Can you describe the movement of the sun, stars, and planets according to the geocentric system?
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In a geocentric system, the Earth is at the center of the universe, and everything else goes around the Earth.  It was believed that the Earth was at the center up until the 1500s, when Gallileo and Copernicus used much more accurate measurements of planetary movements to prove it wrong.  Gallileo was even condemned and tortured by the Church for saying that the Sun was at the center of the solar system.
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Kepler's laws are simply empirical rules. What really predicts planetary motion is Newton's theory of gravity, which confirms Kepler's laws. It also explains most of the deviations from those laws as due to gravitational perturbation from other planets. \n\nEinstein's general relativity adds very little to Newton's calculations for our solar system. Newton calculated that the precession of Mercury's orbit should be 531 arc-seconds per century. General relativity correctly accounted for the full 574 arc-seconds. I'm not sure if you can work time dilation per se into that, but that's the most significant modification to Newton/Kepler by general relativity that I know of. (disclaimer - I am not a physicist)\n\nRe the equivalency of time: There is a time standard based on the center of the sun that is used for these calculations, to eliminate gravitational effects on the time base.
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In a word - yes\n\nAll the planets affect each other, although not always in major ways. The solar system can be considered as a two body system (the sun and Jupiter) with perturbations (all the other planets).\n\nFor an example of this, look at the precession of the perehelion of Mercury. General Relativity accounts for a tiny amount of that, but the rest is from the effects of the other bodies in the solar system.
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I could think of only two things that may (or may not) be that for which you are searching.\n\nThe first is simply a solar system mobile.  A simple string and crossbar mobile that children can put together.  Unfortunately a slight breeze could have them all going retrograde at once! Moons of the various planets are not generally included and the orbits are not elliptical.\n\nThe second is:\n"An orrery is a mechanical device that illustrates the relative positions and motions of the planets and moons in the solar system in heliocentric model. They are typically driven by a large clockwork mechanism with a globe representing the Sun at the center, and with a planet at the end of each of the arms." *\n\nI watched a program on Leonardo DaVinci and a section of this program had this tucked in the 3rd hour.  Coming back to find your question was interesting to say the least.   I hope this is what you need.
51021
No. Planets orbit stars.  The earth is a planet orbitting its star, the Sun.
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(1) They're all spherical in shape\n(2) All orbit around the Sun\n(3) All rotate on their axis
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The earth moves in many ways. For example:\n\n1. The surface of the earth exhibits earth tides, just like the surface of the oceans, because of the gradient of the gravity field the earth is in, due to the moon, sun and other celestial bodies (so there are usually about 2 high earth tides per day, and 2 low earth tides; they have an amplitude of a few feet). \n\n2. The ground moves due to earthquakes and volcanoes, etc.\n\n3. The ground moves due to the slow movement of tectonic plates\n\n4. The earth rotates on its axis (takes about 24 hours; this is slowing down because of the effect of the tides)\n\n5. The earth revolves around the sun (well the center of mass of the solar system actually, and it takes about 365.25 days to make one circuit)\n\n6. The pole of the earth precesses with a period of about 26,000 years (the direction the north pole points rotates)\n\n7. The axis of the earth bobs up and down while it rotates, called nutation (18.6 year period)\n\n8. The pole of the earth wobbles, called the Chandler Wobble (earth's pole moves in irregular circle of 3-15 m diameter with period of about 435 days) because of storms and other atmospheric and ocean redistributions of mass, and conservation of angular momentum. \n\n9. The earth's orbit around the center of mass of the solar system is elliptical, and the eccentricity of the ellipse varies with a period of about 100,000 years\n\n10. The axis tilt of the earth varies from 21.5 to 24.5 degrees with a period of about 41,000 years.\n\n11. The center of mass of the solar system varies a bit due to motion of the sun and the planets.\n\n12. The solar system as a whole moves in our galaxy about the center (a period of 225 million years, and moving at about 250 km/sec)\n\n13. The solar system bobs up and down in the limb of the Milky Way galaxy with a period of tens of millions of years\n\n14. Our galaxy is moving through space very rapidly (about 300 km/sec, but this depends on what you are measuring relative to; see references)
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Astronomers define a coordinate system on the sky that lets them identify the relative positions of stars, planets, the Sun and other celestial phenomena (the coordinates are called "right ascension" and "declination", but we don't need to worry about that here). Because of their great distance from the Earth, the positions of most stars are fixed on the grid. The positions of the planets and the Sun, however, are seen to "travel" through the coordinate grid in systematic (though sometimes complicated) patterns. The paths of the planets was carefully observed by Tycho Brahe in the late 1500s. Following Brahe's death in 1601, Johannes Kepler used the data to develop a set of laws that govern the way the planets move around the Sun (he proposed them in 1609). These laws, (creatively) called Kepler's Laws, still hold today.\n\nWith Kepler's laws in hand, one can easily interpret the motion of the Sun through the coordinate grid described above as the result of the tilt of the Earth by 23.5 degrees with respect to the plane in which the Earth orbits the Sun. Since Kepler was the one to correctly interpret the motion of the planets and the Sun through the sky, he is the one that I would attribute the title "Discoverer of the 23.5 degree tilt", in the early 1600s.
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Finally, the gravitational pull between the Earth and Sun causes the Earth to travel around, or "orbit", the Sun at a velocity of 29.8 km/sec. At the same time, the Earth also turns on its axis causing the daily cycle of day and night. This "rotational velocity" is approximately .47 km/sec. That means that at the same time we're hurdling through space at nearly 67,000 mph, we're also spinning around in circles at over 1000 mph! Whew! Almost makes you dizzy, doesn't it?
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There is only one solar system, and it is the one our planet is part of.\n\nThe solar system comprises the Earth's Sun and the retinue of celestial objects gravitationally bound to it. Traditionally, this is said to consist of the Sun, nine planets and their 158 currently known moons; however, a large number of other objects, including asteroids, meteoroids, planetoids, comets, and interplanetary dust, orbit the Sun as well. Astornomers are debating over the presence of a tenth planet.\n\nAlthough the term "solar system" is frequently applied to other star systems and the planetary systems which may comprise them, it should strictly refer to Earth's system specifically: the word "solar" is derived from the Sun's Latin name, Sol, and thus the term sometimes appears as Solar System. When talking about another stellar system or planetary system, including the stars and bodies associated with them through gravity, it is usual to shorten it to drop the term "stellar" and form names such as "the Alpha Centauri system" or "the 51 Pegasi system".
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Solar system  \n\nThe solar system comprises our Sun and the retinue of celestial objects gravitationally bound to it. Traditionally, this is said to consist of the Sun, nine planets and their 158 currently known moons; however, a large number of other objects, including asteroids, meteoroids, planetoids, comets, and interplanetary dust, orbit the Sun as well.
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The sun doesn't have to move in order for the planets to have a sunset or sunrise.  Always remember that the earth constantly rotates and takes 24 hours to make a full rotation. On one side of the earth there will be light versus the other side will be darkness.
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Newton's laws of motion together with his law of gravity give a relation among\n\n    * the period P of a planet's orbit.\n    * the distance a from the planet to the Sun.\n    * a constant G measured in laboratory experiments.\n    * the mass M of the Sun. \n\n(For our purposes, assume the orbits are circles. Also assume that the mass of a planet is tiny compared to the mass of the Sun.)\n\n\nUsing this relation with P and a for the Earth gives the mass of the Sun.\n\nM ~ 2 x 1030 kg.\n\nWe will use this relation later on to get the masses of other stars.\n\nIt can also be used to get the masses of galaxies!\n\nDavison E. Soper, Institute of Theoretical Science, University of Oregon, Eugene OR 97403 USA soper@bovine.uoregon.edu
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The First law of Kepler is: \nPlanets move along elliptical orbits with the Sun\nat a focus.\n\nSo, all i can say is that the sun is relatively stagnant in our immediate universe.\nThe earth rotates along an elliptic orbit around the sun.\nThe moon rotates along an elliptic orbit around the earth.\n\nWell, all "movements" are relative to some reference point.
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Earth orbits in a counterclock wise direction around the sun.\nIt takes approximately 365.25 days do orbit around the sun.\nThe gravitational forces between the sun and earth and the resulting centripetal and centrufugal forces makes the earth go around.
199932
The earth's rotation.
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I havent a clue what your are asking... are we talking about astronomy terms?  Elevation and declination?  Or are you asting about Lattitude and Longitude?