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Chapter 30 - Cloudfront.net
Chapter 30 - Cloudfront.net

... discovered by Galileo in 1610  In addition to the four large moons discovered by Galileo, scientists have observed dozens of smaller moons around Jupiter.  Of Jupiter’s four Galilean moons, three are larger than Earth’s moon.  Jupiter has a single, thin ring made of microscopic particles that may ...
Is Pluto a Planet
Is Pluto a Planet

... • a star (the sun) • four giant gaseous planets (Jupiter, Saturn, Uranus, Neptune) with generally stable elliptical orbits with e < 0.06 (where e = 0 represents a circle, and e = 1 is a parabola, which is an open-ended or non-closed orbit); their orbits also have low inclinations with respect to the ...
Jovian Planet Systems Jovian Planet Systems
Jovian Planet Systems Jovian Planet Systems

... • Once these planets grew massive enough, they could draw in even lower-density hydrogen and helium gas directly from the nebula by gravitational ...
Universe 8e Lecture Chapter 14 Uranus, Neptune, Pluto
Universe 8e Lecture Chapter 14 Uranus, Neptune, Pluto

... The magnetic axes of both Uranus and Neptune are steeply inclined from their axes of rotation. The magnetic and rotational axes of all the other planets are more nearly parallel. The magnetic fields of Uranus and Neptune are also offset from the centers of the planets. ...
Chapter 9 Asteroids, Comets, and Dwarf Planets
Chapter 9 Asteroids, Comets, and Dwarf Planets

... • Asteroids are rocky leftovers of planet formation. • The largest is Ceres, diameter ~1,000 km. • There are 150,000 in catalogs, and probably over a million with diameter >1 km. • Small asteroids are more common than large asteroids. • All the asteroids in the solar system wouldn’t add up to even a ...
Saturn
Saturn

...  July 2004: Cassini arrived on Saturn ...
Chapter 12 Asteroids, Comets, and Dwarf Planets What are
Chapter 12 Asteroids, Comets, and Dwarf Planets What are

... cross, because of 3:2 orbital resonance • Neptune orbits three times during the time Pluto orbits twice ...
answer key
answer key

... 3. How have the best photographs of asteroids been obtained? Probe flybys are the source of our best images of asteroids. The Galileo probe went on a CRAZY ride before reaching its intended destination, Jupiter. (After launch it passed Venus for a gravity boost, then got halfway to Mars and came bac ...
lecture15_2014_giant_planets
lecture15_2014_giant_planets

... Massive and Gaseous (H, He) ? Formed beyond the frost line (3 AU): so cold that ice particles exist with silicate dust. Ice and Dust collides, sticks grows into icy-rocky core. Core’s gravity captures H/He gas Planet attracts ices and dust that orbit Moons formed out of these disks: A miniature sola ...
CH28 Solar System - Van Buren Public Schools
CH28 Solar System - Van Buren Public Schools

... hundreds of thousands of years to complete a single orbit around the Sun. However, a few short-period comets (those having orbital period of less than 200 years) such as Halley’s comet, make a regular encounters with the ...
Jupiter, Saturn, Uranus, and Neptune
Jupiter, Saturn, Uranus, and Neptune

... Interior of Uranus • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge suppor ...
The Role of Comets in the Late Heavy Bombardment
The Role of Comets in the Late Heavy Bombardment

... •  IniIal  condiIons  using  elements  of  6014  disk   objects  reaching  perihelia  with  q  <  3.9  AU  in  the   Nice  Model  (Brož  et  al.  2013)   •  Down-­‐selec>on  (P  <  20  yr  and  TJ  >  2)  ⇒  5000  sets  of   ele ...
Future exploration of the outer sola
Future exploration of the outer sola

... tilt was caused during the outward planetary migration phase due to a large additional uranian satellite do not seem to agree with existing satellite formation scenarios. Assuming that giant impact hypothesis, Mousis presented two extreme cases: one where the Uranus sub­ nebula contains very little ...
How Planets Form (990L)
How Planets Form (990L)

... raging arena filled with gas, dust, and massive chunks of rock. There is stuff everywhere, and it's hard to see the stars. All around you, rocks are plowing silently and slowly through the gas and dust, leaving powdery trails and twists. Large pieces glow with heat, as they sweep up smaller bodies. ...
here
here

... cross, because of 3:2 orbital resonance • Neptune orbits three times during the time Pluto orbits twice ...
here - ScienceA2Z.com
here - ScienceA2Z.com

... proportion of ices in their makeup. Some astronomers suggest they belong in their own category, “ice giants.” All four gas giants have rings, although only Saturn's ring system is easily observed from Earth. The outer planets from top to bottom: Jupiter, Saturn, Uranus, and Neptune (not to scale) ...
Ch 12 slides - UNLV Physics
Ch 12 slides - UNLV Physics

... •! Pluto will never hit Neptune, even though their orbits cross, because of 3:2 orbital resonance •! Neptune orbits three times during the time Pluto orbits twice ...
12_LectureOutlines
12_LectureOutlines

... By far the smallest planet. Not a gas giant like other outer planets. Has an icy composition like a comet. Has a very elliptical, inclined orbit. Pluto has more in common with comets than with the eight major planets • Its orbit around the sun is mathematically chaotic on time scales of 100million y ...
Asteroids
Asteroids

... Trojan Asteroids • The law of gravity permits an orbit around the sun exactly 60º ahead of and behind Jupiter, called Lagrange points. – Asteroids collect there – Several hundred Trojan asteroids locked to Jupiter ...
Terrestrial Planets - Empyrean Quest Publishers
Terrestrial Planets - Empyrean Quest Publishers

... Pluto: why not a planet? •Pluto is a special case – An outer planet, but smaller than any of the terrestrial planets – Intermediate average density of about 1900 kg/m3 – Density suggests it is composed of a mixture of ice and rock – Its orbit has large eccentricity and inclination angle – It is now ...
Pocket Solar System
Pocket Solar System

... line along the fold marking the orbit and write the name of the planet along that line. This will help keep the writing small enough so the names are less likely to overlap orbits for other planets, especially for the inner planets. An alternative, to speed things up when visitors may not know how t ...
Activity: Pocket solar system
Activity: Pocket solar system

... line along the fold marking the orbit and write the name of the planet along that line. This will help keep the writing small enough so the names are less likely to overlap orbits for other planets, especially for the inner planets. An alternative, to speed things up when visitors may not know how t ...
Asteroids - mjeffries
Asteroids - mjeffries

... Trojan Asteroids • The law of gravity permits an orbit around the sun exactly 60º ahead of and behind Jupiter, called Lagrange points. • Several hundred Trojan asteroids are known. • There are small asteroids locked to other planets. ...
The Fathers of the Gods: Jupiter and Saturn
The Fathers of the Gods: Jupiter and Saturn

... radiates over twice as much energy back into space as it receives from the Sun  Like Jupiter, Saturn is still contracting  As is contracts, heat is produced ...
Lecture 1: Our Solar System
Lecture 1: Our Solar System

... Pluto is very low in mass and moderate in density (about 2000 kg/m3). It is surmised that Pluto is made of mixture of ice and rock. ...
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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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