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Atmosphere of Venus, Mars and Earth (PDF: 1.7MB)
Atmosphere of Venus, Mars and Earth (PDF: 1.7MB)

... artificial lights brighten the night sky and artificial lights brighten the night sky and  prevent star observation.   Under the sky glow  of artificial lights which affect long exposure of artificial lights which affect long‐exposure  photographing, it is very difficult to observe  dark stars.   Fr ...
five minute episode script
five minute episode script

... AND THE ATMOSPHERE IS HEAVY. THE AIR PRESSURE WOULD ACTUALLY SQUISH YOU FLAT. DEAN: AND THEN IF IT RAINS ON VENUS, WATCH OUT. IT DOESN'T RAIN WATER. IT RAINS SULFURIC ACID. SO YOU'D BE A ROASTED, SQUISHED, ACIDY, PILE OF GOOP ON VENUS. ----(STOP) ON MARS (GRAPHICS FROM 1624) JAMES: NOW WE'RE ON MARS ...
Sky, Celestial Sphere and Constellations
Sky, Celestial Sphere and Constellations

... Twinkling is not good for astronomy, for astronomical observations, a steady atmosphere with good “seeing” is needed. ...
Nine Planets and Counting
Nine Planets and Counting

... publishes a free booklet called Space Spin-offs that shows how space technology is used to improve life on Earth. Send for the booklet and share it with students. 8. Many students hear that Neptune and Pluto switch orbits. This is a misconception. Pluto’s orbit is elliptical and tilted which occasio ...
FantasticTrip - Cooper Church of Christ
FantasticTrip - Cooper Church of Christ

... Note that going downwards we could only go to the power of minus 16ª of 10 to reach the (known?) limits of matter... But upwards we went to the power of 23ª of 10 and stopped... But we could have continued our trip subject only to the limits to our imagination!!!! ... then? ... Who says that we are ...
Our Family on the Sky - Northern Stars Planetarium
Our Family on the Sky - Northern Stars Planetarium

... size much more impressive. Every student must then be responsible for not loosing her planet. This isn’t necessarily easy, as some planets, like Mercury and Pluto, are only about the size of a grain of sand! ...
chapter01lecturecdl
chapter01lecturecdl

... • Apparent groupings of stars into constellations seen on celestial sphere are not true, physical groupings. ...
May 2014
May 2014

... – and blue/red shift of the star's light), and transiting planets. The Kepler telescope used the dip-in-light transit method for finding planets. This method is very limited, as the planets' orbit have to be in line with our line of sight. (If the moon was perfectly in line with Earth's orbit with t ...
space - Net Start Class
space - Net Start Class

... Key Concept 1: A star is a large ball of gas that generates its own energy by fusing hydrogen atoms to make helium. It is held together by its own gravity. This process emits a tremendous amount of energy, and some of the energy is in the form of light. Stars come in a variety of sizes and compositi ...
The Earth-Moon-Sun System
The Earth-Moon-Sun System

... • Describe the movements of Earth known as rotation, revolution, and precession • Explain how the moon goes through phases • Explain how eclipses occur ...
Lecture 1 – Astronomy
Lecture 1 – Astronomy

... Netherlands that could bring far objects to appear closer. An optician had made the first telescope. Galileo bought some lenses from his local optician and build his own telescope. When he pointed the telescope towards the Sun in 1610, he noticed dark spots on the surface. He studied the spots over ...
Lecture 2 - The University Centre in Svalbard
Lecture 2 - The University Centre in Svalbard

... Netherlands that could bring far objects to appear closer. An optician had made the first telescope. Galileo bought some lenses from his local optician and build his own telescope. When he pointed the telescope towards the Sun in 1610, he noticed dark spots on the surface. He studied the spots over ...
Infinity Express-1
Infinity Express-1

... telescope, and therefore could not have proved the Heliocentric Solar System was correct. ...
MULTIPLE CHOICE QUESTIONS (50 pts
MULTIPLE CHOICE QUESTIONS (50 pts

... 22. If you know the value of (m – M) for a star, then you can determine A. the spectral class of the star. B. the star’s distance. C. the star’s diameter. D. the surface temperature of the star. E. the star’s mass. 23. In order to be classified as a planet in our Solar System, a body must orbit the ...
Introduction: The Night Sky
Introduction: The Night Sky

... their distances (if they are close) their masses (if they are binaries) ...
grade v and vi - Sacred Heart CMI Public School
grade v and vi - Sacred Heart CMI Public School

... and Neptune. These planets are much bigger than Earth, but very lightweight for their size. They are mostly made of hydrogen and helium. Until recently, the furthest known planet was an icy world called Pluto. However, Pluto is dwarfed by Earth’s Moon and many astronomers think it is too small to be ...
Chapter 27 Stars and Galaxies
Chapter 27 Stars and Galaxies

... and density build within the protostar’s center, causing temperature to rise ►Gas is so hot it becomes plasma (a fourth state of matter) ►Temperature continues to increase until it reaches 10,000,000ºC ...
understanding-the
understanding-the

... determine if the size of the universe is changing. Why do astronomers believe the size of the universe is changing? a. The red shift indicates that distant galaxies are moving away from each other. b. The red shift indicates that distant galaxies are moving towards each other. c. The blue shift indi ...
Training Manual - The Darwin Initiative
Training Manual - The Darwin Initiative

... the Stratosphere. Ozone (O3) in the earth's stratosphere is created by ultraviolet light striking oxygen molecules. This layer absorbs 93-99% of the sun's high frequency ultraviolet light, which is potentially damaging to life on earth. This occurs in the ozone layer, the region from about 10 to 50 ...
Chapter 28 Stars and Galaxies Reading Guide
Chapter 28 Stars and Galaxies Reading Guide

... absolute magnitude is +1.42, what does this tell you about the distance of Sirius from the Earth? ...
Jupiter
Jupiter

... 03º 12´ ...
File
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... away. There are only 11 stars (not including the sun) that are less than 10 light years away from earth. Most stars are much farther away than that. Many stars that we see at night are several thousand light years away. This means that from earth we can only see these stars as they existed thousands ...
The Stars Tonight
The Stars Tonight

... S G1: Science as a Human Endeavor (see the section about Galileo’s trial below) S G2: Nature of Science S G3: History of Science The TST program lends itself to engaging the audience using any and all of the three History and Nature of Science standards. The TST host can opt to describe observationa ...
Chapter 1 Section Misconception Truth Distances in the Universe
Chapter 1 Section Misconception Truth Distances in the Universe

... The Photosphere The Sun and stars have absorption spectra because the photosphere is cooler than  the core. All the light we see comes from the photosphere; the core is well hidden below hundreds of  thousands of kilometers of solar gas. The absorption lines and the continuum are both formed in the  ...
Document
Document

... as a framework for how that history made our existence possible. So first we need to know something of the structure and arrangement of this universe whose history we want to describe. Theme - Gaining perspective on how we connect to the universe: we are products of the whole universe, not just our ...
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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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