Neptune's elliptical, oval-shaped orbit keeps the planet an average distance from the sun of almost 2.8 billion miles (4.5 billion kilometers), or roughly 30 times as far away as Earth, making it invisible to the naked eye
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When Johannes Kepler made the intuitive leap in the early 1600s to realize that planetary orbits were not circular, as they had been assumed to be for millennia, he stuck to the trusty ellipse. Indeed, the ellipse accurately and precisely describes the motions of all the major planets.
When Johannes Kepler made the intuitive leap in the early 1600s to realize that planetary orbits were not circular, as they had been assumed to be for millennia, he stuck to the trusty ellipse. Indeed, the ellipse accurately and precisely describes the motions of all the major planets.In this view, a circle is just a special case of the ellipse, where the eccentricity (a term which, for lack of a better phrase, measures the "stretchiness" of an ellipse) is exactly 0. In our solar system, Venus and Neptune have nearly circular orbits with eccentricities of 0.007 and 0.009, respectively, while Mercury has the most elliptical orbit with an eccentricity of 0.206.
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Answer:
the answer is A.NEPTUNE
Explanation:
Neptune's elliptical, oval-shaped orbit keeps the planet an average distance from the sun of almost 2.8 billion miles (4.5 billion kilometers), or roughly 30 times as far away as Earth, making it invisible to the naked eye
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Answer:
A.Neptune
Explanation:
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carry on answering the module and carry on learning…(⌒∇⌒)
When Johannes Kepler made the intuitive leap in the early 1600s to realize that planetary orbits were not circular, as they had been assumed to be for millennia, he stuck to the trusty ellipse. Indeed, the ellipse accurately and precisely describes the motions of all the major planets.
When Johannes Kepler made the intuitive leap in the early 1600s to realize that planetary orbits were not circular, as they had been assumed to be for millennia, he stuck to the trusty ellipse. Indeed, the ellipse accurately and precisely describes the motions of all the major planets.In this view, a circle is just a special case of the ellipse, where the eccentricity (a term which, for lack of a better phrase, measures the "stretchiness" of an ellipse) is exactly 0. In our solar system, Venus and Neptune have nearly circular orbits with eccentricities of 0.007 and 0.009, respectively, while Mercury has the most elliptical orbit with an eccentricity of 0.206.