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  1. The fundamental principle to be understood concerning satellites is that a satellite is a projectile. That is to say, a satellite is an object upon which the only force is gravity. Once launched into orbit, the only force governing the motion of a satellite is the force of gravity. Newton was the first to theorize that a projectile launched ...

  2. Newton’s universal law of gravitation and Kepler’s laws describe the motions of Earth satellite s and interplanetary spacecraft as well as the planets. Sputnik, the first artificial Earth satellite, was launched by what was then called the Soviet Union on October 4, 1957. Since that time, thousands of satellites have been placed into orbit ...

  3. Lecture L15 - Central Force Motion: Kepler’s Laws. When the only force acting on a particle is always directed to wards a fixed point, the motion is called central force motion. This type of motion is particularly relevant when studying the orbital movement of planets and satellites. The laws which gov ern this motion were first postulated by ...

  4. Apr 10, 2022 · To illustrate how a satellite is launched, imagine a gun firing a bullet horizontally from the top of a high mountain, as in Figure 3.5.1 3.5. 1, which has been adapted from a similar diagram by Newton. Imagine, further, that the friction of the air could be removed and that nothing gets in the bullet’s way. Then the only force that acts on ...

  5. Key Concepts and Summary. The orbit of an artificial satellite depends on the circumstances of its launch. The circular satellite velocity needed to orbit Earth’s surface is 8 kilometres per second, and the escape speed from our planet is 11 kilometres per second. There are many possible interplanetary trajectories, including those that use ...

    • OpenStax
    • 2017
  6. The orbit of an artificial satellite depends on the circumstances of its launch. The circular satellite velocity needed to orbit Earth’s surface is 8 kilometers per second, and the escape speed from our planet is 11 kilometers per second. There are many possible interplanetary trajectories, including those that use gravity-assisted flybys of ...

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  8. Kepler’s Laws of Planetary Motion. Kepler’s First Law. The orbit of each planet about the Sun is an ellipse with the Sun at one focus. Figure 6.29(a) An ellipse is a closed curve such that the sum of the distances from a point on the curve to the two foci (f 1 f 1 size 12 {f rSub { size 8 {1} } } {} and f 2 f 2 size 12 {f rSub { size 8 {2 ...

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