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KS4 Physics Earth and Beyond 1 of 20 41 © Boardworks Ltd 2005 2004 Contents Earth and Beyond The solar system The life cycles of stars In orbit The Universe Summary activities 1 2 of 20 41 © Boardworks Ltd 2005 2004 Nuclear fusion In nuclear fusion reactions, lighter atomic nuclei are joined together (fused) to form heavier atomic nuclei. This process releases massive amounts of energy. In our Sun, a typical star, hydrogen is being fused to form helium. This provides the energy for life on Earth. When all the hydrogen is used up, other elements will be fused together to make even heavier elements. Not all elements are made in this way. The heaviest elements, some of which are found in your body, can only be made when stars explode. 1 3 of 20 41 © Boardworks Ltd 2005 2004 The Sun as our energy source The Sun is the source of energy for life on Earth. Where does this energy come from? The Sun is powered by nuclear fusion reactions. Atomic nuclei are joined together (fused) due to the very high pressures inside the Sun. What would happen on Earth if the Sun suddenly disappeared? There would be no light, all plants would die (no photosynthesis), all animals would die (no food source) and temperatures would drop. It would lead to the end of all life on Earth! 1 4 of 20 41 © Boardworks Ltd 2005 2004 Contents Earth and Beyond The solar system The life cycles of stars In orbit The Universe Summary activities 1 5 of 20 41 © Boardworks Ltd 2005 2004 The life cycles of stars 1 6 of 20 41 © Boardworks Ltd 2005 2004 Small stars Lighter stars, like our Sun, follow this life cycle: Nebula collapses due to its own gravity. Very small nebulae form failed stars. 1 7 of 20 41 Forms a star like our Sun. Expands to form a red giant. Outer layers of star drift away to leave a dense white dwarf. © Boardworks Ltd 2005 2004 Massive stars Stars that are much heavier than our Sun follow this life cycle: Forms a star more massive than our Sun. Larger nebula collapses due to its own gravity. Expands to form a massive red giant. Red giant collapses violently in a supernova explosion. Very dense neutron star formed. 1 8 of 20 41 © Boardworks Ltd 2005 2004 Really massive stars The end of the life cycle of really massive stars is different to that of massive stars. After a really massive red giant collapses in a supernova explosion, it leaves a star so dense that not even light can escape its gravitational pull. This is called a black hole! Some scientists believe that there are black holes at the centre of galaxies. If light cannot escape a black hole, then how can a black hole be observed? 1 9 of 20 41 © Boardworks Ltd 2005 2004 Black holes How can a black hole be observed? A black hole cannot be seen directly and even if it could it wouldn’t be black! A black hole is ‘seen’ by observing the effect it has on nearby matter. If there is a star nearby, matter from the star will spiral into the black hole and as it does so the matter emits X ray radiation which can be detected. 1 10ofof20 41 X rays © Boardworks Ltd 2005 2004 Birth of a star What is the correct order for these sentences about how a star is formed? This causes the ‘nebula’ to collapse. Gravity causes a dust and gas cloud to condense into a smaller volume. As the nebula collapses, temperatures and pressures inside the nebula increase. 1 11ofof20 41 When the temperature and pressure are great enough nuclear fusion starts. Eventually gravity and the outward pressure of escaping energy is balanced. At this stage, it is called a star. © Boardworks Ltd 2005 2004 Comparing the life cycles of stars Use these words below to complete the life cycles of different stars: small nebula white dwarf star larger than our Sun red giant 1 12ofof20 41 large nebula nebula massive red giant neutron star star like our Sun supernova © Boardworks Ltd 2005 2004 Comparing the life cycles of stars small nebula nebula large nebula star like our Sun star larger than our Sun red giant massive red giant white dwarf supernova neutron star 1 13ofof20 41 © Boardworks Ltd 2005 2004 Questions about stars 1. What two elements make up most of our Sun? hydrogen and helium 2. What is a nebula? A huge cloud of gas and dust from which a star is born. 3. What process has allowed the Sun to emit light and heat radiation over billions of years? nuclear fusion 4. Which is the most dense, a white dwarf or a neutron star? neutron star 5. Describe the possible fate of a star similar to our Sun. red giant white dwarf 1 14ofof20 41 © Boardworks Ltd 2005 2004 Contents Earth and Beyond The solar system The life cycles of stars In orbit The Universe Summary activities 1 15ofof20 41 © Boardworks Ltd 2005 2004 Orbiting the Sun 1. What force keeps the planets in orbit around the Sun? the Sun’s gravity 2. Which planet shown will feel this force… a) …the strongest? b) …the weakest? not to scale 1 16ofof20 41 © Boardworks Ltd 2005 2004 Questions about satellites 1. What are the two types of satellite? natural and artificial 2. Give an example of each type? natural – the Moon artificial – navigation, spy, military, weather, communications 3. Why are certain satellites, such as the Hubble Space Telescope, put into space? To view the Universe above the Earth’s atmosphere which can obstruct view from Earth. 1 17ofof20 41 © Boardworks Ltd 2005 2004 Artificial satellites – different orbits geostationary orbit Satellite stays above the same location on the Earth’s surface. This means that the speed of its orbit matches the Earth’s rotation. 1 18ofof20 41 polar orbit The satellite’s orbit passes over the poles, whilst the Earth spins underneath. This allows large areas of Earth to be seen and is used for mapping and weather monitoring. © Boardworks Ltd 2005 2004 Comparing orbits Complete this the table comparing the different types of orbits that artificial satellites can follow? 1 19ofof20 41 Polar Geostationary Height of orbit low high Orbital speed fast slow Orbits per day 3-4 1 Orbit position over poles above equator Example weather communications © Boardworks Ltd 2005 2004 Which type of orbit? Do these uses of satellites involve a polar orbit or a geostationary orbit? communications spy weather navigation monitoring ocean temperatures 1 20ofof20 41 geostationary polar polar and geostationary geostationary polar © Boardworks Ltd 2005 2004 Contents Earth and Beyond The solar system The life cycles of stars In orbit The Universe Summary activities 1 21ofof20 41 © Boardworks Ltd 2005 2004 Size in the Universe 1 22ofof20 41 © Boardworks Ltd 2005 2004 Matching words and definitions a star a planet Our Sun is one. a galaxy Billions of stars together - ours is called the Milky Way. the Universe the Solar System 1 23ofof20 41 There are nine of these in our Solar System. The Earth is one. The Sun, planets, moons, asteroids and comets make up this. All the galaxies and everything else. © Boardworks Ltd 2005 2004 Identify the different bodies a galaxy 1 24ofof20 41 a star the Universe © Boardworks Ltd 2005 2004 The Doppler effect Think about the noise a plane makes as it passes you. As the plane approaches, it sounds higher pitched... …as it moves away from you, it sounds lower pitched. This apparent shift in frequency is called the Doppler effect. The same thing happens with light: The wavelength of light emitted by approaching objects appears to be shortened (blue-shifted); The wavelength of light emitted by receding objects appears to be increased (red-shifted). 1 25ofof20 41 © Boardworks Ltd 2005 2004 Hubble and the expanding Universe Edwin Hubble (1889-1953) was a famous scientist who examined the light from nearby galaxies. He made two important observations: 1. That most of the galaxies’ light was shifted towards the red end of the spectrum; 2. The further away a galaxy was, the more its light was red-shifted. From his observations, Hubble made these conclusions: 1. That most galaxies were moving away from our own; 2. The further away a galaxy was, the faster it was moving away from us; 3. That the Universe must be expanding. 1 26ofof20 41 © Boardworks Ltd 2005 2004 The big-bang theory The big-bang theory states that the Universe is expanding due to a large ‘explosion’ (big bang) billions of years ago. Evidence to support this theory includes: 1. The Cosmic Microwave Background Radiation (CMB), which is thought to be an ‘echo’ of the initial explosion. 2. Hubble’s observations about red-shifted light. This theory gives rise to different fates for the Universe: 1.If the mass of the Universe is large enough, it will eventually start to contract due to gravity – closed Universe. 2.If the mass of the Universe is smaller, it will expand forever as there is not enough gravity to halt its expansion – open Universe. 1 27ofof20 41 © Boardworks Ltd 2005 2004 Steady state theory The steady state theory states that the Universe is expanding and, as it expands, matter is created to maintain a uniform universal density of matter. Evidence to support this theory is Hubble’s observations about red-shifted light. However, the steady state theory has become less popular since the discovery of Cosmic Microwave Background Radiation (CMB). 1 28ofof20 41 © Boardworks Ltd 2005 2004 Are we alone? There are many different opinions about life in the Universe: For life to exist there must be liquid water, on a planet or moon and oxygen. The Universe is so big, We are all aliens, life even if there are aliens, began on comets and they are too far away for asteroids and transferred us to ever meet them. to the Earth when they collided with it. Life exists on Earth and only on Earth. There are 10 stars in the universe. There must be If there are aliens they If there are aliens, they would have contacted us by now. 21 will probably not look like you or me. 1 29ofof20 41 life on planets around some of them. © Boardworks Ltd 2005 2004 Is there life out there? Many people believe that we are not the only intelligent life in the Universe. The challenge for scientists is to find evidence of other life. 1 30ofof20 41 © Boardworks Ltd 2005 2004 Contents Earth and Beyond The solar system The life cycles of stars In orbit The Universe Summary activities 1 31ofof20 41 © Boardworks Ltd 2005 2004 Glossary (1) black hole – An object in space that forms after a really massive star collapses in a supernova. Its gravity is so strong that nothing can escape its pull. comet – A lump of rock and ice which has a very elliptical orbit around the Sun. galaxy – A vast collection of billions of stars. geostationary orbit – The path of a satellite that stays above the same position on the Earth’s surface and orbits at the same speed as the Earth rotates. meteor – A lump of material from space that burns up in the Earth’s atmosphere. meteorite – A large meteor that does not completely burn up in the Earth’s atmosphere and crashes to Earth. nebula – A massive cloud of gas and dust in which a star is formed. 1 32ofof20 41 © Boardworks Ltd 2005 2004 Glossary (2) neutron star – The very dense core that remains after a massive red giant collapses in a supernova. nuclear fusion – The process in which lighter atomic nuclei are joined together to form heavier atomic nuclei and a massive amount of energy is released. polar orbit – The path of a satellite which passes over the North and South poles. satellite – Any object that is in orbit around a larger object. red giant – A star that has expanded and has a red glow. supernova – The huge explosion that occurs when a massive red giant is at the end of its life. white dwarf – The core that remains after the outer layers of a small red giant drift away. 1 33ofof20 41 © Boardworks Ltd 2005 2004 Anagrams 1 34ofof20 41 © Boardworks Ltd 2005 2004 Multiple-choice quiz 1 35ofof20 41 © Boardworks Ltd 2005 2004