 
									
								
									Origins of Earth
									
... Our Very Own Island Universe Milky Way Galaxy Milky Way Galaxy is 100 million light in diameter  Our galaxy contains roughly 400 billion stars  Sun is a very typical star located in one of the arms of the Milky Way Galaxy  Other planetary systems have been found in our galaxy ...
                        	... Our Very Own Island Universe Milky Way Galaxy Milky Way Galaxy is 100 million light in diameter  Our galaxy contains roughly 400 billion stars  Sun is a very typical star located in one of the arms of the Milky Way Galaxy  Other planetary systems have been found in our galaxy ...
									Origin of Ocean
									
... Our Very Own Island Universe Milky Way Galaxy Milky Way Galaxy is 100 million light in diameter  Our galaxy contains roughly 400 billion stars  Sun is a very typical star located in one of the arms of the Milky Way Galaxy  Other planetary systems have been found in our galaxy ...
                        	... Our Very Own Island Universe Milky Way Galaxy Milky Way Galaxy is 100 million light in diameter  Our galaxy contains roughly 400 billion stars  Sun is a very typical star located in one of the arms of the Milky Way Galaxy  Other planetary systems have been found in our galaxy ...
									Volume 20 Number 10 September 2012
									
... same as the spectacular Perseids shower which peaks in mid-August and is one of the year's highlights. They both appear to radiate from the same constellation but are not related - they were formed by different comets. September has five minor showers with three or less per hour. ------------------- ...
                        	... same as the spectacular Perseids shower which peaks in mid-August and is one of the year's highlights. They both appear to radiate from the same constellation but are not related - they were formed by different comets. September has five minor showers with three or less per hour. ------------------- ...
									Convolution - UW
									
... The convolution of two functions is an important concept in a number of areas of pure and applied mathematics such as Fourier Analysis, Differential Equations, Approximation Theory, and Image Processing. Nevertheless convolutions often seem unintuitive and difficult to grasp for beginners. This proj ...
                        	... The convolution of two functions is an important concept in a number of areas of pure and applied mathematics such as Fourier Analysis, Differential Equations, Approximation Theory, and Image Processing. Nevertheless convolutions often seem unintuitive and difficult to grasp for beginners. This proj ...
									PPT - Mr.E Science
									
... universe began 15 to 20 billion years ago. Scientist have viewed thousands of galaxies and can measure the fact that all galaxies are moving away from each other. If you could run the film “backwards”, it would appear that all of the galaxies come together at a single incredibly dense point. Scienti ...
                        	... universe began 15 to 20 billion years ago. Scientist have viewed thousands of galaxies and can measure the fact that all galaxies are moving away from each other. If you could run the film “backwards”, it would appear that all of the galaxies come together at a single incredibly dense point. Scienti ...
									The Solar System: Cosmic encounter with Pluto
									
... The Voyagers successfully completed their mission making discoveries such as the active volcanoes on Jupiter's moon, Io, and learning details about Saturn's rings. They had only been made to last five years but were still both going strong, so NASA extended their mission. Voyager 2 went on to take a ...
                        	... The Voyagers successfully completed their mission making discoveries such as the active volcanoes on Jupiter's moon, Io, and learning details about Saturn's rings. They had only been made to last five years but were still both going strong, so NASA extended their mission. Voyager 2 went on to take a ...
									Gravity
									
... the sun to the Earth. Which of the following best describes the gravitational influence of Vega on Earth? 1. It is roughly equal to that of the sun. 2. Its influence is greater than that of the sun. 3. Its influence is small because of its distance. 4. It influences the magnitude of Earth’s mass. ...
                        	... the sun to the Earth. Which of the following best describes the gravitational influence of Vega on Earth? 1. It is roughly equal to that of the sun. 2. Its influence is greater than that of the sun. 3. Its influence is small because of its distance. 4. It influences the magnitude of Earth’s mass. ...
									Astronomical Ideas Fall 2012 HW 2 solutions 1. a. Compare the
									
... This could be a result of true planetary demographics (planets tend to be closer than the Sun than the Earth is) or a result of observational bias. We are biased towards finding planets nearby their parent stars in transit searches, because planets with smaller orbital radii have shorter periods. We ...
                        	... This could be a result of true planetary demographics (planets tend to be closer than the Sun than the Earth is) or a result of observational bias. We are biased towards finding planets nearby their parent stars in transit searches, because planets with smaller orbital radii have shorter periods. We ...
									Kepler`s Law - New Mexico Tech
									
... evolution, during this time, nuclear fusion reactions in its core fuse hydrogen into helium. • It will spend approx. 10 billion years as a main ...
                        	... evolution, during this time, nuclear fusion reactions in its core fuse hydrogen into helium. • It will spend approx. 10 billion years as a main ...
									Solar System from Web
									
... evolution, during this time, nuclear fusion reactions in its core fuse hydrogen into helium. • It will spend approx. 10 billion years as a main ...
                        	... evolution, during this time, nuclear fusion reactions in its core fuse hydrogen into helium. • It will spend approx. 10 billion years as a main ...
									Tuesday, October 28th "The Formation and Evolution of Galaxies"
									
... of the Sun's shape resulting from gravitational forces and motions alone," says Hudson. "The corrected oblateness of the non-magnetic Sun is 8.01 +- 0.14 milli-arcseconds, near the value expected from simple rotation." "These results have far ranging implications for solar physics and theories of gr ...
                        	... of the Sun's shape resulting from gravitational forces and motions alone," says Hudson. "The corrected oblateness of the non-magnetic Sun is 8.01 +- 0.14 milli-arcseconds, near the value expected from simple rotation." "These results have far ranging implications for solar physics and theories of gr ...
									The Earth - for physicists - University of California, Riverside
									
... Back to the Hadean. As befits its name, this was a time when the Earth was hellishly hot. It began with an event that formed the Moon around 4.53 billion years ago. What made the Moon? The most popular current explanation is the “giant-impact theory” – sometimes called the “big splat” theory. The id ...
                        	... Back to the Hadean. As befits its name, this was a time when the Earth was hellishly hot. It began with an event that formed the Moon around 4.53 billion years ago. What made the Moon? The most popular current explanation is the “giant-impact theory” – sometimes called the “big splat” theory. The id ...
									The Ever Expanding Universe: Part II
									
... measurements came from Edmond Halley, England’s 18th century Royal Astronomer, who urged the next generation of astronomers to measure the upcoming transits of Venus (he would die before these events would occur) in order to get some of the best possible parallax data on the closest and easiest to m ...
                        	... measurements came from Edmond Halley, England’s 18th century Royal Astronomer, who urged the next generation of astronomers to measure the upcoming transits of Venus (he would die before these events would occur) in order to get some of the best possible parallax data on the closest and easiest to m ...
									Kaler`s MEASURING THE SKY
									
... plus 12 hours (the 12 hours added so that the "day" starts at midnight). Because of the eccentricity of the Earth's orbit and the obliquity of the ecliptic, apparent solar time does not keep a constant pace. Corrections for their effects lead to constant mean solar time, which can differ from appare ...
                        	... plus 12 hours (the 12 hours added so that the "day" starts at midnight). Because of the eccentricity of the Earth's orbit and the obliquity of the ecliptic, apparent solar time does not keep a constant pace. Corrections for their effects lead to constant mean solar time, which can differ from appare ...
									Ch9CTa
									
... Kepler's second law, the planet moves faster (has higher KE) when it is nearer the Sun, so KE>0. ...
                        	... Kepler's second law, the planet moves faster (has higher KE) when it is nearer the Sun, so KE>0. ...
									6 Scale Model of the Solar System
									
... where we need a telescope to see their tiny disks). Let’s see what the Sun looks like from the other planets! Ask each of the “planets” whether they can tell that the Sun is a round object from their “orbit”. What were their answers? List your results here: (5 points): ...
                        	... where we need a telescope to see their tiny disks). Let’s see what the Sun looks like from the other planets! Ask each of the “planets” whether they can tell that the Sun is a round object from their “orbit”. What were their answers? List your results here: (5 points): ...
									6 Scale Model of the Solar System
									
... where we need a telescope to see their tiny disks). Let’s see what the Sun looks like from the other planets! Ask each of the “planets” whether they can tell that the Sun is a round object from their “orbit”. What were their answers? List your results here: (5 points): ...
                        	... where we need a telescope to see their tiny disks). Let’s see what the Sun looks like from the other planets! Ask each of the “planets” whether they can tell that the Sun is a round object from their “orbit”. What were their answers? List your results here: (5 points): ...
									Kepler`s Second Law
									
... Click ‘Start Sweeping’ when the planet is in a different part of its orbit around the Sun The areas displayed in colour are equal, which is what is stated in Kepler’s 2nd Law. As the planet gets closer to the Sun in its orbit, it will be moving faster due to the increased effects of gravity. In a gi ...
                        	... Click ‘Start Sweeping’ when the planet is in a different part of its orbit around the Sun The areas displayed in colour are equal, which is what is stated in Kepler’s 2nd Law. As the planet gets closer to the Sun in its orbit, it will be moving faster due to the increased effects of gravity. In a gi ...
									Cosmic Samples & Origin of Solar System
									
... The solar nebula model attempts to explain how the solar system may have formed The model is still “evolving” and many of its details are yet to be worked out Powerful computers are used for simulations ...
                        	... The solar nebula model attempts to explain how the solar system may have formed The model is still “evolving” and many of its details are yet to be worked out Powerful computers are used for simulations ...
									the orbit of venus
									
... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth?___________________ ________________________ ...
                        	... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth?___________________ ________________________ ...
									Student Text, pp. 139-144
									
... of the universe. Astronomers studied the motion of Uranus over many years and discovered that its path was not quite as smooth as expected. Some distant hidden object appeared to be “tugging” on Uranus causing a slightly uneven orbit. Using detailed mathematical analysis, they predicted where this h ...
                        	... of the universe. Astronomers studied the motion of Uranus over many years and discovered that its path was not quite as smooth as expected. Some distant hidden object appeared to be “tugging” on Uranus causing a slightly uneven orbit. Using detailed mathematical analysis, they predicted where this h ...
									Lecture 10
									
... objects, which are defined by reference to the celestial equator and celestial poles, must also be constantly changing. • Because of this change in the direction of the Earth's pole with time, the coordinate systems of RA and DEC that we adopt for one epoch are actually different for other epochs. • ...
                        	... objects, which are defined by reference to the celestial equator and celestial poles, must also be constantly changing. • Because of this change in the direction of the Earth's pole with time, the coordinate systems of RA and DEC that we adopt for one epoch are actually different for other epochs. • ...
									doc - Steve Kluge
									
... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth? _________ _________________________________ ...
                        	... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth? _________ _________________________________ ...
									Powerpoint - Physics and Astronomy
									
... How did the Solar System Form? We weren't there (it was 5 billion years ago). We need a good theory. We can try to check it against other forming solar systems. What must it explain? - Solar system is very flat. - Almost all moons and planets (and Sun) rotate and revolve in the same direction. - Pl ...
                        	... How did the Solar System Form? We weren't there (it was 5 billion years ago). We need a good theory. We can try to check it against other forming solar systems. What must it explain? - Solar system is very flat. - Almost all moons and planets (and Sun) rotate and revolve in the same direction. - Pl ...
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.
 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									