Topic study hub

Solar system; stability of orbital motions; satellites

When applying this idea, Solar system; stability of orbital motions; satellites sits inside 4.8 Space physics and should be revised as a connected set of physical ideas, not as isolated definitions. Context: the topic brings together Our Solar System, The life cycle of a star, Orbital motion, natural and artificial satellites and asks students to move between description, calculation, graph interpretation and explanation where appropriate. Key Concept: identify the quantity, model or interaction first, then state how evidence or a mathematical relationship supports it. Worked Example: for a typical exam item, name the relevant principle, use the given data or diagram, and finish with a sentence that interprets the physical consequence. Exam Focus: keep command words visible; describe asks for features, explain asks for a causal link, calculate requires equation, substitution and unit, and evaluate needs evidence. Common Mistake: avoid using a nearby concept as a substitute, such as confusing field with force, current with potential difference, speed with acceleration, or red-shift evidence with the Big Bang model itself.

43

Objectives

215

Flashcards

215

Questions

90 min

Study time

AQAGCSEPhysicsSpace physics

Choose a revision tool

Start revising Solar system; stability of orbital motions; satellites

Syllabus checklist

What you need to know

43 objective pages available

Our Solar System12 objectives
  • (Physics only) State that the Sun is a star.
  • (Physics only) State that the Sun is one of many stars in the Milky Way galaxy.
  • (Physics only) State that the Milky Way galaxy is one of many billions of galaxies in the universe.
  • (Physics only) Describe the Solar System as the Sun, planets, dwarf planets, moons, asteroids and comets.
  • (Physics only) State that planets and dwarf planets orbit the Sun.
  • (Physics only) State that moons orbit planets.
  • (Physics only) Describe a moon as a natural satellite.
  • (Physics only) Describe artificial satellites as human-made objects that orbit planets or moons.
  • (Physics only) Distinguish planets from moons by what they orbit.
  • (Physics only) Distinguish stars from planets by explaining that stars produce their own light by fusion whereas planets do not.
  • (Physics only) Distinguish a galaxy from the universe.
  • (Physics only) Apply WS 1.4 when interpreting diagrams or models of the Solar System.
The life cycle of a star18 objectives
  • (Physics only) Describe a star as forming from a cloud of dust and gas called a nebula.
  • (Physics only) Describe how gravitational attraction pulls dust and gas together to form a protostar.
  • (Physics only) State that the temperature rises as the protostar becomes denser.
  • (Physics only) State that a star enters the main sequence when it becomes hot enough for hydrogen nuclei to fuse to form helium.
  • (Physics only) Explain that fusion of hydrogen nuclei releases energy in a main sequence star.
  • (Physics only) Explain that a main sequence star is stable because the forces within it are balanced.
  • (Physics only) Describe the balance in a main sequence star as gravity acting inwards and pressure from fusion energy acting outwards.
  • (Physics only) State that the Sun is currently a main sequence star.
  • (Physics only) Describe how a star about the same size as the Sun becomes a red giant.
  • (Physics only) Describe how a red giant becomes a white dwarf.
  • (Physics only) Describe how a white dwarf cools to become a black dwarf.
  • (Physics only) Describe how a star much more massive than the Sun becomes a red super giant.
  • (Physics only) Describe how a red super giant may explode as a supernova.
  • (Physics only) State that a supernova explosion distributes elements throughout the universe.
  • (Physics only) Describe how a supernova can leave behind a neutron star.
  • (Physics only) Describe how a supernova can leave behind a black hole if the remaining mass is large enough.
  • (Physics only) Compare the life cycle of a Sun-sized star with the life cycle of a much more massive star.
  • (Physics only) Apply WS 1.2 when using models to represent stages in the life cycle of a star.
Orbital motion, natural and artificial satellites13 objectives
  • (Physics only) State that gravity provides the force that allows planets and satellites to maintain circular orbits.
  • (Physics only) Explain that an object moving in a circular orbit is accelerating because its velocity is changing direction.
  • (Physics only) State that for a stable circular orbit the speed of the object is constant but its velocity changes.
  • (Physics only) Explain that the direction of the velocity of an orbiting object is at right angles to the force of gravity.
  • (Physics only) Describe the force of gravity on an orbiting object as acting towards the centre of the orbit.
  • (Physics only) Explain that a change in orbital radius changes the speed of an orbiting object.
  • (Physics only) State that for a given central object, a smaller orbital radius is associated with a higher orbital speed.
  • (Physics only) State that artificial satellites can orbit the Earth.
  • (Physics only) State that natural satellites such as moons can orbit planets.
  • (Physics only) Distinguish orbital motion from rotation.
  • (Physics only) Distinguish natural satellites from artificial satellites.
  • (Physics only) Apply WS 1.4 when interpreting diagrams of orbital motion.
  • (Physics only) Apply MS 1c and MS 3b when interpreting proportional relationships between orbital radius and orbital speed.

Key terms

space-63-term-01 classification Our Solar Systemspace-63-term-02 evidence Our Solar Systemspace-65-term-01 classification Our Solar Systemspace-65-term-02 evidence Our Solar Systemspace-62-term-01 classification Our Solar Systemspace-62-term-02 evidence Our Solar Systemspace-25-term-01 classification Our Solar Systemspace-25-term-02 evidence Our Solar Systemspace-60-term-01 classification Our Solar Systemspace-60-term-02 evidence Our Solar Systemspace-58-term-01 classification Our Solar Systemspace-58-term-02 evidence Our Solar System

Exam tips

  • Our Solar System exam tip 1: Use the named Space Physics term first, then link it to (Physics only) State that the Sun is a star with evidence or a clear sequence; add one boundary check for Our Solar System.
  • Our Solar System exam tip 2: Use the named Space Physics term first, then link it to (Physics only) State that the Sun is one of many stars in the Milky Way galaxy with evidence or a clear sequence; add one boundary check for Our Solar System.

Common mistakes

  • Our Solar System common mistake 1: Answer by clearly explaining how to (Physics only) State that the Sun is a star..
  • Our Solar System common mistake 1: Answer by clearly explaining how to (Physics only) State that the Sun is one of many stars in the Milky Way galaxy..

Practice preview

Continue by objective

Objectives are grouped by subtopic so students can jump straight to the exact skill they want to revise.

Related topics

Study nearby topics next

AQA GCSE Physics Solar system; stability of topic hub | ExamCompanion