ASTR 1120H – Spring Semester 2010 Exam 1 – Answers The AU is
... model), then as a result of its motion parallax of the nearest stars should be observed. He didn't see parallax, so he concluded that the heliocentric model could not be correct. ...
... model), then as a result of its motion parallax of the nearest stars should be observed. He didn't see parallax, so he concluded that the heliocentric model could not be correct. ...
Core Theme 3: The Solar System
... through the main part of the Earth's shadow, there is not much to see, and if you didn't know that an eclipse was taking place you would not be aware of it. So we will have to wait for a decent lunar eclipse until the early morning of September 28, 2015. The next good lunar eclipses after that are o ...
... through the main part of the Earth's shadow, there is not much to see, and if you didn't know that an eclipse was taking place you would not be aware of it. So we will have to wait for a decent lunar eclipse until the early morning of September 28, 2015. The next good lunar eclipses after that are o ...
Integrative Studies 410 Our Place in the Universe
... – The year is the rotation period of the Earth around the Sun – The year is subdivided into months, the period of the Moon around the Earth – The weeks seven days are named after the seven bodies in the solar system known in ...
... – The year is the rotation period of the Earth around the Sun – The year is subdivided into months, the period of the Moon around the Earth – The weeks seven days are named after the seven bodies in the solar system known in ...
Gravitation Worksheet
... 4. Discuss the variation in ‘g’ with altitude and depth. 5. Derive expression for escape velocity. 6. State and prove Kepler’s second and third law of planetary motion 7. How much faster than its present rate should earth rotate about its axis so that the weight of a body at equator becomes zero? 8. ...
... 4. Discuss the variation in ‘g’ with altitude and depth. 5. Derive expression for escape velocity. 6. State and prove Kepler’s second and third law of planetary motion 7. How much faster than its present rate should earth rotate about its axis so that the weight of a body at equator becomes zero? 8. ...
Space Exam Review
... another object (orbit); this movement is not in a perfect circle, but in an elliptical shape Since the Sun in not directly in the centre of the ellipse, the Earth is actually closer to the Sun in December than it is in June!!! ...
... another object (orbit); this movement is not in a perfect circle, but in an elliptical shape Since the Sun in not directly in the centre of the ellipse, the Earth is actually closer to the Sun in December than it is in June!!! ...
the copernican revolution - University of Florida Astronomy
... Center of epicycle moves at a constant distance from the eccentric, but at a uniform angular rate from the equant. •! Ptolemy never claimed his model described reality. It was a mathematical representation to predict the positions of the planets. •! The model successfully predicted the observed moti ...
... Center of epicycle moves at a constant distance from the eccentric, but at a uniform angular rate from the equant. •! Ptolemy never claimed his model described reality. It was a mathematical representation to predict the positions of the planets. •! The model successfully predicted the observed moti ...
Gatesville Elementary School 2012-2013 Science Pacing Guide 1st
... components and patterns observed in the earth/moon/sun system. 3.E.1.1 Recognize that the earth is part of a system called the solar system that includes the sun (a star), planets, and many moons and the earth is the third planet from the sun in our solar system. 3.E.1.2 Recognize that changes in th ...
... components and patterns observed in the earth/moon/sun system. 3.E.1.1 Recognize that the earth is part of a system called the solar system that includes the sun (a star), planets, and many moons and the earth is the third planet from the sun in our solar system. 3.E.1.2 Recognize that changes in th ...
Explain. How is Copernicus`s description of the system of planets
... • People usually say that the sun rises in the east, moves across the sky, and sets in the west. Is this description literally correct? Explain. • How is Copernicus's description of the system of planets different from Ptolemy's description? ...
... • People usually say that the sun rises in the east, moves across the sky, and sets in the west. Is this description literally correct? Explain. • How is Copernicus's description of the system of planets different from Ptolemy's description? ...
Test#1
... What do we call the event when the Sun is located 23.5o north and south of the celestial equator. a) solstices, b) equinox, c) day of dawns, d) solar eclipses Which one of Kepler's laws explains what happens when a twilling ice skater brings their arms towards their center? a) the planets follow ell ...
... What do we call the event when the Sun is located 23.5o north and south of the celestial equator. a) solstices, b) equinox, c) day of dawns, d) solar eclipses Which one of Kepler's laws explains what happens when a twilling ice skater brings their arms towards their center? a) the planets follow ell ...
AST 105 HW #2 Solution
... objects traveled in perfect circles. Eudoxus added separate spheres for each planet, as well as for the Sun and the Moon. Ptolemy incorporated all of this, as well as other ideas, into his Ptolemaic model, published in ...
... objects traveled in perfect circles. Eudoxus added separate spheres for each planet, as well as for the Sun and the Moon. Ptolemy incorporated all of this, as well as other ideas, into his Ptolemaic model, published in ...
Monday Sept 14
... A planetary system is a star and all of the planets, moons, and other objects and materials that orbit that star. Until very recently, there was only one known planetary system Even though many People suspected that most stars had planets orbiting them, we had no scientific evidence to support th ...
... A planetary system is a star and all of the planets, moons, and other objects and materials that orbit that star. Until very recently, there was only one known planetary system Even though many People suspected that most stars had planets orbiting them, we had no scientific evidence to support th ...
Understanding Planetary Motion
... center of the system and that all bodies revolve about the Sun. ...
... center of the system and that all bodies revolve about the Sun. ...
ASTRONOMY 110G Review Questions for
... Which observation, invention, experiment, or discovery of Galileo proved that the Ptolemaic System had to be incorrect. Prior to this, what was the strongest observational indication favoring the Copernican view? The Ptolemaic view? Where on Earth are all stars visible at one time or another? Where ...
... Which observation, invention, experiment, or discovery of Galileo proved that the Ptolemaic System had to be incorrect. Prior to this, what was the strongest observational indication favoring the Copernican view? The Ptolemaic view? Where on Earth are all stars visible at one time or another? Where ...
Chapter 27 – The Planets and the Solar System
... c. Because of their Earth like appearance they are also known as terrestrial planets 2. Outer Planets – Jupiter, Saturn, Uranus, Neptune and Pluto a. 1st four are called Jovian – or Jupiter like b. very large gaseous planets with no rocky crust c. low density due to size d. have ring systems e. Plut ...
... c. Because of their Earth like appearance they are also known as terrestrial planets 2. Outer Planets – Jupiter, Saturn, Uranus, Neptune and Pluto a. 1st four are called Jovian – or Jupiter like b. very large gaseous planets with no rocky crust c. low density due to size d. have ring systems e. Plut ...
Extra-Solar Planets continued
... One of them orbits very close to the star named 55 Cancri, which is about the same size as our sun and located 41 light-years away in the constellation Cancer. The new planet was located by University of Texas-Austin astronomers using the Hobby-Eberly telescope in the Davis Mountains southeast of ...
... One of them orbits very close to the star named 55 Cancri, which is about the same size as our sun and located 41 light-years away in the constellation Cancer. The new planet was located by University of Texas-Austin astronomers using the Hobby-Eberly telescope in the Davis Mountains southeast of ...
Homework Assignment 1 — Solutions
... passes the Earth on the inside. Therefore, f = f⊕ + 1, leading to ∆t ∆t ...
... passes the Earth on the inside. Therefore, f = f⊕ + 1, leading to ∆t ∆t ...
PH109 Exploring the Universe
... d) Jupiter was not perfect but had moving clouds of gas. 2) When Galileo viewed the Moon, what discovery helped change our view of the solar system? a) Because the Moon rises in the East and sets in the West, its orbit must be opposite that of the planets. b) The Moon went through phases like Jupite ...
... d) Jupiter was not perfect but had moving clouds of gas. 2) When Galileo viewed the Moon, what discovery helped change our view of the solar system? a) Because the Moon rises in the East and sets in the West, its orbit must be opposite that of the planets. b) The Moon went through phases like Jupite ...
Slide 1
... covered in rocks and impact craters, and the solar system's biggest volcano, Olympus Mons. •Weak or nonexistent magnetic field •A year on Mars is 687 Earth days. •A day on Mars is 24 hours and 37 minutes ...
... covered in rocks and impact craters, and the solar system's biggest volcano, Olympus Mons. •Weak or nonexistent magnetic field •A year on Mars is 687 Earth days. •A day on Mars is 24 hours and 37 minutes ...
mid term exam crossword
... 61. located between mars and jupiter 63. the sun is a ____, a ___ forms when fusion starts in a nebula 65. the sun's color is ____ 66. steepness of the landscape 68. movement that is actually occuring 69. gases that surround the earth, reason that the Earth has relatively few impact craters, Mercury ...
... 61. located between mars and jupiter 63. the sun is a ____, a ___ forms when fusion starts in a nebula 65. the sun's color is ____ 66. steepness of the landscape 68. movement that is actually occuring 69. gases that surround the earth, reason that the Earth has relatively few impact craters, Mercury ...
Space Science Chapter 1 Study Guide
... 16. What is the visible light spectrum? The range of colors of light that occurs when white light passes through a prism 17. How are the objects in our universe arranged? Use the terms universe, planet, galaxy, star, solar system. (Write in complete sentences for questions 17 & 18) Objects in the un ...
... 16. What is the visible light spectrum? The range of colors of light that occurs when white light passes through a prism 17. How are the objects in our universe arranged? Use the terms universe, planet, galaxy, star, solar system. (Write in complete sentences for questions 17 & 18) Objects in the un ...
Notes on Sun-Earth-Moon (pg. 119)
... 5. Explain how a lunar eclipse differs from a solar eclipse. During a lunar eclipse, Earth is directly between the Sun and the Moon, causing the Moon to pass through Earth’s shadow. During a solar eclipse, the Moon is directly between the Sun and Earth, casting a shadow upon Earth. 6. How does the ...
... 5. Explain how a lunar eclipse differs from a solar eclipse. During a lunar eclipse, Earth is directly between the Sun and the Moon, causing the Moon to pass through Earth’s shadow. During a solar eclipse, the Moon is directly between the Sun and Earth, casting a shadow upon Earth. 6. How does the ...
The Solar System - University of Sioux Falls
... negative 67 degrees Fahrenheit There are permanent ice caps at both poles on Mars People have landed on Mars to explore its surface ...
... negative 67 degrees Fahrenheit There are permanent ice caps at both poles on Mars People have landed on Mars to explore its surface ...
History of astronomy
... Why were there no telescopes prior to 1600? Consider the following passage, from the Opus Majus of Roger Bacon (1267): “Greater things than these may be performed by refracted vision. For it is is easy to understand by the canons above mentioned that the greatest things may appear exceeding small, ...
... Why were there no telescopes prior to 1600? Consider the following passage, from the Opus Majus of Roger Bacon (1267): “Greater things than these may be performed by refracted vision. For it is is easy to understand by the canons above mentioned that the greatest things may appear exceeding small, ...
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.