Understanding Our Universe
Understanding Our Universe
3rd Edition
ISBN: 9780393614428
Author: PALEN, Stacy, Kay, Laura, Blumenthal, George (george Ray)
Publisher: W.w. Norton & Company,
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Chapter 2, Problem 6QAP
To determine

The motion of Sun, Moon and stars.

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Given exactly 360° in a circle and 365.24 days in a year, how many degrees per day does one's view of the night sky shift? (This assumes one looks in exactly the same direction, at the meridian - the middle of the sky defined by a line across it running due north to due south, at exactly the same time each night.)
6. A star is observed to cross the meridian (due south) at an elevation of 34°, as seen from an observatory sited at a latitude of 42° north. What is the declination of the star? At the moment of transit, a clock running on Universal Time (UT) read 03 h 16min 24 s. At the previous midnight, the sidereal time was 14h 38 min 54 s. Calculate the Right Ascension of the star.
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Time Dilation - Einstein's Theory Of Relativity Explained!; Author: Science ABC;https://www.youtube.com/watch?v=yuD34tEpRFw;License: Standard YouTube License, CC-BY