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Earth and Space Sciences 9 - UCLA
Earth and Space Sciences 9 - UCLA

... b) If Io’s eccentricity decreased, what would happen to the amount of heating it experiences? (1 point) It would decrease c) Why does Io’s eccentricity not decrease over time? (4 points) Because it is in a Laplace resonance with Europa and Ganymede and so its eccentricity is continuously pumped up b ...
How Was the Solar System Formed?
How Was the Solar System Formed?

... forming larger and larger bodies. Eventually they formed the rocky inner planets. These include Mercury, Venus, Earth, and Mars. They are the closest planets to the sun. Farther from the Sun, the temperature was very cold. Water froze into ice. Chunks of ice bumped into each other. Gas and dust were ...
How Was the Solar System Formed? Questions
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... Eventually they formed the rocky inner planets. These include Mercury, Venus, Earth, and Mars. They are the closest planets to the ...
8. Welcome to the Solar System
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... material comes from dust from comets, some from asteroids. ...
solar system - cayugascience
solar system - cayugascience

... material comes from dust from comets, some from asteroids. ...
Solar System Exam: Name:
Solar System Exam: Name:

... ____31. A couple features in the solar system are named “The Great Red Spot” or “The Dark Spot?” A. These are large, long-lived “hurricane” storm systems. B. These are anomalies in the belts and zones of the planet. C. These are methane and ammonia gas eruption zones from a hotspot region. D. These ...
Moons of the Outer Solar System
Moons of the Outer Solar System

... Io and Europa Jupiter’s Io  Is the most volcanic object in the Solar System due to  Tidal heating caused by the gravitational tug of war it experiences from Jupiter and its sister Galilean satellites. Jupiter’s Europa  Has similar but weaker tidal heating,  Has a young cracked water ice crust pe ...
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Outer Planets!

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... but, because Saturn is further from the sun and colder, the cloud layers are deeper in the hydrogen atmosphere below a layer of methane haze. ...
The Planets
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... – Earth is the only planet known to harbor life. • hydrosphere: the portion of Earth that is water • The atmosphere protects Earth from radiation. – Earth’s atmosphere is 78% nitrogen, 21% oxygen, and 1% carbon dioxide and other gases. – The atmosphere protects Earth from harmful radiation and high- ...
The Other Distant Giants Are Kindred Planets with Individual Quirks
The Other Distant Giants Are Kindred Planets with Individual Quirks

... so much farther from the Sun that its orbit takes nearly 30 Earth years to complete, but its day is a whirlwind eleven hours. Haze high in its atmosphere masks its bands of jet streams that are similar to Jupiter’s. Liquid metallic hydrogen surrounding Saturn’s core is responsible for its magnetic ...
The Solar System: JUPITER by - Etiwanda E
The Solar System: JUPITER by - Etiwanda E

... 1610. These moons are known as the Galilean moons: Io, Ganymede, Callisto, and Europa. This was important evidence that the earth was not the center of the solar ...
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CHAPTER 9.3: The Outer Planets

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The Modern Solar System
The Modern Solar System

...  Greatest Elongation - the largest separation of the planet from the Sun in our sky, either to the East, or to the West ...
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The Planets - Giants video questions

... pieces stuck together resulting in the surface Voyager observed. Perhaps it was just such a collision that knocked Uranus over on its ________________ during the early days of the Solar System. 34) Neptune is 3 billion miles from Earth. The challenge with Neptune was that the scientists had to know ...
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The Outer Planets

... List 4 ways the Jovian planets are different than the inner planets? For one of the differences above, explain why they have this difference List 1 similarity between the outer and inner planets ...
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PPT
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ASTRONOMY 161
ASTRONOMY 161

... made of ice, hundreds of kilometers across. (The “Kuiper Belt” lies beyond the orbit of Neptune.) ...
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The Planets

... Uranus, and Neptune  The four planets beyond the asteroid belt ...
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Solar System Formation

... Describe something you have already learned in this course that you did not know previously. 1. clathrates are ices with molecules inserted into ice structure 2. storm on Neptune is a downwelling compared to Jupiter’s GRS upwelling 3. Titan has magic islands on its mare that appear/disappear 4. spac ...
Week 6 Notes The Outer Planets
Week 6 Notes The Outer Planets

... e. __GRAVITY__ keeps the gases from __ESCAPING__ f. Gas Giants are made up of __LIQUID__ for of the gas due to the enormous __PRESSURE__ g. All of the gas giants have many __MOONS__ and a set of __RINGS__ ...
This is the Edge
This is the Edge

... Voyager flyby Neptune and Triton ...
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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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