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Kepler satellite

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kepler satellite

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In February 2009, NASA will launch the Kepler satellite. This mission is designed to discover Earth-like planets around Sun-like stars. The satellite has a 0.95-m telescope with
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Kepler's First Law: Satellite orbits are elliptical Paths with the Earth at one focus of the ellipse. Kepler's Second Law: A line between the center of the Earth and the satellite
Johann Kepler developed empirically three laws of planetary motion, based on conclusions drawn from the extensive observations of Mars by Tycho Brahe
Kepler Mission to find Earth-size planets in the habitable zones of stars
Kepler satellite Kepler's photometer (a device that measures the brightness of light) will function
F c = F G m satellite v 2 R Kepler's 3rd Law Took several more years to work out, but the creation looked like this: R F G The force responsible for delivering the required
Let a line ("radius vector") be drawn from the center of the Sun to the planet (or from the center of Earth to the satellite). Kepler's law states:"

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