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Outer Planets - MrTravisSciencePage
Outer Planets - MrTravisSciencePage

... Neptune • Neptune’s atmosphere is similar to Uranus’s – Hydrogen, helium,methane & nitrogen – The core/center of Neptune is probably ice and rock – Called an “ice giant like Uranus ...
Our Solar System
Our Solar System

... terrestrial worlds — Mercury, Venus, Earth and Mars. After that are four gas giants — Jupiter, Saturn, Uranus and Neptune. Between the orbits of Mars and Jupiter lies the asteroid belt, which includes the dwarf planet Ceres. Beyond the orbit of Neptune one finds the disk-shaped Kuiper belt, in which ...
Planets Around Sun
Planets Around Sun

... than 0.1 AU all reside in circular orbits, plausibly induced by tidal interactions with the host star. In contrast, all 9 planet candidates that orbit farther than 0.2 AU (out to 2.5 AU) reside in eccentric orbits with ellipticities, e>0.1, more elliptical than the orbits of Jupiter (e=0.048) and Ea ...
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The Outer Planets

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... thin atmosphere of mostly carbon dioxide. The surface of Mars shares many features in common with Earth. There are shield volcanoes (extinct) and a deep canyon that indicate that tectonic activity once occurred on Mars, and there are erosional features—dried river and lake beds, gullies, and runoff ...
Other tenants
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... We have already mentioned that the planets with their satellites and rings are not the only bodies that occupy the Solar System. To start with, between the orbits of Mars and Jupiter, there is the Main Asteroid Belt that is not just a flat disc with rocks of different sizes and shapes as we usually ...
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A Tour of Our Solar System

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How the Universe Works – Planets
How the Universe Works – Planets

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How the Universe Works – Planets Astronomy Name: Date: 1. How

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... cores form first, then their gravity draws in gases 2. Gravitational Instability: clumps of gas form within a protoplanetary disk, they have strong enough gravity to collapse rapidly ...
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... worlds combined - yet, no spacecraft has been sent to a planet in this class. NASA's New Horizons mission to Pluto, its moon Charon and the Kuiper Belt is provisionally planned for launch in January 2006. After using a flyby of Jupiter in 2007 to get a gravitational kick, the spacecraft will reach P ...
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A Brief History of Planetary Science

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Page one 2011 November Rock Magnet

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HW Solar System Mnemonic

... The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt region is also termed the main belt to distinguish it from other concentra ...
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... Millions of Tiny Planets between Mars and Jupiter • State the nature and location in space of asteroids and describe the likelihood and danger of collisions with them. ...
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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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