Space Physics: The Solar System and Orbits
Space Physics: The Solar System and Orbits
The Solar System
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The solar system consists of the Sun, planets, dwarf planets, moons, asteroids, and comets.
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The Sun is located at the centre of the solar system and is a star.
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Planets, dwarf planets and their moons, as well as many asteroids and comets, orbit around the Sun.
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The eight recognised planets in our solar system are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
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Dwarf planets, such as Pluto, are smaller bodies that have not cleared their orbital path of other debris.
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Comets are icy bodies that develop tails as they approach the Sun.
Orbits
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The gravitational pull of the Sun is what keeps planets and other bodies in their orbits.
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In the solar system, all planets move in elliptical (oval-shaped) orbits around the Sun following Kepler’s first law of planetary motion.
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The closer a planet is to the Sun, the stronger the Sun’s gravitational pull and the faster the planet moves.
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Orbital speed varies depending on the distance a planet or object is from the Sun: objects further away from the Sun move more slowly than those closer to it.
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Satellites, both natural (like moons) and artificial, also follow elliptical orbits around the planets they orbit.
Gravitational Field Strength
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The force of gravity decreases with distance. It is stronger closer to a planet and weaker the further away you are.
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This change in gravitational field strength explains why objects weigh less the further they are from the centre of the Earth.
Centripetal Force
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When bodies move in circular paths, they constantly change direction, which means that they are accelerating.
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This acceleration is caused by a resultant force, known as a centripetal force, which always acts towards the centre of the circle.
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In the case of orbits, the centripetal force is provided by gravity.
** Satellites and their uses**
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Artificial satellites are human-made objects that orbit Earth or other celestial bodies.
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There are two types of artificial satellites: geostationary satellites, which stay above the same point on the Earth’s equator, and low Earth orbit satellites, which orbit closer to the Earth and travel around it very quickly.
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Uses for these satellites include communications, weather forecasting, observing the Earth’s climate, and scientific research.
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The time periods and paths of satellites depend on their height above the Earth. The higher the satellite is above the Earth, the longer its orbital period.
Space Travel
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Missions such as those conducted by NASA’s Apollo programme have allowed astronauts to land on the moon and return safely to Earth.
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Modern space exploration includes unmanned missions to Mars, the use of space telescopes and the international space station.
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The challenges of such exploration include surviving in a vacuum and dealing with extreme temperatures, managing power supplies, taking off and landing, and the long durations of space travel.