The Solar System (Edexcel GCSE Physics)
Revision Note
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Objects in the Solar System
The Solar System consists of:
The Sun
Eight planets
Natural and artificial satellites
Dwarf planets
Asteroids and comets
The objects in our solar system
The Sun & the Planets
The Sun lies at the centre of the Solar System
The Sun is a star that makes up over 99% of the mass of the solar system
There are 8 planets and an unknown number of dwarf planets which orbit the Sun
The gravitational field around planets is strong enough to have pulled in all nearby objects with the exception of natural satellites
The gravitational field around a dwarf planet is not strong enough to have pulled in nearby objects
Satellites
There are two types of satellite:
Natural
Artificial
Some planets have moons which orbit them
Moons are an example of natural satellites
Artificial satellites are man-made and can orbit any object in space
The International Space Station (ISS) orbits the Earth and is an example of an artificial satellite
Asteroids & Comets
Asteroids and comets also orbit the sun
An asteroid is a small rocky object which orbits the Sun
The asteroid belt lies between Mars and Jupiter
Comets are made of dust and ice and orbit the Sun in a different orbit to those of planets
The ice melts when the comet approaches the Sun and forms the comet’s tail
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The Planets
The 8 planets in our Solar System in ascending order of the distance from the Sun are:
Mercury
Venus
Earth
Mars
Jupiter
Saturn
Uranus
Neptune
There are 4 rocky planets: Mercury, Venus, Earth and Mars
There are 4 gas planets: Jupiter, Saturn, Uranus and Neptune
The eight planets of our Solar System
Distances between Planets in the Solar System
The planets and moons of the Solar System are visible from Earth when they reflect light from the Sun
The outer regions of the Solar System are around 5 × 1012 m from the Sun, which means even light takes some time to travel these distances
The light we receive on Earth from the Sun takes 8 minutes to reach us
The nearest star to us after the Sun is so far away that light from it takes 4 years to reach us
The Milky Way galaxy contains billions of stars, huge distances away, with the light taking even longer to be seen from Earth
The speed of light is a constant 3 × 108 m/s
Therefore, using the equation:
The time taken to travel a certain distance can be calculated by rearranging to:
Worked Example
The radius of Mercury's orbit around the Sun is 5.8 × 109 m.
Calculate the time taken for light from the Sun to reach Mercury.
Answer:
Step 1: State the equation for the time taken for light to travel a certain distance
Step 2: Substitute in the values
The distance travelled is the radius of the orbit
Distance, d = 5.8 × 109 m.
Speed = the speed of light, v = 3.0 × 108 m/s
Step 3: Round up the answer and include units
Examiner Tips and Tricks
You need to know the order of the 8 planets in the solar system. The following mnemonic gives the first letter of each of the planets to help you recall them:
My Very Easy Method Just Speeds Up Naming (Planets)
Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, (Pluto)
Of course, Pluto has been classed as a dwarf planet since 2006, so you shouldn't include it as one of the 8 planets, but old mnemonics still include it so that the mnemonic makes sense!
The Creation of the Solar System
The way humans have thought about the solar system has changed many times throughout history
Before the development of the telescope, these ideas were based on what could be seen with the naked eye
This restricted the details that could be gathered about the solar system, as asteroids, most of the satellites of other planets, and the most distant planets are not visible to the naked eye
Ancient Model of the Solar System
An Egyptian astronomer called Ptolemy (AD 100-168) described one of the earliest ideas for how the solar system is structured
Ptolemy’s model and many earlier ideas from scholars of the solar system had the Earth at the centre of it
Over time, though, it became apparent that the old model did not quite fit with observation due to more detailed observations of the motions of the planets
This was called the geocentric model of the solar system
Modern Model of the Solar System
Placing the Sun at the centre of the solar system and having the Earth and other planets orbit it gave a much more accurate explanation of astronomical observations
Nicolas Copernicus (1473-1543) first suggested changing the model of the solar system to one with the Sun at the centre
Detailed observations with telescopes have given us evidence that this is the correct idea
This is now the accepted heliocentric model of the solar system
The geocentric model vs. the heliocentric model
Worked Example
A long time ago, astronomers thought that the Earth was the centre of the Universe. This was called the geocentric model.The evidence for this model came from observations of the sky using the naked eye. After the telescope was invented, astronomers quickly gathered evidence that showed that the geocentric model is not correct. Describe the evidence both for the geocentric model and against the geocentric model.
Answer:
Step 1: Describe the evidence supporting the geocentric model
When observing the Sun, Moon, stars or planets with the naked eye, they appear to be moving across the sky and not just orbiting the Sun
Instead, they seem to appear to be going around the Earth
From simple observation, objects appear to move in the same direction and in a predictable pattern of movement which is the same each day
Step 2: Describe the evidence against the geocentric model
The moons of other planets (such as Jupiter) can clearly be seen to be orbiting the other planet and not the Earth
Careful observations of the Sun (and other objects) show their movements are, in fact, not quite the same each day
Detailed telescope observations show the planets of the Solar System do not move in a simple orbital path around the Earth
This is evidenced by the retrograde motion of planets, which can only be explained by a heliocentric model
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