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Lecture 2

Lecture 2 - September 12-astronomy lecture.docx
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Department
Natural Science
Course
NATS 1745
Professor
Robin Metcalfe
Semester
Fall

Description
September 12, 2011 -last time we discussed archaeoastronomy, how there are sites that show these civilizations understood some form of relationship to the sun, today we’ll discuss how they were able to determine these things and how much astronomy they were actually able to comprehend The Sun’s Daily Cycle 1 . due to Earth’s 24-hour eastward-spin around its polar axis, the Sun moves westward across the sky; it rises in the east, reaches its highest point at noon, then sets in the west 2. N-hemisphere: Sun is mostly seen on the South side of the sky, reaching due (exact) South at noon 3. S-hemisphere: Sun is mostly seen on the North side of the sky, reaching due North at noon. The Sun’s Annual Cycle Fall and Spring Equinox (~Sept 23, ~Mar 21): Sun rises due E and sets due W, spending equal time above and below the horizon (equal day and night). (Equinox: Latin for “equal night”) on other days of year it’s a little bit off east when it rises, and a little bit off west. 2. Winter Solstice (~Dec 23): Sun rises and sets at its southernmost position, traversing a short, low arc in sky (shortest day of the year and lowest noon sun) (Solstice: Latin for “solar standstill”). -causes day to be shorter, arc is significantly lower than on the day of the equino
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