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Moon and Rings - Mid
Moon and Rings - Mid

... Ganymede - largest moon in Solar System, slightly larger than Mercury The closer to Jupiter, the higher the moon density (similar to behavior of terrestrial planets) => like mini “planetary” system! Intense heat of young Jupiter played role of sun. ...
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Satellites of Other Planets

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Universe Now - Course Pages of Physics Department
Universe Now - Course Pages of Physics Department

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Jovian planet

... and Santa Claus. December’s word is Jovian and it is most appropriate for this time of year. What is the connection between Santa and Jovian? Read on! Word of the Month for December 2001 Jovian plane t Any of the four giant planets (Jupiter, Saturn, Uranus and Neptune) that lie beyond the asteroid b ...
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The Asteroid Belt - peterboroughastronomy.com
The Asteroid Belt - peterboroughastronomy.com

... Current thinking holds that there should be a planet filling the gap between Mars and Jupiter. With a bit of imagination there is, only some assembly is required. The problem is the asteroids just can’t get together to form a planet when Jupiter’s incredible gravitational pull keeps tearing them apa ...
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JUPITER AND URANUS

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THE SOLAR SYSTEM Colton Morgan Baleigh Mercury Type a brief

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The Solar System

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Lecture Six (Powerpoint format) - FLASH Center for Computational

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... A) The planet is composed mostly of ice, with only a small fraction of rock. B) The planet has a satellite whose diameter is about half its own diameter. C) The planet has a circular orbit well beyond the orbit of Neptune. D) The planet will eventually break apart due to tidal forces from the Sun. 5 ...
The Planets - OrgSites.com
The Planets - OrgSites.com

... 23.4 Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
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... 23.4 Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
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... 23.4 Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
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Touring_Our_Solar_System_PowerPoint

... 23.4 Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
The Planets - Plain Local Schools
The Planets - Plain Local Schools

... 23.4 Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
Sample Final - Lawrence University
Sample Final - Lawrence University

... Why are mountains and volcanoes on Mars so much taller on Mars than on the Earth? (a) Mars lacks plate tectonics and has a lower surface gravity than the Earth. (b) The atmospheric pressure on Mars is much lower than on the Earth. (c) The surface of mars is composed of low-density ices. (d) Gigantic ...
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Physics 110 - Lawrence University

... Why are mountains and volcanoes on Mars so much taller on Mars than on the Earth? (a) Mars lacks plate tectonics and has a lower surface gravity than the Earth. (b) The atmospheric pressure on Mars is much lower than on the Earth. (c) The surface of mars is composed of low-density ices. (d) Gigantic ...
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Modeling the Solar System

... Science Standard 8-4 The student will demonstrate an understanding of the characteristics, structure, and predictable motions of celestial bodies. Indicator 8-4.1 Summarize the characteristics and movements of objects in the solar system (including planets, moons, asteroids, comets, and meteors). Pu ...
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Volcanoes and Igneous Activity Earth

... Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
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Space - SSI General Science

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Chapter 18 Folder
Chapter 18 Folder

... 2. universe 3. galaxy 4. crater 5. solar system 6. satellite 7. space probe p. 167 1. late 2009 2. middle 2012; late 2015 3. Yes, the second full moon would have occurred at the very end of the month. 4. They are referring to something that rarely or seldom happens. ...
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The composition of planetary atmospheres: a historical

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Jupiter is the fifth planet from the sun. It is by far the
Jupiter is the fifth planet from the sun. It is by far the

... scientist only knew of Saturn’s rings. Rings were seen on Uranus and Neptune as well. Both Voyager spacecraft have now left our solar system. They continue to fly outward through space. Who knows if they may make another unexpected discovery? ...
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Jumping-Jupiter scenario

The jumping-Jupiter scenario specifies an evolution of giant-planet migration described by the Nice model, in which an ice giant (Uranus, Neptune, or an additional Neptune-mass planet) encounters first Saturn and then Jupiter, causing the step-wise separation of their orbits. The jumping-Jupiter scenario was proposed by Ramon Brasser, Alessandro Morbidelli, Rodney Gomes, Kleomenis Tsiganis, and Harold Levison after their studies revealed that the smooth divergent migration of Jupiter and Saturn resulted in an inner Solar System significantly different from the current Solar System. The sweeping of secular resonances through the inner Solar System during the migration excited the eccentricities of the terrestrial planets beyond current values and left an asteroid belt with an excessive ratio of high- to low-inclination objects. The step-wise separation of Jupiter and Saturn described in the jumping-Jupiter scenario allows these resonances to quickly cross the inner Solar System without altering orbits excessively. The jumping-Jupiter scenario also results in a number of other differences with the original Nice model. The fraction of lunar impactors from asteroid belt during the Late Heavy Bombardment is significantly reduced, most of the Jupiter trojans are captured via an alternative mechanism, and Jupiter acquires its population of irregular satellites via the same process as the other planets. The frequent ejection of an ice giant during simulations of the jumping-Jupiter scenario has led some to propose an additional giant planet in the early Solar System.
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