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Earth does not move around the Sun
scribd.com ext: .pdf 1 KB date: 2012-01-30
Source title: test bench for dynamic range testing of adc
www.scribd.com 
Video results for: earth moving the sun 
model of our solar system,Earth Is Not Orbiting…
Beautiful model of our solar system avaiable in (More) Beautiful model of our solar system avaiable in online store: http://www.orrerystore.com/ .Earth Is Not Orbiting The Sun in the way we were taught More to do with Something Wrong With The Sun Moon & Earth series. Here we find an understanding of Why the Earth & our solar system do not actually orbit the Sun as taught, "Rather", We follow or better still, are dragged by the Sun in a Spiral Pattern through the universe & time.This video offers explanations how, besides spinning on its axis and rotating as if going 'Around' the Sun, the Earth is shown to 'Follow' the Sun's movement through the Milky Way galaxy, in a continuous Spiral, not a Flat elliptical plane, thus we find a 3D universe as opposed to the accepted 2D. ** Believe it or not, there is no empirical evidence that the Earth actually orbits the sun ! **This compilation of videos runs thus:"The solar system's motion thru space by The Resonance Project / Nassim Haramein"This simple animation was created by Nassim Haramein and The Resonance Project Foundation This is a video clip that every human should see. Many of us have been taught about how the solar system works by viewing a physical model that has the sun in the middle with the planets going around and around in a simple circular orbit without properly accounting for the motion of the sun (aprox. 450,000 miles per hour). Because the both sun and the galaxy are moving through space, the Earth spirals an incredible distance through space in a year's time. How far the Earth moves depends on the reference point you are using for something "stationary" or "background" even though all objects in the universe are in motion. The Earth rotates at 0-1040 mi/hr (depends on latitude)The Earth orbits the sun at aprox. 66,629 mi/hrThe sun orbits the galactic centre at aprox. 447,000 mi/hrIn just considering how fast the sun is moving, we know the Earth travels at least 3,918,402,000 miles in a years time! (as it also orbits around the sun)Total speed of the Earth moving through space is difficult to approximate do to the combination of motions.Using Cosmic Microwave Background (CMB) radiation it is estimated the total motion of the Earth through space is aprox. 1,342,000 mi/hrOr 11,763,972,000 miles in 1 year! (which is still only 0.2% the speed of light!)The old model might make one picture being back where you started after a year of time has past, when in fact, you are over 11 BILLION miles from where you were a year ago!I hope this video helps people to visualize what the motion of the Earth in our solar system looks like.For more information on Nassim Haramein and The Resonance Project, Please visit:xxx.theresonanceproject.org" ---xxx.youtube.com/user/EarthPilgrims"Nassim Haramein describing the limitations of the 2D solar system image, and how our evolution imprints space time. Excerpt from the film 'Earth Pilgrims' " ---xxx.youtube.com/user/aukruger"This animation is a video screenshot from Voyage through The Solar System version 1.20 (1989) and shows the earth's true motion in spirals. Besides spinning on its axis and rotating around the Sun, the Earth also follows the Sun's movement through the Milky Way galaxy. " Please Visittheresonanceproject.org/xxx.earthpilgrims.com/xxx.youtube.com/user/aukrugerxxx.YouTube.Com/MichelDezanger;model of our solar system. An orrery is a mechanical device that illustrates motions and the relative positions of the planets and moons in the Solar System in a heliocentric model.They are typically driven by a motor or a clockwork mechanism with a globe representing the Sun at the centre, and with a planet at the end of each of the arms. Though the Greeks had working planetaria, the first orrery that was a planetarium of the modern era was produced in 1704, and one was presented to the Earl of Orrery --- whence the name came. An orrery can be seen as a scale model of our solar system.The first modern orrery was made circa 1704 by Thomas Tompion and George Graham.Graham gave the first model (or its design) to the celebrated instrument maker John Rowley lived in London,in order to make a copy for Prince Eugene of Savoy. Rowley made ather copy for his patron Charles Boyle,4th Earl of Orrery, from which the model took its name.This device was given to Charles' son John as present,later the 5th Earl. Its importance was partially in that mechanical scale models of the solar system and the universe, correctly named planetariums gained the name Orrery.I have a beautiful orrery(solar system scale model).Get it at http://www.orrerystore.com (Less)
Venus Transit of the Sun, A Celestial Rarity
NASA joined the world in viewing a rare celestial (More) NASA joined the world in viewing a rare celestial event, one not seen by any person now alive. The planet Venus appeared to cross in front of the Sun as seen from Earth. The last "Venus transit" occurred more than a century ago, in 1882, and was used to compute the distance from the Earth to the Sun. Scientists with NASA's Kepler mission hope to discover Earth-like planets outside our solar system by searching for transits of other stars by planets that might be orbiting them. The Venus transit was visible over about 75 percent of the Earth, and ended at sunrise over central and eastern North America. The event was over by the time the Sun rises over the West Coast of North America (but viewers in Alaska could see the beginning of the transit and, for Northern Alaskans, the entire transit, because the Sun does not go below the horizon). "People using a filter approved for safe solar viewing can expect to see a small black dot, about 1/30 the size of the solar disk, very slowly moving across the Sun," said Fred Espenak, an eclipse expert at NASA's Goddard Space Flight Center, Greenbelt, Md. If people missed the June 8 Venus transit, they will have another chance in 2012 (June 6). After that, there will not be another Venus transit until 2117 (December 11). "There will be no other till the twenty-first century of our era has dawned upon the Earth and the June flowers are blooming in 2004. What will be the state of science ... God only knows." - William Harkness, U.S. Naval Observatory 1882 During the 19th century, Venus transits were essential for astronomers to fathom the scale of the heavens, because they were used to give a relatively accurate distance from the Earth to the Sun. Once that distance was known accurately, astronomers could determine the size of our solar system, and calculate the distances to nearby stars by measuring how much they appeared to shift against remote background stars as the Earth progressed in its orbit around the Sun. So critical was this measurement that, beginning in 1761, leading nations sent expeditions to remote corners of the globe to time exactly when Venus appeared to begin its transit of the Sun. The precise timing of the transit depended on location because different places on the globe saw the event from different angles. The times were compared and the distance to the Sun calculated using the known distances between expedition locations on the Earth and trigonometry. Educators and students may do the calculations by following an activity on the Web site or on the half-hour NASA Connect TV program. The transit phenomenon has relevance to the future of astronomy as well. There is evidence for more than 100 extrasolar planets (planets outside our solar system) around other nearby stars. However, current techniques can only detect large planets, gas giants like Jupiter. But a star might have a planet that appears to pass in front of it by chance alignment with the Earth, and planets similar in size to the Earth could be detected if they transit their parent star. NASA's Kepler mission, scheduled for launch in October 2007, will allow astronomers to find smaller, presumably terrestrial extrasolar planets by looking for tiny dips in the brightness of a star when a planet crosses in front of it. Periodic brightness dips will signal the presence of a planet in orbit around the star, even if the planet itself is not directly visible. Kepler will observe about 100,000 stars in a patch of sky in the direction of the constellation Cygnus for four years, making brightness measurements every 15 minutes, in hopes of catching elusive transits. The Kepler mission is expected to detect 50 to 60 extrasolar planets with a similar distance from their parent stars as the Earth is from the Sun. (Less)
model of our solar system,Earth Is Not Orbiting… Beautiful model of our solar system avaiable in (More) Beautiful model of our solar system avaiable in online store: http://www.orrerystore.com/ .Earth Is Not Orbiting The Sun in the way we were taught More to do with Something Wrong With The Sun Moon & Earth series. Here we find an understanding of Why the Earth & our solar system do not actually orbit the Sun as taught, "Rather", We follow or better still, are dragged by the Sun in a Spiral Pattern through the universe & time.This video offers explanations how, besides spinning on its axis and rotating as if going 'Around' the Sun, the Earth is shown to 'Follow' the Sun's movement through the Milky Way galaxy, in a continuous Spiral, not a Flat elliptical plane, thus we find a 3D universe as opposed to the accepted 2D. ** Believe it or not, there is no empirical evidence that the Earth actually orbits the sun ! **This compilation of videos runs thus:"The solar system's motion thru space by The Resonance Project / Nassim Haramein"This simple animation was created by Nassim Haramein and The Resonance Project Foundation This is a video clip that every human should see. Many of us have been taught about how the solar system works by viewing a physical model that has the sun in the middle with the planets going around and around in a simple circular orbit without properly accounting for the motion of the sun (aprox. 450,000 miles per hour). Because the both sun and the galaxy are moving through space, the Earth spirals an incredible distance through space in a year's time. How far the Earth moves depends on the reference point you are using for something "stationary" or "background" even though all objects in the universe are in motion. The Earth rotates at 0-1040 mi/hr (depends on latitude)The Earth orbits the sun at aprox. 66,629 mi/hrThe sun orbits the galactic centre at aprox. 447,000 mi/hrIn just considering how fast the sun is moving, we know the Earth travels at least 3,918,402,000 miles in a years time! (as it also orbits around the sun)Total speed of the Earth moving through space is difficult to approximate do to the combination of motions.Using Cosmic Microwave Background (CMB) radiation it is estimated the total motion of the Earth through space is aprox. 1,342,000 mi/hrOr 11,763,972,000 miles in 1 year! (which is still only 0.2% the speed of light!)The old model might make one picture being back where you started after a year of time has past, when in fact, you are over 11 BILLION miles from where you were a year ago!I hope this video helps people to visualize what the motion of the Earth in our solar system looks like.For more information on Nassim Haramein and The Resonance Project, Please visit:xxx.theresonanceproject.org" ---xxx.youtube.com/user/EarthPilgrims"Nassim Haramein describing the limitations of the 2D solar system image, and how our evolution imprints space time. Excerpt from the film 'Earth Pilgrims' " ---xxx.youtube.com/user/aukruger"This animation is a video screenshot from Voyage through The Solar System version 1.20 (1989) and shows the earth's true motion in spirals. Besides spinning on its axis and rotating around the Sun, the Earth also follows the Sun's movement through the Milky Way galaxy. " Please Visittheresonanceproject.org/xxx.earthpilgrims.com/xxx.youtube.com/user/aukrugerxxx.YouTube.Com/MichelDezanger;model of our solar system. An orrery is a mechanical device that illustrates motions and the relative positions of the planets and moons in the Solar System in a heliocentric model.They are typically driven by a motor or a clockwork mechanism with a globe representing the Sun at the centre, and with a planet at the end of each of the arms. Though the Greeks had working planetaria, the first orrery that was a planetarium of the modern era was produced in 1704, and one was presented to the Earl of Orrery --- whence the name came. An orrery can be seen as a scale model of our solar system.The first modern orrery was made circa 1704 by Thomas Tompion and George Graham.Graham gave the first model (or its design) to the celebrated instrument maker John Rowley lived in London,in order to make a copy for Prince Eugene of Savoy. Rowley made ather copy for his patron Charles Boyle,4th Earl of Orrery, from which the model took its name.This device was given to Charles' son John as present,later the 5th Earl. Its importance was partially in that mechanical scale models of the solar system and the universe, correctly named planetariums gained the name Orrery.I have a beautiful orrery(solar system scale model).Get it at http://www.orrerystore.com (Less)
Venus Transit of the Sun, A Celestial Rarity NASA joined the world in viewing a rare celestial (More) NASA joined the world in viewing a rare celestial event, one not seen by any person now alive. The planet Venus appeared to cross in front of the Sun as seen from Earth. The last "Venus transit" occurred more than a century ago, in 1882, and was used to compute the distance from the Earth to the Sun. Scientists with NASA's Kepler mission hope to discover Earth-like planets outside our solar system by searching for transits of other stars by planets that might be orbiting them. The Venus transit was visible over about 75 percent of the Earth, and ended at sunrise over central and eastern North America. The event was over by the time the Sun rises over the West Coast of North America (but viewers in Alaska could see the beginning of the transit and, for Northern Alaskans, the entire transit, because the Sun does not go below the horizon). "People using a filter approved for safe solar viewing can expect to see a small black dot, about 1/30 the size of the solar disk, very slowly moving across the Sun," said Fred Espenak, an eclipse expert at NASA's Goddard Space Flight Center, Greenbelt, Md. If people missed the June 8 Venus transit, they will have another chance in 2012 (June 6). After that, there will not be another Venus transit until 2117 (December 11). "There will be no other till the twenty-first century of our era has dawned upon the Earth and the June flowers are blooming in 2004. What will be the state of science ... God only knows." - William Harkness, U.S. Naval Observatory 1882 During the 19th century, Venus transits were essential for astronomers to fathom the scale of the heavens, because they were used to give a relatively accurate distance from the Earth to the Sun. Once that distance was known accurately, astronomers could determine the size of our solar system, and calculate the distances to nearby stars by measuring how much they appeared to shift against remote background stars as the Earth progressed in its orbit around the Sun. So critical was this measurement that, beginning in 1761, leading nations sent expeditions to remote corners of the globe to time exactly when Venus appeared to begin its transit of the Sun. The precise timing of the transit depended on location because different places on the globe saw the event from different angles. The times were compared and the distance to the Sun calculated using the known distances between expedition locations on the Earth and trigonometry. Educators and students may do the calculations by following an activity on the Web site or on the half-hour NASA Connect TV program. The transit phenomenon has relevance to the future of astronomy as well. There is evidence for more than 100 extrasolar planets (planets outside our solar system) around other nearby stars. However, current techniques can only detect large planets, gas giants like Jupiter. But a star might have a planet that appears to pass in front of it by chance alignment with the Earth, and planets similar in size to the Earth could be detected if they transit their parent star. NASA's Kepler mission, scheduled for launch in October 2007, will allow astronomers to find smaller, presumably terrestrial extrasolar planets by looking for tiny dips in the brightness of a star when a planet crosses in front of it. Periodic brightness dips will signal the presence of a planet in orbit around the star, even if the planet itself is not directly visible. Kepler will observe about 100,000 stars in a patch of sky in the direction of the constellation Cygnus for four years, making brightness measurements every 15 minutes, in hopes of catching elusive transits. The Kepler mission is expected to detect 50 to 60 extrasolar planets with a similar distance from their parent stars as the Earth is from the Sun. (Less)
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