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Astro history notes 1
Astro history notes 1

... Earth’s orbiting of the Sun The nearest stars are much farther away than the Greeks thought. So the parallax angles of the star are so small, that you need a telescope to observe them. ...
Chapter 22: Origin of Modern Astronomy
Chapter 22: Origin of Modern Astronomy

... A modern version of an earthcentered system. ...
Word - UW-Madison Astronomy
Word - UW-Madison Astronomy

... Aristotle argued that the Earth did not go around the Sun because if it did we would observe the stars to show the parallax effect. Let’s explore this idea a bit. a) Look at Figure i) on the back page. If you were to walk from A to B, all the while looking at Tree C, briefly describe what you would ...
Review Unit 1 - Effingham County Schools
Review Unit 1 - Effingham County Schools

... every thing in the universe revolved around the Sun. ...
powerpoint jeopardy
powerpoint jeopardy

... • Who was the first to suggest the sun was at the center? • Who used his telescope to help prove the heliocentric model? ...
Nicolaus Copernicus Describes What Is Seen in
Nicolaus Copernicus Describes What Is Seen in

... impossible to find the correct explanation of what is seen in the heavens. . . Every observed change of place is caused by a motion of either the observed object or the observer or, of course, by an unequal displacement of each. For when things move with equal speed in the same direction, the motion ...
NIE10x301Sponsor Thank You (Page 1)
NIE10x301Sponsor Thank You (Page 1)

... astronomy, the tables of planetary data based on Ptolemy’s model were found to be quite inaccurate. Copernicus thought a simpler model with the Sun as the center would produce better results. This view had been presented by Aristarchus 400 years before Ptolemy, but Copernicus’ work, published just b ...
The Solar System - RHIG - Wayne State University
The Solar System - RHIG - Wayne State University

... Claudius Ptolemaeus (90 to 168 AD), or Ptolemy, created the first “standard model” of the cosmos, a model that lasted 1500 years. He developed a system describing the motion and placement of all the known major objects in our solar system. Following Aristotle, he placed the Earth at the center, unmo ...
Study guide for Space Unit Key
Study guide for Space Unit Key

... 21. Explain how a revolution is different from a rotation. A revolution requires two bodies, one orbits around the other. A rotation requires only one body which spins around its own axis. 22. What causes the seasons? The Earth’s tilt on its axis and the Earth’s orbit around the sun. 23. What causes ...
6._Motions_in_Solar_System_student
6._Motions_in_Solar_System_student

... the solar system. (even suggested star movement is due to Earth rotation!) ...
The Ancient Mystery of the Planets
The Ancient Mystery of the Planets

... the solar system. (even suggested star movement is due to Earth rotation!) ...
Light year - TeacherWeb
Light year - TeacherWeb

...  Light year – the distance light can travel in a year (9.5 trillion km or 5.88 trillion miles / year - that’s 12 “0”s!!!) Just for Interest:  Light travels about 300,000 km (186,000 miles) per second  The North Star is 431 light years from Earth  Our nearest star, Proxima Centauri, is 4.28 light ...
Chapter 10
Chapter 10

... each planet revolved around a point on its orbit, called an epicycle, to explain its motion through the heavens ...
Saraswati River - Ancient Greece
Saraswati River - Ancient Greece

... 1. sun, moon, Mercury, Mars, Venus, Jupiter and Saturn 2. 1000s of stars – of which only about 1000 were identifiable in groups – namely the 48 ancient constellations which were formalised by Ptolemy (c.AD100 – 178) 3. Occasional phenomena – e.g. eclipses, comets and shooting stars. All ancients (th ...
Adobe Acrobat - Ancient Greece
Adobe Acrobat - Ancient Greece

... 1. sun, moon, Mercury, Mars, Venus, Jupiter and Saturn 2. 1000s of stars – of which only about 1000 were identifiable in groups – namely the 48 ancient constellations which were formalised by Ptolemy (c.AD100 – 178) 3. Occasional phenomena – e.g. eclipses, comets and shooting stars. All ancients (th ...
February 6
February 6

... http://www.geographyalltheway.com/ks3_geography/maps_atlases/longitude_latitude.htm ...
Test 1 Overview - Physics and Astronomy
Test 1 Overview - Physics and Astronomy

... - Occam’s Razor: Simpler Theories are better -You can prove a theory WRONG but not RIGHT Prediction ...
History of astronomy
History of astronomy

... but one that results in specific predictions, which we can test and confirm or refute. It has become a commonly used word as a result of the success of Thomas Kuhn's 1962 book The Structure of Scientific Revolutions. Examples of scientific paradigms are: 1) the Earth is just one of a number of plane ...
The Night Sky
The Night Sky

... and does not move, geocentric model ...
Lecture notes -
Lecture notes -

... • First quarter Moon. Note where it is at this time of day • Look to south-southeast. Lots of stars • At 8 pm…look east. The planet Mars is in the constellation of Leo • 10:30 pm…look east. Bright object in constellation of Virgo. The planet Saturn (orbited by piece of U of I) • Back to Leo. The ast ...
22 Jan: The Sky Tonight and Overview of the Solar System
22 Jan: The Sky Tonight and Overview of the Solar System

... • First quarter Moon. Note where it is at this time of day • Look to south-southeast. Lots of stars • At 8 pm…look east. The planet Mars is in the constellation of Leo • 10:30 pm…look east. Bright object in constellation of Virgo. The planet Saturn (orbited by piece of U of I) • Back to Leo. The ast ...
Our Place in Space
Our Place in Space

... Group 1 Group 2 Group 3 Group 4 Group 5 Group 1: Have you ever looked up into the night sky and wondered what was out there? Group 2: Throughout time, astronomers have gazed to the heavens, hoping to find clues about our place in the universe. Group 3: Long ago people assumed that Earth was the cent ...
Unit8TheUniverse
Unit8TheUniverse

... A. 13-15 b.y.a. the Universe came into being and began to expand at an incredible rate (Inflation). B. Evidence for the Big Bang: The BBT is not designed to explain the origins of the universe only how it developed. 1). Expanding Universe 2). Background radiation that was predicted and later found. ...
science - TCDSB.org
science - TCDSB.org

... The Earth rotates once every 24 hours. Each time the Earth rotates we have one day and one night. When we are on the sun side of the earth, we have daylight. When we rotate away from the sun, we have night. ...
Astronomy Powerpoint
Astronomy Powerpoint

... Earth Mars Jupiter Saturn Uranus Neptune ...
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Geocentric model



In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.
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