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I.   Astronomy of the Earth's Motion in Space

    Here is an algebra-based overview of astronomy and space-flight, from pre-telescope discoveries to the space age. It is meant for personal study and reference, also as a resource for middle school (parts), high school (mostly) and beginning college. Starting with the apparent motions of the Sun and stars across the night sky, it explains the seasons of the year, latitude and longitude, time zones and universal time, and the basics of navigation.

    Next calendars are described--Julian and Gregorian, Metonic (esp. Jewish), Moslem, Persian and even Maya.

    After that the site tells how the spherical shape of the Earth was recognized and measured, leading to the formula for the distance of the horizon, the concept of parallax and the derivation of the Moon's distance by ancient Greeks. The Greeks also tried to derive the distance of the Sun, starting the road to heliocentric theory, continued by Ptolemy, Copernicus, Galileo and Kepler.

    Folowing this is a fairly comprehensive tour of the solar system and its planets, ending in a comprehensive discussion of Kepler's laws and planetary orbits, which serves as a bridge to the next section, on Newtonian Mechanics.

    Interspersed with the above are three web pages on the Moon (which may also be tied to the Greek calculations of the Moon's distance) and one on the precession of the equinoxes, connected to the Milankovitch theory of ice ages.



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Author and Curator:   Dr. David P. Stern
     Mail to Dr.Stern:   stargaze["at" symbol]phy6.org .

Last updated: 3-27-2014


Above is background material for archival reference only.

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