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Chapter 1
Chapter 1

... Revolution – to go around in the orbit. Rotation – to spin around an axis. The Moon revolves once in about 29 days. The Moon rotates once in exactly the same time. We see only one side of the Moon. The side we don’t see is called the “dark side”. ...
history of astronomyppt
history of astronomyppt

... geocentric model in which each celestial object was mounted on its own revolving transparent sphere with its own separate tilt  The faster an object moved in the sky, the smaller was its corresponding sphere  This simple geocentric model could not explain retrograde motion without appealing to clu ...
PDF only
PDF only

... but its spectral range could nonetheless support photosynthesis on a planet’s surface. M dwarf stars are smaller and more parsimonious still and can steadily shine for hundreds of billions of years, but they shine so dimly that their habitable zones are very close-in, potentially subjecting planets ...
Space_Review_Coelho
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... Orbital and Linear; Orbital shows that the sun is in the center of our solar system and linear does not; Linear is easier to draw; Orbital shows the revolving/ path of the planets ...
Test and answer key  - Solar Physics and Space Weather
Test and answer key - Solar Physics and Space Weather

... A precession of Earth's axis. B motion of the Moon across the sky. C revolution of Earth around the Sun. D *rotation of Earth on its axis. 13. When we watch the nighttime sky, we find that A the stars and constellations remain fixed in our sky, not rising or setting in a time as short as one night b ...
Careful measurements reveal that the earth has a slight difference in
Careful measurements reveal that the earth has a slight difference in

... they appear to “sink” over the horizon Curved Earth ...
Extreme Tidal Waves in Binary Star Systems
Extreme Tidal Waves in Binary Star Systems

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Combining Practices with Core Ideas in the NGSS
Combining Practices with Core Ideas in the NGSS

Stars and The Universe
Stars and The Universe

... Introduction to the study of stars, galaxies, and cosmology. Includes the nature of light and matter, telescopes, spectroscopy, stellar formation and evolution, galaxies, quasars, and cosmology. Designed for non-majors in mathematics or a physical science. A companion science lab, Astronomy 30, is a ...
Venus - Mr. Nussbaum
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... Venus is sometimes called Earth’s sister planet, though its similarities with Earth are limited apart from size and relative condition of its surface. It is easily observed with the naked eye and is sometimes called the “evening star” or “morning star.” Venus is covered by thick, noxious clouds of s ...
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Size of Sun and Size of Planets
Size of Sun and Size of Planets

... Name ________________________ ...
Starry Night Lab
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Geoview by R. Buckminster Fuller
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... Shining brightly at the miniature Earth’s north pole center and looking outwardly through the dome’s transparent shell. Any stars seen at any location on any of the continents or oceans are at that moment exactly in zenith over those very geographical points on the real Earth—which can be verified i ...
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... At approximately which position is Earth’s solar system located? (1) A (3) C (2) B (4) D __2__7. The Milky Way galaxy is best described as (1)a constellation visible to everyone on Earth (2)a spiral-shaped formation composed of billions of stars (3)a region in space between the orbits of Mars and Ju ...
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... professional teams announced their own observations of the same transit. We are very encouraged that our results compare so favourably with those obtained from bigger European facilities, and that our results constrain tightly the nature of HD 80606b and its unusual orbit." "For example, spectroscop ...
PPT slide - Solar Physics Group
PPT slide - Solar Physics Group

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Venus - Mr. Nussbaum
Venus - Mr. Nussbaum

... and relative condition of its surface. It is easily observed with the naked eye and is sometimes called the “evening star” or “morning star.” Venus is covered by thick, noxious clouds of sulfuric acid that obscure its surface. The thick layers of cloud create an extreme insulating effect (like the g ...
Stars, Galaxies and the Universe FORM A
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... 25. Which is NOT thought to be a location of dark matter in the universe? (a) in the halo of our Galaxy (b) in the outer regions of our Galaxy (c) in the core of the Sun and most stars (d) in the halo and outer regions of other galaxies (e) in the centers of galaxy clusters 26. What is the source o ...
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... B. a Doppler shift D. convection 2. The hottest layer of the sun, the _______, is most visible to the naked eye during a solar eclipse. A. photosphere B. corona C. ionosphere D. magnetosphere 3. We feel sure that the sun is now fueled by nuclear energy rather than by energy left over from its gravit ...
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... But early scientists thought that the Sun and other planets orbited Earth. In about 260 BCE, a Greek astronomer and mathematician named Aristarchus may have been the first to argue that Earth orbits the Sun. Most people ignored his ideas for a very long time because other well-known scientists did n ...
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... SATURN - Roman god of the harvest. Saturn was only visible in the northern hemisphere during the growing seasons of summer. ...
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... how the brightness of the background source changes with time. If the lensing star has a planet which also passes exactly between us and the background ...
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"It`s increasingly seeming that the solar system is

... orbit at large angles compared to the rotational axis of its star. A few systems even orbit two stars at once, getting Star Wars fans excited about a real-life Tatooine planet with two suns. ...
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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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