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Planets orbit in ellipses from "summary" of Astronomy and Astro-physics by

Planets in our solar system move in an elliptical path around the Sun, following a set orbit determined by its mass, period and other factors. This motion is commonly known as an elliptical orbit, and it is a fundamental feature of the solar system.
  1. Our Solar System is composed of planets that all revolve around a central star called the Sun in an elliptical orbit.
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  3. All of these orbiting objects, including planets, asteroids, comets and moons, are affected by gravitation from the Sun and therefore move in paths governed by Newton’s laws of motion.
  4. As the orbiting bodies traverse their orbits, their speed and distance from the Sun varies due to gravitational forces and other influences.
  5. To describe these orbits mathematically, astronomers use the concept of an ellipse - a symmetrical closed curve with two foci - which has the property of making the sum of the distances from any point to each focus always equal.
  6. The shape of this orbit is determined by two factors: the force exerted by gravity from the Sun and the initial velocity of the planet when it was formed.
  7. This means that every celestial body follows its own path, which can vary greatly depending on its characteristics such as mass, density and distance from the Sun.
  8. Understanding how these trajectories work allow us to better understand the fundamental dynamics of our Solar System and how the planets interact with one another.
  9. Ellipses are special cases of conic sections, along with parabolas and hyperbolas, but are characterised by being completely closed inside a given area.
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Astronomy and Astro-physics

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