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HW4 due - Yale Astronomy
HW4 due - Yale Astronomy

... Please  give  answers  in  both  light-­‐minutes  and  astronomical  units.   Assume  that  the  planets  have  circular  orbits.   [HINT:  Draw  a  diagram.]   [HINT:  A  light-­‐minute  is  a  distance:  how  far  light  goes  in  1   ...
ASTRONOMY 120
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... By setting these two equations equal, we can figure out the centripetal acceleration of the Earth about the Sun, or conversely, if we know the Earth's acceleration, we can figure out the Sun's mass. Centripetal acceleration is a  ...
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PPT File - Brandywine School District
PPT File - Brandywine School District

... Cassini is the first spacecraft to orbit Saturn. The NASA orbiter is studying the intriguing features of Saturn's system of rings and moons. It also delivered the European Space Agency's Huygens Probe into the atmosphere of Saturn's moon Titan. The spacecraft reached speeds of 70,700 mph on its way ...
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... Cassini is the first spacecraft to orbit Saturn. The NASA orbiter is studying the intriguing features of Saturn's system of rings and moons. It also delivered the European Space Agency's Huygens Probe into the atmosphere of Saturn's moon Titan. The spacecraft reached speeds of 70,700 mph on its way ...
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... direction means that it’s getting around the cirlce in less time, so therefore P would be lower. A number of you indicated that the eccentricities of the orbits would change (either to be higher or lower). This is not necessarily the case. Were you to take the planets in their current orbits and wit ...
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... Ocean Tides and the Sun • The sun also contributes to ocean tides, but since it is further away, it influences tides to a lesser extent • Spring Tides – A high or low tide that occurs when the sun, Earth and the moon are all lined up so that the tides due to the sun and the moon coincide, making th ...
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Mercury Mercury is a dead planet and the

... pieces  of  unfinished   words  left  over  from  the   early  solar  system.     Collisions  frequently   occur  between  the  rocky  leftovers.    Occasionally,  Jupiter’s   gravity  nudges  an  asteroid  out  of  its  orbit  and  sends ...
Assignment 1 - utoledo.edu
Assignment 1 - utoledo.edu

... d. it orbits (revolves around) the Sun e. it is much, much larger than any other planet ...
Name: Period: ______ Date: 1/16/07
Name: Period: ______ Date: 1/16/07

... What is the nearest star to Earth? Our sun is the nearest star. It is about 150,000,000 km. away. The next closest star to Earth is Proxima Centauri. Proxima Centauri is 40 trillion (40,000,000,000,000) kilometers from Earth. Such a large number is difficult to understand and use in calculations. Fo ...
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solutions

... Thus, rotation at ω = 24hrs ≈ 7 × 10−5 s−1 yields a total energy of about 1035 ergs. As far as the energy in a nuclear bomb: we could simply take a standard yield, i.e. maybe a megaton bomb (which means its energy yield is equivalent to 1 megaton of TNT; or about 5 PJ = 5 × 1015 J = 5 × 1022 ergs); ...
LESSON PLANS Week/Date: Dec. 1, 2014 Grade/Subject: Science
LESSON PLANS Week/Date: Dec. 1, 2014 Grade/Subject: Science

... Daily Objective Students will discover various parts of the Solar System and how they move through time. ...
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Geocentric model



In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.
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