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Saturn
Saturn

...  Five missions have been sent to Saturn. Since 2004, Cassini have been exploring Saturn, its moons and rings.  To enter Saturn’s orbit, you have to fly rings through the gap between the F and G, which is farther from the planet than the Cassini Division. ...
Jupiter and Saturn
Jupiter and Saturn

... of Jupiter and Saturn? 2. What is going on in Jupiter’s Great Red Spot? 3. What is the nature of the multicolored clouds of Jupiter and Saturn? 4. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 5. How do astronomers know about the deep interiors of Jupite ...
Jupiter and Saturn
Jupiter and Saturn

... of Jupiter and Saturn? 2. What is going on in Jupiter’s Great Red Spot? 3. What is the nature of the multicolored clouds of Jupiter and Saturn? 4. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 5. How do astronomers know about the deep interiors of Jupite ...
Chapter 9 Lecture Notes
Chapter 9 Lecture Notes

... of Jupiter and Saturn? 2. What is going on in Jupiter’s Great Red Spot? 3. What is the nature of the multicolored clouds of Jupiter and Saturn? 4. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 5. How do astronomers know about the deep interiors of Jupite ...
By Shannon and Sonia
By Shannon and Sonia

... these are large. • Titan is one of Saturn's moons and is the second largest moon in the Solar System, but What is the most are tiny. name of • More moons of Saturn's will Saturn's probably be discovered in the largest moon? coming years. ...
Jupiter`s and Saturn`s Moons
Jupiter`s and Saturn`s Moons

... of Jupiter and Saturn? 2. What is going on in Jupiter’s Great Red Spot? 3. What is the nature of the multicolored clouds of Jupiter and Saturn? 4. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 5. How do astronomers know about the deep interiors of Jupite ...
The Outer Planets
The Outer Planets

... Chapter 3, Lesson 3 ...
Lecture 12
Lecture 12

... planet’s equator • This system is tilted away from the plane of Saturn’s orbit, which causes the rings to be seen at various angles by an Earth-based observer over the course of a Saturnian year ...
Ch. 15
Ch. 15

... Icy planetesimals far from the Sun were ejected into distant orbits by gravitational interaction with the jovian planets, into the Kuiper belt and the Oort cloud. Some were left with extremely eccentric orbits, and appear in the inner solar system as comets. ...
Comins Chapter 8 - The Outer Planets
Comins Chapter 8 - The Outer Planets

... surrounded by a thick layer of liquid metallic hydrogen and an outer layer of ordinary liquid hydrogen. Both planets have an overall chemical composition very similar to that of the Sun. The visible features of Jupiter exist in the outermost 100 km of its atmosphere. Saturn has similar features, but ...
It is marvelous indeed to watch on television the
It is marvelous indeed to watch on television the

... It is marvelous indeed to watch on television the rings of Saturn close; and to speculate on what we may yet find at galaxy’s edge. But in the process, we have lost the human element; not to mention the high hope of those quaint days when flight would create “one world.'” Instead of one world, we ha ...
The orbital history of two periodic comets encountering Saturn
The orbital history of two periodic comets encountering Saturn

... found, by means of numerical integrations, to have recently encountered Saturn, leading to drastic orbital changes. In both cases the orbit was transformed from a Saturn-dominated regime (roughly tangential to Saturn’s orbit) into a deep Jupiter-crossing orbit. For P/1997 T3 a close encounter to wit ...
Asteroids,Comets, Meteor ppt.
Asteroids,Comets, Meteor ppt.

... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Asteroids,Comets, Meteor ppt.
Asteroids,Comets, Meteor ppt.

... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Neptune - barransclass
Neptune - barransclass

... Plan your trip today, to the last and farthest planet out into our solar system. ...
The Jovian Planets - Sierra College Astronomy Home Page
The Jovian Planets - Sierra College Astronomy Home Page

... Planetary Rings - Saturn Planetary Rings  Saturn’s rings are very thin, in some cases less than 100 meters thick.  The rings are not solid sheets but are made up of small particles of water ice or water-ice mixed with dust.  Three distinct rings are visible from Earth, and were named (outer to in ...
(1)In bold text, Knowledge and Skill Statement
(1)In bold text, Knowledge and Skill Statement

... 9 (C) relate the role of Newton's law of universal gravitation to the motion of the planets around the Sun and to the motion of natural and artificial satellites around the planets ...
The Structure of Earth`s Atmosphere
The Structure of Earth`s Atmosphere

... magnetic field • Rapid rotation and large size → belt-zone cloud pattern • Dust from meteorite impacts onto inner moons trapped to form ring ...
Uranus
Uranus

... making it the least massive of the giant planets. Its diameter is slightly larger than Neptune's at roughly four times Earth's. A resulting density of 1.27 g/cm3 makes Uranus the second least dense planet, after Saturn. This value indicates that it is made primarily of various ices, Improve yourand ...
Uran_Nep
Uran_Nep

... Neptune’s Magnetic Field ...
09 Giant Planets
09 Giant Planets

... into a single storm, which then turned red. This may provide some clues to the dynamics behind Jupiter’s cloud movements. ...
jupiter facts for kids - National Astronomy Week 2014
jupiter facts for kids - National Astronomy Week 2014

... Six have got there so far, although five of those went straight past without stopping. The first two probes to reach Jupiter were Pioneer 10 and Pioneer 11 which flew past in 1973 and 1974. These were followed by Voyagers 1 and 2, both in 1979. The first probe to go into orbit around Jupiter was cal ...
Jupiter Reading Comprehension Worksheet
Jupiter Reading Comprehension Worksheet

... Jupiter has its own 'mini solar system' of 49 moons. Scientists are most interested in the Galilean satellites the four largest moons discovered by Galileo Galilei in 1610. Europa, may have an ocean under its frozen surface. Calisto's crater-pocked landscape may be the oldest in the solar system. Ga ...
Jupiter - Mestre a casa
Jupiter - Mestre a casa

... Jupiter has its own 'mini solar system' of 49 moons. Scientists are most interested in the Galilean satellites the four largest moons discovered by Galileo Galilei in 1610. Europa, may have an ocean under its frozen surface. Calisto's crater-pocked landscape may be the oldest in the solar system. Ga ...
Voyager 2
Voyager 2

... indicating a different chemical composition there. ...
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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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