6.1.3

The Solar System & The Accretion Model

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The Solar System

Our solar system is a small part of the Milky Way Galaxy. It is made up of:

The Sun

The Sun

  • The Sun is the only star in our solar system.
Planets and dwarf planets

Planets and dwarf planets

  • Planets and dwarf planets orbit around the Sun.
    • There are eight planets in our solar system (Pluto is a dwarf planet).
Moons

Moons

  • Moons are in orbit around many of the planets.
  • Moons are called natural satellites.
Comets and asteroids

Comets and asteroids

  • Comets and asteroids also orbit around the Sun.

The Accretion Model

Characteristics of the planets

Characteristics of the planets

  • The four inner planets (Mercury, Venus, Earth, Mars) are small and rocky.
  • The four outer planets (Jupiter, Saturn, Uranus, Neptune) are large and gaseous.
The accretion model

The accretion model

  • Billions of years ago, the Solar System began as a huge cloud of gas and dust (called a nebula) in space.
    • The cloud contained many different elements, such as hydrogen, helium, carbon, oxygen, and iron.
  • Slowly, gravity began pulling the gas and dust particles closer.
    • As particles collided, they stuck together, forming bigger and bigger clumps.
  • As gravity pulled the cloud inward, it started to rotate.
    • This rotation caused the cloud to flatten into a thin, spinning accretion disc with most material near the centre.
Formation of the Sun and planets

Formation of the Sun and planets

  • Most of the material moved to the centre of the disc, where gravity made it collapse and heat up.
    • This eventually formed the Sun.
  • Smaller clumps of dust and rock in the disc collided and stuck together.
    • These growing bodies are called planetesimals. Over time, they grew larger, becoming the planets.
Why are planets different?

Why are planets different?

  • Close to the Sun:

    • It was very hot, so gases like hydrogen and helium escaped.
    • Only heavy, solid materials stayed, forming the small, rocky inner planets.
  • Far from the Sun:

    • It was cooler, so gases could stay.
    • Planets here gathered huge amounts of gas around a rocky core, becoming the large, gaseous outer planets.
Jump to other topics
1

Motion, Forces & Energy

1.1

Physical Quantities & Measurement Techniques

1.2

Motion

1.3

Mass & Weight

1.4

Density

1.5

Forces: Effects of Forces

1.6

Forces: Turning Effects of Forces

1.7

Forces: Centre of Gravity

1.8

Momentum

1.9

Energy, Work, & Power: Energy

1.10

Energy, Work & Power: Work

1.11

Energy, Work & Power: Energy Resources

1.12

Energy, Work & Power: Power

1.13

Pressure

2

Thermal Physics

3

Waves

4

Electricity & Magnetism

4.1

Simple Phenomena of Magnetism

4.2

Electrical Quantities: Electric Charge

4.3

Electrical Quantities: Electric Current

4.4

Electromotive Force & Potential Difference

4.5

Electrical Quantities: Resistance

4.6

Electrical Energy & Electrical Power

4.7

Electric Circuits: Circuit Diagrams & Components

4.8

Electric Circuits: Series & Parallel Circuits

4.9

Electric Circuits: Action & Use

4.10

Electrical Safety

4.11

Electromagnetic Effects: Electromagnetic Induction

4.12

Electromagnetic Effects: The A.C. Generator

4.13

Magnetic Effect of a Current

4.14

Force on a Current-Carrying Conductor

4.15

Electromagnetic Effects: The D.C. Motor

4.16

Electromagnetic Effects: The Transformer

5

Nuclear Physics

6

Space Physics

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