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Intermediate - Maggie`s Earth Adventures
Intermediate - Maggie`s Earth Adventures

... 2. Why do you think the elements in the chart that shows “What Makes Up the Sun?” do not add up to one hundred? _______________________________________________________ ___________________________________________________________________________ ________________________________________________________ ...
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... There are important areas of the solar system to know about. -The Asteroid Belt – the area between Mars and Jupiter where most of the solar systems asteroids and meteoroids orbit the sun. The Kuiper Belt- area outside the planet Neptune, containing several dwarf planets as well as smaller objects, ...
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... • Moves with the seasons north and south of the equator between the Tropics of Cancer and Capricorn • Close to the equator, the ITCZ influences the weather twice a year during the equinoxes in March and September. • Near the Tropic of Cancer, the ITCZ approaches only during June and July, and climat ...
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Fulltext PDF - Indian Academy of Sciences
Fulltext PDF - Indian Academy of Sciences

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Astronomy - Bemidji State University
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... years, he made very accurate observations of the night sky, all without the aid of a telescope, which had not yet been invented. Tycho also built the world's first observatory and kept a star catalogue with over 1000 stars. Tycho's records were used by Johan Kepler to describe the orbits of planets ...
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Copernican heliocentrism



Copernican heliocentrism is the name given to the astronomical model developed by Nicolaus Copernicus and published in 1543. It positioned the Sun near the center of the Universe, motionless, with Earth and the other planets rotating around it in circular paths modified by epicycles and at uniform speeds. The Copernican model departed from the Ptolemaic system that prevailed in Western culture for centuries, placing Earth at the center of the Universe, and is often regarded as the launching point to modern astronomy and the Scientific Revolution.Copernicus was aware that the ancient Greek Aristarchus had already proposed a heliocentric theory, and cited him as a proponent of it in a reference that was deleted before publication, but there is no evidence that Copernicus had knowledge of, or access to, the specific details of Aristarchus' theory. Although he had circulated an outline of his own heliocentric theory to colleagues sometime before 1514, he did not decide to publish it until he was urged to do so late in his life by his pupil Rheticus. Copernicus's challenge was to present a practical alternative to the Ptolemaic model by more elegantly and accurately determining the length of a solar year while preserving the metaphysical implications of a mathematically ordered cosmos. Thus his heliocentric model retained several of the Ptolemaic elements causing the inaccuracies, such as the planets' circular orbits, epicycles, and uniform speeds, while at the same time re-introducing such innovations as,Earth is one of several planets revolving around a stationary Sun in a determined orderEarth has three motions: daily rotation, annual revolution, and annual tilting of its axisRetrograde motion of the planets is explained by Earth's motionDistance from Earth to the Sun is small compared to the distance to the stars.↑ 1.0 1.1 ↑
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