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Profile Documents Logout
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Introducing Astronomy
Introducing Astronomy

... Betelgeuse (α Orionis) R.A.: 5 hours, 55’, ...
Old Sample Exam #2
Old Sample Exam #2

... _____ 3) How long can a star run on gravity without nuclear fusion? (in years) a) 1031 b) 1012 c) 1010 d) 107 e) 100 _____ 4) What element cannot be nuclear burned to release energy? a) oxygen b) iron c) hydrogen d) uranium e) helium _____ 5) Planetary nebulae are often shaped like a(n) a) hourglass ...
The Nine Planets
The Nine Planets

... Venus After the Sun and the Moon, Venus is the brightest object that we can see in the sky because it is so close to our planet Earth. Also, the atmosphere on Venus is very thick and the light it receives from the Sun is reflected to us. Venus’s atmosphere is made up from mainly carbon dioxide. Thi ...
Applications of Light to Astronomy
Applications of Light to Astronomy

... o Observing which wavelengths are missing after reflection tells you about the composition of the reflecting surface! o Observing which wavelengths are missing after passing through material (e.g. atmosphere of a planet or star) tells you about that material ƒ Most of the stuff in the universe is hy ...
WORD - UWL faculty websites
WORD - UWL faculty websites

... o Observing which wavelengths are missing after reflection tells you about the composition of the reflecting surface! o Observing which wavelengths are missing after passing through material (e.g. atmosphere of a planet or star) tells you about that material  Most of the stuff in the universe is hy ...
Word version with live links
Word version with live links

... science view eg Hardy and Bonestall – book are available for lone on these topics. Stars These have a life cycle from birth to death when they seem to either collapse in on themselves and then explode, or just explode. By all accounts, we are safe for a good while because our own sun is fairly insig ...
Standard 1 Information Sheet
Standard 1 Information Sheet

... which makes use of the Doppler effect. Distances to some nearby stars can be measured by parallax: if a star appears to move slightly with respect to more distant stars as Earth orbits from one side of the Sun to the other, then the angle through which the star appears to move and the diameter of Ea ...
Earth Dimensions
Earth Dimensions

... The Atmosphere is layered, or divided into four zones based on temperature. The lowest, the troposphere contains most of the gases that we need to survive and our weather. The other three layers are the Stratosphere, Mesosphere, and ...
An earthllke planet would have a rocky mantle surround
An earthllke planet would have a rocky mantle surround

... cautioned that lab experiments today suggest life might be based on molecular structures substantially different from systems used by llfe on Earth. What's more, if life Is possible in solvents other than liquid water. It might exist In a wider range of planetary environments. The second theme Is th ...
HR.MOON.doc
HR.MOON.doc

... The earth is like a big blue marble. The earth rotates and orbits around the sun. Our earth has an atmosphere,the mesesphere protects us from meteors. When the earth rotates it creates day and night. ...
The Stars
The Stars

...  There are more stars in the sky than anyone can easily count, but they are not scattered evenly, and they are not all the same in brightness or color. By the end of the 5th grade, students should know that  The patterns of stars in the sky stay the same, although they appear to move across the sk ...
The Solar System. The Inner Planets.
The Solar System. The Inner Planets.

... It has volcanic activity, but probably no tectonic activity. The Soviet spacecraft Venera 9 landed on Venus and send a panoramic view of its surface. The US Magellan spacecraft transmitted radio images. ...
Document
Document

... b-Poles experience several weeks of day and night ...
FORMATION OF THE SOLAR SYSTEM
FORMATION OF THE SOLAR SYSTEM

... of gas and dust  4 to 5 billion years ago  Fusion began in center ...
Observing the Solar System
Observing the Solar System

... Why do the planets stay in orbit? • INERTIA and GRAVITY • Inertia is a tendency of a moving object to continue in a straight line or a stationary object to remain in place. The more mass an object has, the more inertia it has. • The force of gravity attracts all objects towards each other. No one i ...
THE UNIVERSE Celestial Bodies - Joy Senior Secondary School
THE UNIVERSE Celestial Bodies - Joy Senior Secondary School

... A planet (from Ancient Greek (astēr planētēs), meaning "wandering star") is an astronomical object orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighboring region of planetesimals. ...
Astronomy vs. Astrology: Uptodate Zodiac Signs and Dates
Astronomy vs. Astrology: Uptodate Zodiac Signs and Dates

... Constellations of the Zodiac are NOT in accordance with astronomical observations. Moreover, the Sun is now seen to transit through 13 constellations, not 12, as generally believed. Ergo: Your horoscope is of little value; the dates are wrong and quite different from those determined by astronomers, ...
the solar system and the universe - Colegio Nuestra Señora del Prado
the solar system and the universe - Colegio Nuestra Señora del Prado

... a diameter of 3,476 km, which is about a quarter of the Earth’s diameter. It has no atmosphere, so the average surface temperature is about -18 ⁰C. The Moon has not water on its rocky surface and it is covered with craters, caused by the impact of asteroids. All the planets in the solar system have ...
Please jot down or ponder your answers. 1. What causes seasons
Please jot down or ponder your answers. 1. What causes seasons

... Using an arm’s length of register tape, each student will illustrate the relative distances between the orbits of the planets. 1. Write “Sun” on one end of the paper strip and “Pluto” on the other end. 2. Fold the tape in half; this is Uranus. Label the strip. 4. Fold Pluto to Uranus; this is Neptun ...
- MrKowalik.com
- MrKowalik.com

... Varying Distance of Planets from the Sun 23. What does the elliptical shape of planetary orbits cause? _____________________ ___________________________________________________________________ 24. When are we closest to the sun?________________________________________ 25. When are we farthest from t ...
ppt
ppt

... For those people with more background, continue to part II: Looking East ...
Looking out at the Night Sky What questions do you have?
Looking out at the Night Sky What questions do you have?

... For those people with more background, continue to part II: Looking East ...
Name
Name

... As the Earth rotates only part of the Earth’s surface faces the sun at a time. This rotation is what causes day and night. One complete rotation takes place every 24 hours (1 day). Each planet rotates, but not at the same speed. This means that each planet’s day lasts a different amount of time. The ...
For each statement or question, select the word or expression that
For each statement or question, select the word or expression that

... ____ 18. Which objects are listed in order of scale from smallest to largest? A. sun, red giant, Earth, galaxy B. red giant, sun, galaxy, Earth C. Earth, sun, red giant, galaxy D. galaxy, Earth, sun, red giant ____ 19. The Milky Way is an example of a(n) A. spiral galaxy B. elliptical galaxy C. sum ...
Sample Chapter
Sample Chapter

... of the solar system. It formed 5 billion years ago from a cloud of gas and dust. The sun’s diameter is 1,392,000 kilometres. It is much bigger than the Earth. ...
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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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