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PHYS 390 Lectures 1/2 - The Big Picture 1/2
PHYS 390 Lectures 1/2 - The Big Picture 1/2

... Earth-Sun distance is defined as the Astronomical Unit (AU) and has a modern value of 1 AU = 1.4960 x 108 km ...
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... release – travelling at 37,000km/h. it could punch a crater in the comet big enough to swallow Rome’s Coliseum.” – Taken from http://news.bbc.co.uk/2/hi/science/nature/4162869.stm What is the purpose of the Deep Impact mission? A. To divert the comet from a collision course with Earth B. To investig ...
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... precise, detailed map of the sky as defined by the fixed stars. (The stellar patterns don’t change perceptibly over human lifetimes.) 2. Make similar measurements, night after night, to see how the moving dots of light (the planets) change position over time. ...
Chapter 13: Earth, Moon, and Beyond
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...  As Earth revolves around the sun, different parts of Earth are tilted toward Earth.  When your part of Earth is tilted toward the sun, it is summer for you.  The path that Earth moves on around the sun is called its orbit. ...
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... though it appears as though the Sun is moving! The Sun is the force which keeps our solar system together! • Rotation – spinning of Earth on its axis (23 degrees), which occurs once every 24 hours. • Earth moves around the Sun in a regular, curved path called an orbit • It takes about one year for E ...
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... a diameter; the observations are made at midnight with a full moon. The curvature of the earth, effects of atmospheric refraction, and further corrections are neglected. The geometrical situation is pictured above. Parallel rays of light from a distant star are received by the two observers OW and O ...
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... the top of a 5-m-tall mast on a ship that is 8 kilometers away • If you threw a ball fast enough to go a horizontal distance of 8 kilometers during the time (1 second) it takes to fall 5 meters, it would follow the curvature of Earth! • This would be about 29,000 km/hr (or 18,000 mi/hr) • At this sp ...
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... 38. Why are different constellations visible in the night sky throughout the year? (A picture might help you with this one.) The difference in Earth’s position over a year changes what we can see because it is daylight when some constellations are in the sky. Those overhead during the day change fro ...
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The Moon - Kaufman ISD
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Dialogue Concerning the Two Chief World Systems



The Dialogue Concerning the Two Chief World Systems (Dialogo sopra i due massimi sistemi del mondo) was a 1632 Italian-language book by Galileo Galilei comparing the Copernican system with the traditional Ptolemaic system. It was translated into Latin as Systema cosmicum (English: Cosmic System) in 1635 by Matthias Bernegger. The book was dedicated to Galileo's patron, Ferdinando II de' Medici, Grand Duke of Tuscany, who received the first printed copy on February 22, 1632.In the Copernican system the Earth and other planets orbit the Sun, while in the Ptolemaic system everything in the Universe circles around the Earth. The Dialogue was published in Florence under a formal license from the Inquisition. In 1633, Galileo was found to be ""vehemently suspect of heresy"" based on the book, which was then placed on the Index of Forbidden Books, from which it was not removed until 1835 (after the theories it discussed had been permitted in print in 1822). In an action that was not announced at the time, the publication of anything else he had written or ever might write was also banned.
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