Universe: Stars And Galaxies
Universe: Stars And Galaxies
6th Edition
ISBN: 9781319115098
Author: Roger Freedman, Robert Geller, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 2, Problem 28Q
To determine

The reason behind the tilt of ecliptic with respect to the celestial equator.

The path along which the sun appears to move with respect to Earth.

The amount of degree by which the sun moves on the celestial sphere each day.

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Students have asked these similar questions
If you go out at midnight and look at constellations along the zodiac (i.e. more or less along the ecliptic plane), and then go out at midnight six months later and do the same thing, by how many degrees will the center of your view (along the ecliptic, looking to the south) have shifted during those six months?
If you go on vacation down to the Florida Keys, the North Star (aka Polaris) located near the North Celestial Pole is found at an altitude of approximately 25 degrees above the horizon. Why is it found near that altitude?
If you are at latitude 25 degrees north of Earth's equator, what is the angular distance (in degrees) from your zenith to the north celestial pole? What is the shortest angular distance (in degrees) from your nadir to the north celestial pole?
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