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Motion across the Sky
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Learning goals We are learning how celestial objects move in our night sky. We are learning to distinguish between different types of satellites.
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Ecliptic Ecliptic: the path across the sky that the Sun, the Moon, the planets, and the Zodiac constellations appear to follow over the course of a year
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Changing Views in the Night Sky
changing views in the night sky are due to: Earth’s rotation distance celestial object is from Earth Earth’s revolution around the Sun
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Retrograde Motion retrograde motion: the apparent motion of an object in the sky from east to west, rather than west to east occurs because Earth travels around the Sun faster than the outer planets
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satellites
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history 1957 USSR: Sputnik 1 – size of football
Sputnik 2 – much larger 1958 USA: Explorer 1 Alouette 1: Canada ! Anik 1 in 1972: transimitted 12 tv channels
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orbit Earth’s gravity pulls – satellite must have enough velocity
Low earth orbit – up to 2000 kms military and earth observation International Space Station (430km above earth) travels at a speed of km/h
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Geostationary orbit Satellite which orbits Earth at same rate as Earth rotates km used to broadcast tv, radio and internet
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gps Global Positioning System medium earth orbit (up to 35000km)
uses three satellites to triangulate position
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Learning goals We are learning how celestial objects move in our night sky. We are learning to distinguish between different types of satellites.
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Homework: Section 8.9 #1, 3-7 Section 8.11 #7
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