Retrograde Motion.(Read the following question and post your answer to the discussion board. Stimulate discussion! Respond to at least two of your classmate's posts." This will have two parts to it.

For centuries, people had no simple explanation for what causes the apparent retrograde motion of the planets in the sky. Today, we have a straight forward explanation, but it can still be a tough topic to understand. What confuses you most about the concept of planetary retrograde motion (or does it all make perfect sense to you)?For this week's discussion activity, you are asked to explain what you find confusing or interesting about retrograde motion.

Helpful reading " Retrograde Motion One phenomenon that aincient astronomers had difficulty explaining was the retrograde motion of the planets.

Over the course of a single night, a planet will move from East to West across the sky, like any other celestial object near the ecliptic. (Most objects in our sky appear to rise somewhere on the Eastern horizon and set somewhere on the Western horizon. The only exceptions are stars near the North celestial pole, that stay above the horizon all the time and appear to make counterclockwise circles around the celestial pole. As one travels further North, the region of the sky that remains above the horizon at all times becomes larger, until the entire sky appears -to an observer at the North Pole- to be simply circling the North star.

As one ravels South, the region that remains above the horizon becomes smaller, diminishing to zero size for an observer on the Equator. If one continues South of the Equator, one would observe a progressively larger region surrounding the South celestial pole that remains above the horizon at all times. Stars in that region would appear to circle the South celestial pole in clockwise circles.)

If observed from one night to the next, however, a planet appears to move from West to East against the background stars most of the time. Occasionally, however, the planet's motion will appear to reverse direction, and the planet will, for a short time, move from East to West against the background constellations. This reversal is known as retrograde motion, and is illustrated in the following animation. Apparent Motion of Mars Against Background Stars Oct 13, 1996 - Jul 26, 1997 (This animated gif was converted from a QuickTime movie that I obtained from Dr. Ted Snow's web site at The University of Colorado, Boulder.) Ptolemaic Explanation The model of the solar system developed by Ptolemy (87 - 150 A.D.) was a refinement of Aristotle's (384 - 322 B.C.) universe.

This model consisted of a series of concentric spheres, with the Earth at the center (geocentric). The motions of the Sun, Moon, and stars was based on perfect circles. To account for the observed retrograde motion of the planets, it was necessary to resort to a system of epicycles, whereby the planets moved around small circular paths that in turn moved around larger circular orbits around the Earth. This accounts for retrograde motion, as shown in the animation below: Retrograde Motion in the Ptolemaic (Geocentric) System (This animated gif was obtained from Dr. Stephen J. Daunt's Astronomy 161 web site at The University of Tennesee, Knoxville.) In its final form, the model was extremely complicated, requiring many nested levels of epicycles, and with even the major orbits offset so that they were no longer truly centered on the Earth.

Despite all of this fine tuning, there remained significant discrepancies between the actual positions of the planets and those predicted by the model. Nevertheless, it was the most accurate model available, and it remained the accepted theory for over 13 centuries, before it was finally replaced by the model of Copernicus.

Copernican Explanation Copernicus replaced the geocentric universe of Ptolemy with one that was centered on the Sun (heliocentric), with only the Moon orbiting the Earth. His model was still based on circular orbits (and therefore still required further refinement), but it was able to achieve superior precision than the Ptolemaic model without the need for epicycles or other complications.

The explanation for retrograde motion in this system arises from the fact that the planets further from the sun are moving more slowly in their orbits than those closer to the sun. The retrograde motion of Mars occurs when the Earth passes by the slower moving Mars, as shown in the following animation: Retrograde Motion in the Copernican (Heliocentric) System (This animated gif was obtained from Dr. Stephen J.

Daunt's Astronomy 161 web site at The University of Tennesee, Knoxville.) When combined with the refinements of Kepler (elliptical orbits with the sun at one focus, relationships between distance from sun and orbital speed - both within a single orbit and between orbits) this does, in fact, provide the correct explanation for the observed retrograde motion along with precise predictions of the positions of the planets. For additional discussion of retrograde motion and the Ptolemaic and Copernican models of the solar system, you may want to check out the following web sites: . The Apparent Motion of Planets on the Celestial Sphere . The Universe of Aristotle and Ptolemy .

The Copernican Model: A Sun-Centered Solar System . The Retrograde Motion of the Planets . Planetary Motions" The second part will be in the next day or two. 2.For your responsive post, try to use your own best understanding to assist a classmate with something she or he finds difficult.To receive full credit, you must also post two substantial (~1 paragraph) replies to other student posts.

You can fellow ask students further questions on the topic or about their post. You can also provide help if they did not fully answer the discussion questions.