20 original exam-style questions - 9 pages of questions with a full mark scheme - free printable PDF.
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The Solar System consists of the Sun (a star) and the objects that orbit it: eight planets, their natural satellites (moons), dwarf planets, asteroids and comets. A star forms from a nebula, a cloud of dust and gas, which is pulled together by gravity to form a protostar; once the core becomes hot and dense enough, nuclear fusion begins and a new star is born. For most of its life, a star sits on the main sequence, a long, stable period in which nuclear fusion of hydrogen into helium in its core balances the inward pull of gravity. A star with a similar mass to the Sun eventually becomes a red giant, then loses its outer layers to leave a white dwarf, which cools over a very long time into a black dwarf. A much more massive star becomes a red super giant, then explodes as a supernova, leaving behind either a neutron star or, if the remaining core is massive enough, a black hole; elements heavier than iron are only formed during a supernova explosion. An object moving in a circular orbit has a constantly changing direction of velocity, so it is always accelerating towards the centre of the orbit; this centripetal acceleration is caused by a centripetal force, which for an orbiting planet, moon or satellite is provided by gravitational attraction. For a stable orbit, an orbit with a larger radius requires a slower orbital speed, because gravitational force is weaker at greater distances. Equation used in this worksheet: orbital speed = (2 x pi x orbital radius) / time period (v = 2 x pi x r / T). A satellite is an object that orbits a larger object; a geostationary satellite orbits above the equator with a time period of 24 hours, staying above the same point on the Earth's surface, while a low polar orbit satellite orbits much closer to the Earth with a much shorter time period, passing over a different strip of the Earth's surface on each orbit.