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The Solar System
The Solar System

... and nine known planets and the moons that orbit those planets. • The force of gravity keeps planets in orbit around the sun. ...
Astronomical Figures
Astronomical Figures

... Astronomical Figures 190 BC - 120 BC Mathematicians ...
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50 FACTS about SPACE

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Homework Assignment 1 — Solutions
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... (a). The first day of summer is the summer solstice, when the Sun is at a declination +23◦ 300 above the celestial equator (see Fig. 1.12). For an observer at 42◦ N latitude, the Sun will appear 42◦ − 23◦ 300 = 18◦ 300 from the zenith, corresponding to an altitude of 71◦ 300 above the horizon. (b). ...
PTYS/ASTR 206 – Section 2 – Spring 2006 Practice Exam 1 Note
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Seasonal Visibility of Stars, and Visibility of Planets in 2014
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Clicker Frequency Setting Lecture 2 Outline
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Geocentric vs. Heliocentric Models of the Solar System
Geocentric vs. Heliocentric Models of the Solar System

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How long does it take sunlight to reach the Earth?
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The Structure of Our Solar System
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Celestial Sphere - Otterbein University
Celestial Sphere - Otterbein University

... • A computer program that simulates the vision of the sky during day and night Things to observe: • Set your position on Earth: observe how view of sky changes as you move E,W, N,S • Note the distribution of sunlight on Earth! • Rotation is around Polaris which is not in zenith ...
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... Absolute  Magnitude  -­‐  how  bright  a  star  really  is  if  all  stars  were  the  same  distance  from  us     A.M.  -­‐  Ante  Meridiem,  meaning  before  the  middle  of  the  day   Apparent  Magnitude  -­‐  how  bright  a  star  appears  in  our  sky   The  Arctic  Circle  -­‐  the  latitude ...
Section 22.2 The Earth-Moon-Sun System
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...  The sidereal month is the true period of the moon’s revolution around Earth. It lasts 27 1/3 days.  The difference of two days between the synodic and sidereal cycles is due to the Earth–moon system also moving in an orbit around the sun.  The moon’s period of rotation about its axis and its rev ...
(Lecture 3). The Solar System in the Night Sky (cont)
(Lecture 3). The Solar System in the Night Sky (cont)

... The Solar System in the Night Sky (Part 2) → Initial pleasantries…watch the position and appearance of the moon over the next few days.  Let’s think about the significance of the fact mentioned in the previous lecture. 1 tropical year is 365.2422 mean solar days. To simplify things a bit, let’s ass ...
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PowerPoint 演示文稿

... 100,000 light-years across. It is about 14 billion years old and takes 225 million years or so to rotate(旋转) once. Like all spirals, it contains plenty of gas and dust, from which new stars are formed. The dense nucleus(核心) is the oldest part and has no gas left for new star. ...
Our solar system - astronomyuniverse
Our solar system - astronomyuniverse

... Some clumps got bigger, as particles and small clumps stuck to them, forming planets and moons. At the center of the cloud, where planets like Earth formed, only rocky material could stand the great heat. Icy matter settled in the outer region of the disk along with rocky material, where the giant p ...
3.1 Notes
3.1 Notes

... •Weather is the condition of the atmosphere in a certain place at a specific time. • The climate of an area is its longterm typical weather pattern. • The climate of an area is determined by many things; the most important is the earth’s position in relation to the sun. 2.6 describe factors that inf ...
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Extraterrestrial skies



In astronomy, the term extraterrestrial sky refers to a view of outer space from the surface of a world other than Earth.The sky of the Moon has been directly observed or photographed by astronauts, while those of Titan, Mars, and Venus have been observed indirectly by space probes designed to land on the surface and transmit images back to Earth.Characteristics of extraterrestrial skies appear to vary substantially due to a number of factors. An extraterrestrial atmosphere, if present, has a large bearing on visible characteristics. The atmosphere's density and chemical composition can contribute to differences in colour, opacity (including haze) and the presence of clouds. Astronomical objects may also be visible and can include natural satellites, rings, star systems and nebulas and other planetary system bodies.For skies that have not been directly or indirectly observed, their appearance can be simulated based on known parameters such as the position of astronomical objects relative to the surface and atmospheric composition.
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