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Earth, Moon, and Sun - Effingham County Schools
Earth, Moon, and Sun - Effingham County Schools

... 27. How did the Earth form? While solar gas and dust (nebula) were swirling around and slowly condensing to form the Sun, a small part of the nebula escaped the Sun’s gravity and became trapped in an orbit around the Sun. 28. Why do we have a leap year every four years? The Earth actually takes 365 ...
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... The Sun The sun is a relatively small star whose projected lifetime on the main sequence is ~ 11 billion years. Theory and observations of stars similar to the sun suggest that the luminosity has increased 25-30% over the last 4.5 billion years. Despite the increasing energy delivered to Earth, many ...
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An Introduction To Parallax

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Chapter 19 The Solar System

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GEK - National University of Singapore

... 3) [Hubble’s Law and Cepheids] a) What is Hubble’s Law and how it changes our view on universe? Discuss. Hubble’s Law: Mathematically expresses the idea that more distant galaxies move away form us faster; its formula is ν=Ho x d, where ν is the galaxy’s speed away from us, d is its distance, and H ...
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Astro 205 Ch. 2

... •  Early  observers  had  a  geocentric  model  of  the   universe  (Earth  at  center).   •  Ptolemy  created  a  model  in  which  planets  moved  on   small  wheels  aNached  to  a  larger  wheel.   •    The  small  circle  is  cal ...
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Science_Jeopardy_Q3 - Galena Park ISD Moodle

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Sept2 - University of Arizona
Sept2 - University of Arizona

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Chapter 7 Notes

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Shape of the Earth

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History of Astronomy
History of Astronomy

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Part I: Moons, Asteroids, and Comets
Part I: Moons, Asteroids, and Comets

... 1.  What is a moon? _________________________________________________________________________ 2.  How many moons are in our solar system? _________________________________________________________________________ 3.  Do all planets have moons? _________________________________________________________ ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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