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Slide 1
Slide 1

... Leaving the Solar System, our next stop will be at the Alpha Centauri system. Source: Wikipedia ...
Answer to question 1 - Northwestern University
Answer to question 1 - Northwestern University

... Appropriately the proununciation is also very close to Hipparchus, the name of a Greek astronomer who lived from 190 to 120 BCE. By measuring the position of the Moon against the stars, Hipparchus was able to determine the Moon's parallax and thus its distance from the Earth. He also made the first ...
The Moon
The Moon

...  However, in 2006, the International Astronomical ...
BBA IInd SEMESTER EXAMINATION 2008-09
BBA IInd SEMESTER EXAMINATION 2008-09

... Note: Attempt six questions in all. Q. No. 1 is compulsory. ...
The Solar System Information Pack
The Solar System Information Pack

... sun (and the new planet that has been found!).  The relative sizes of the planets and their distance from the sun.  The sun is a star at the centre of our solar system.  The sun, earth and moon are approximately spherical bodies.  That some of the planets have moons and the number of moons for e ...
The solution set
The solution set

... General grading rules: One point off per question (e.g., 1a or 2c) for egregiously ignoring the admonition to set the context of your solution. Thus take the point off if relevant symbols aren’t defined, if important steps of explanation are missing, etc. If the answer is written down without *any* ...
Lecture Summary (11/22)
Lecture Summary (11/22)

... If the iron core develops, the star is destined to become a supernova. Iron does not fuse and yield energy, it takes energy away in the core. The inner regions of the star catastrophically collapse beyond the white dwarf size to a size of about 20 km across. The electrons and protons are forced toge ...
The Far Future Sun and the Ultimate Fates of
The Far Future Sun and the Ultimate Fates of

... At the crash: RSun = 180 Rnow (varying from 173 to 188 with P = 313 days) LSun = 2790 Lnow At the end: LSun = 3950 is the maximum achieved. ...
Earth-sized planet found just outside solar system
Earth-sized planet found just outside solar system

... similar to the Sun orbiting close to each other, designated Alpha Centauri A and B, and a more distant and faint red component known as Proxima Centauri. Since the nineteenth century astronomers have speculated about planets orbiting these bodies, the closest possible abodes for life beyond the Sola ...
ppt-file 2.4 MB
ppt-file 2.4 MB

... mathematical model to locate the 'habitable zone' of 47 UMa, a Sun-like star some 45 light years away. The pair devised equations coupling stellar age and luminosity, distance from the star, and planetary climate, to determine the chance of habitable planets existing near 47 UMa. They also calculate ...
Ch.1, Sec.3 - Mapping the Stars
Ch.1, Sec.3 - Mapping the Stars

... - the use of an astrolabe helps show the location of a star or planet ...
Stars
Stars

... luminosity is 1, Sirius is 23, Adhara is 5,000. Luminosity is measured in ergs per second. ...
Normal Stars - Chandra X
Normal Stars - Chandra X

... flares. Flares can occur on the Sun at any time, but their frequency tends to rise from a peak of five to ten a day and fall to less than one per day in a cycle of about eleven years. Solar flares can shower the Earth in high energy particles. A strong one can disrupt radio communications and produc ...
The Sun
The Sun

... unexpected discovery and formed Kepler’s Laws! What was this? ...
Stars, Constellations, and the Celestial Sphere
Stars, Constellations, and the Celestial Sphere

... The horizon for an observer at O is the intersection of a plane tangent to Earth at O with the celestial sphere. Everything that the observer can see is above the tangent plane (represented by the green line in the figure). The angle between the celestial equator (yellow line) and the horizon (gree ...
problems  - Villanova University
problems - Villanova University

... 79. Using the Titius-Bode rule, determine the distance of the asteroid belt from the Sun. If the asteroid belt were a planet, what would its orbital period around the Sun be? 80. Imagine an Earth-size extra-solar planet that orbits a star similar to the Sun at 1.4 au. Can such a planet be habitable? ...
Boonesborough Days - Tri
Boonesborough Days - Tri

... Mars, with one or more missions launching every twenty-six months. We are directing more of our attention to the moons of the giant planets as we see intriguing signs of both water and dynamism on their surfaces, knowing that on Earth, where there is water and energy there is also life. We are progr ...
Search for Life in the Universe
Search for Life in the Universe

... • Life just under the surface: e.g., Mars with possible life a few hundred meters under the surface • Life deep underground: e.g., Europa, Ganymede, Callisto • Liquid other than water: e.g., Titan • Tidal heating: Energy source is a planet, not the star  any distance from star • Brown dwarfs – Mass ...
lesson 5-8 quiz.show.pps
lesson 5-8 quiz.show.pps

... It happens in late September. It occurs one time a year. It is the beginning of fall in the southern hemisphere. ...
Unit 8 Chapter 29
Unit 8 Chapter 29

... 1,380,000km (~100 earth’s). It is 94,000,000 miles from the earth. It takes 8 minutes 20 seconds for sunlight to reach the earth. It would take 195 years at 55 mph to drive to the sun. The sun’s rotation period at the equator is approximately 25.3 earth days and 33 earth days at poles. This gives it ...
Astro 2 - Red Hook Central School District
Astro 2 - Red Hook Central School District

... • Supergiant – very heavy star fuses elements beyond carbon. • White dwarf – solar mass but planetary size no more fusion. ...
Solar System Power Point
Solar System Power Point

... closely spaced together • They are known as the terrestrial planets because their surfaces are dense and rocky ...
Slide 1
Slide 1

... We should be surrounded by evidence of these civilizations, but we have no idea yet how to find them. This is interesting: if they are somewhere, then then, the should have arisen long before we came to the scene. We know the universe is about 14 billion years old, but the Earth is “only” about 4.5 ...
ITB - In the Beginning
ITB - In the Beginning

... the fainter it is. ...
SOLAR eclipse LUNAR eclipse
SOLAR eclipse LUNAR eclipse

... * In a sidereal month, the moon makes a 360˚ orbit around Earth (with respect to a distant star). This takes 27.3 days. In a synodic month, the moon makes a 360˚ orbit of Earth, but continues on in its path to end up in the same orientation with the Sun as when it started. Remember, during the month ...
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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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