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Solar System Model and
Solar System Model and

... 100! (This assumes the children take two steps per meter.) Space allowing, your students could model planetary orbits by walking around the Sun. See if you can get close to the correct year lengths for each planet! ...
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... caused by the pull of a small unseen planet. b. We have seen the motion of the planet caused by the wobble of the star. c. We have seen the changing position of the star caused by the pull of the small unseen planet. d. We have seen the changing velocity of the planet caused by the motion of the sta ...
Lecture 25: The Outer Planets
Lecture 25: The Outer Planets

... •Observations of the parallax of Neptune show that a = 30.1 AU, and therefore we obtain P = 164 Earth years •Since its discovery in 1846, 157 years have passed and Neptune has almost completed one orbit around the Sun ...
Chapter 22: Origin of Modern Astronomy
Chapter 22: Origin of Modern Astronomy

... Modern Greece, however, honors him, and even puts his theories on stamps… ...
Our Solar System
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...  Why is it that we can see certain planets, but not all planets?  Why do planets take different amounts of time to orbit the sun?  What is the difference between planets and moons? ...
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... Science and Exploration in the Outer Solar System in 2050. A. A. Simon (NASA Goddard Space Flight Center) Introduction: The best way to approach a vision 35 years into the future is to begin by looking back. A snapshot of the state of knowledge of the outer solar system in 1980 is quite different fr ...
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... There are about 500-600 known planets circling around other stars (other than the Sun). Many are likely to be barren (too hot or too cold), but some may be `habitable . Habitable = a narrow region of orbits around a star where water can be in liquid form Future NASA (and other) missions may establis ...
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... We viewed the TED Talk “The Search for Planets Beyond Our Solar System” by astronomer Dr. Sara Seager, MIT Professor. She asked you to be “the first generation to find the earth-like worlds” for our descendants to have interstellar travel. Your team will research at least seven details about your pl ...
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... Somewhere along the line, you should have noticed that many (if not the vast majority) of the smaller objects found in the solar system have wildly eccentric orbits. In addition, its seems possible that early in the Sun’s own life, one or more partner stars may have been near enough to cause gravita ...
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... and small rocky particles. They usually have long, narrow elliptical orbits. Asteroids are small, rocky space objects often found in orbit between Mars and Jupiter. Meteoroids are chunks of rock or dust in space. 21. It represents a gas giant. Its overall structure and composition resemble those of ...
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... closest to the sun.  Between March 21 and September 21, there are three days more than between September 21 and March 21. These two dates are the spring and fall equinoxes, when the days and nights are of equal length. Between the equinoxes, the Earth moves 180° around its orbit with respect to the ...
Our Solar System
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Solar System research questions Group 1 River, Mark, Tommy
Solar System research questions Group 1 River, Mark, Tommy

... consequences of that. Some of the large planets have sets of moons in retrograde revolutions around the planet. Which planets? How could that be explained? Why is Uranus orbiting on its side? Why don’t its rings and magnetic field align with its rotation? Why is Venus rotating backwards? Why do all ...
The Solar System
The Solar System

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The Outer Planets

... terrestrial planets in several ways. First, Jovian planets are much larger. The smallest Jovian planet, Uranus, is nearly 15 times more massive than the largest terrestrial planet, Earth. Second, Jovian planets do not have solid surfaces; instead the “surface” of each one consists of the uppermost g ...
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Planets beyond Neptune



Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.
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