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Study Guide for 1ST Astronomy Exam
Study Guide for 1ST Astronomy Exam

... o Location of the planets and the observational basis for that ordering. (See Figure 11.10)  Describe the cause of retrograde motion in our modern Copernican Model.  Describe why inferior planets demonstrate a maximum elongation in their motion.  Describe how Copernicus determined the relative d ...
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... bright then fades in a few months or years) and five comets that were beyond the Moon’s orbit. His findings did not agree with either Ptolemy or Copernicus so Brahe developed his own theory called the Tychonic system. This system suggests that the Sun and Moon revolve around the Earth and all other ...
Heliocentric Model by Copernicus
Heliocentric Model by Copernicus

... What paths do the planets follow as they move around the Sun? Johannes Kepler (1571-1630) What did Galileo (1564-1642) see in his telescope that confirmed that the planets orbit the Sun? What fundamental laws of nature explain the motions of objects on Earth as well as the motions of the planets? Wh ...
WEST ORANGE PUBLIC SCHOOLS
WEST ORANGE PUBLIC SCHOOLS

... (or orbits) around the Sun. One revolution takes about 365 days. A period of revolution is the time it takes a moon or planet to make one complete orbit. 2. What causes the apparent movement of the sun across the sky during the day on Earth? ...
P101.EXAM1.931.v2 - KFUPM Faculty List
P101.EXAM1.931.v2 - KFUPM Faculty List

... 19) Astronomers have found planets around a star called Upsilon Andromedae, which is at a distance of 44 light years from our solar system. Assume a spacecraft that can travel with a speed of 5  104 km/hr (a typical speed of a present day spacecraft), how long would it take to reach that new planet ...
Earth and Space - Sun, Moon and Stars
Earth and Space - Sun, Moon and Stars

... communicate information from careful observations and simple investigation through a variety of methods. ...
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... Sidereal and Solar Time  We measure time according to the position of the Sun in the sky. o Our day is the time from Noon to Noon and is exactly 24 hours long.  This time period is called a ``Solar Day''.  It takes the Earth 23 hours 56 minutes and 4 seconds to complete a rotation. o This time pe ...
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... (a) Explain how such a curious unit of measure came to be defined. Why is it called parsec? (b) What is the distance to the nearest stars and how was this distance measured? 4. Describe qualitatively what is the precession of perihelion. (a) What are the dominant cause of this precession? (b) What i ...
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... 37: <= 12hrs 14: 24 hrs 5: 10 hrs 4: 6 hrs 3: 14-16 hrs 2: “A night” 2: Answer had nothing to do with question 1: 5hr, 9.5hr, 8hr, 72 hrs,6 min, “Couple of days”, No Answer ...
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... (Ptolemy of ancient Greece had explained that the universe was a closed system revolving around the Earth, and the Catholic church concurred). Hesitant to publish his work for fear of being charged with heresy, Copernicus summarized it in 1530 and circulated it among Europe's scholars, where it was ...
university of british columbia: astronomy 310: final
university of british columbia: astronomy 310: final

... (a) Sketch the interior structure of the Earth. Indicate briefly how it was determined. (b) [For those who love calculations.] (i) Imagine that a new comet has been discovered and that studies of its motion indicate that it orbits the Sun with a period of 1,000 years. What is the comet’s average dis ...
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... the rest of the objects in the solar system put together. The next largest object is the planet Jupiter. ...
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... • Most ancient Greeks held a geocentric (Earth-centered) view of the universe • Seven heavenly bodies (planetai) • Changed position in sky • The seven wanderers included the • Sun • Moon • Mercury through Saturn (excluding Earth) ...
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... Use an appendix to find the length of a light year. White this length with regular numerals. 9.46 x 1015m. 9,460,000,000,000,000m ...
`Does the Universe Exist for Man Alone? According to Dr. Wallace
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... could not possibly arise. Many of the brightest stars are much larger than our sun, but there are probably ten times as many that, being much smaller, are unsuited to yield adequate light and heat for a sufficient time, and with sufficient uniformity for life-development on planets. In given regions ...
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... A star is a hot ball of glowing gases. ...
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... periodically, during which time they appear to move “backwards” in the sky. This caused a lot of headaches for those trying to explain the apparent motion of the planets. The “S” shape is due to the fact that the orbital planes aren’t quite aligned. ...
CelestialSphere02
CelestialSphere02

... periodically, during which time they appear to move “backwards” in the sky. This caused a lot of headaches for those trying to explain the apparent motion of the planets. The “S” shape is due to the fact that the orbital planes aren’t quite aligned. ...
Powerpoint - BU Imaging Science
Powerpoint - BU Imaging Science

... • He also used a Sun-centred model to relate the known periods of the planets to their relative distances from the Sun, something not possible with the Ptolemy model • But how could you test these predicted distances? • Copernicus proposed that the planets go in circles-upon-circles around the Sun. ...
Sun, Moon and Stars - Mona Shores Public Schools
Sun, Moon and Stars - Mona Shores Public Schools

... 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. ...
Chapter 4 Gravitation and the Waltz of the Planets
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... 2. Why did Copernicus think that the Earth and the other planets revolved around the Sun? 3. What did Galileo see in his telescope that confirmed that planets orbit the Sun? 4. How did Tycho Brahe attempt to test the ideas of Copernicus? 5. What paths do the planets follow as they move around the Su ...
The Earth in Orbit - School
The Earth in Orbit - School

... demonstrate an understanding that one astronomical unit (AU) is the mean distance between the Earth and Sun. recall that planets move in elliptical orbits, slightly inclined to the ecliptic ...
astronomy ch 2 edit 1 - Fort Thomas Independent Schools
astronomy ch 2 edit 1 - Fort Thomas Independent Schools

... clues suggesting that Earth is not the center of the universe the scientific revolution that dethroned Earth from its location at the center of the universe Copernicus’s argument that the planets orbit the Sun why the direction of motion of the planets on the celestial sphere sometimes appears to ch ...
astronomy history time machine
astronomy history time machine

... clues suggesting that Earth is not the center of the universe the scientific revolution that dethroned Earth from its location at the center of the universe Copernicus’s argument that the planets orbit the Sun why the direction of motion of the planets on the celestial sphere sometimes appears to ch ...
The REAL OCCULT - Montgomery College
The REAL OCCULT - Montgomery College

... PRECESSION CYCLE: originally motion of the first day of a season around the ecliptic, now cycle of the rotation axis (day and night axis) about the year axis (this angle is around 23 ½ degrees now and takes around 26,000 years) GALACTIC YEAR: revolution of solar system about the Galactic center in a ...
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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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