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CHAPTER 9.3: The Outer Planets
CHAPTER 9.3: The Outer Planets

... 32.  In  2005  the  Cassini  orbiter  released  the  ___________________  probe  which  landed  on   Titan’s  surface.    It  discovered  seas  and  lakes  of  methane!!    Methane  is  a  gas  on  Earth   but  on  colder  Titan  it ...
1 - Humble ISD
1 - Humble ISD

... Solar System Debris: Dwarf & Minor Planets 19. What holds the Trojan asteroids in the position 60º ahead of and behind Jupiter?The gravity of the Sun and Jupiter are balanced 20. A carbonaceous asteroid is classified as what type?C-Type 21. An asteroid that is mostly stone is classified as what typ ...
Planets
Planets

... c. Tectonically dead d. Several canyons 1) Some larger than Earth’s Grand Canyon 2) Valles Marineras – the largest canyon a) Almost 5000 km long b) Formed from huge faults e. "Stream drainage" patterns 1) Found in some valleys 2) No bodies of surface water on the planet 3) Possible origins a) Past r ...
Solar System Study Guide Key
Solar System Study Guide Key

... 11. Give 3 facts about Jupiter. Has a very thick atmosphere; great red spot = storm larger than earth; largest planet in the solar system 12. Give 3 facts about Saturn. Second largest planet in the solar system; has several rings; and it’s atmosphere is mostly hydrogen and helium 13. Give 3 facts ab ...
6.8
6.8

... compare and contrast revolution and rotation and apply these terms to the relative movements of planets and their moons. (B2 and B2) model and describe how day and night and the phases of the moon occur. (B1 and B2) model and describe how Earth’s axial tilt and its annual orbit around the sun cause ...
The Solar System
The Solar System

Our Solar System
Our Solar System

... • Earth is warm enough to keep most of its water from freezing and cold enough to keep it’s water from boiling • Temperature is between –13 degrees Celsius and 37 degrees Celsius ...
SolarSystemPowerPoint
SolarSystemPowerPoint

... • Earth is warm enough to keep most of its water from freezing and cold enough to keep it’s water from boiling • Temperature is between –13 degrees Celsius and 37 degrees Celsius ...
Mercury`s year length is only 88 days compared to
Mercury`s year length is only 88 days compared to

Solar System Outlines
Solar System Outlines

... VII. The Inner Planets a. Surface ­ Rocky b. Size ­ Small c. Mercury ­ smallest planet, no atmosphere, no  moons d. Venus ­ about same size as Earth, thick  atmosphere, 475 Celsius, no moons e. Earth ­ largest inner planet, one moon, only  planet with liquid water, only known planet to support  life ...
Name_________________________ 1 AST 101 Ancient
Name_________________________ 1 AST 101 Ancient

... If  the  Earth  was  moving,  objects  like  the   Discovery  of  Jupiter’s  Moons   Moon  would  get  left  behind   Jupiter  is  moving  and  its  moons  are  not   left  behind   If  the  Earth  was  moving,  we  would  see   S ...
After Dark  M S
After Dark M S

... Professor Horace Smith It was not long ago that we knew only of the planets within our own solar system. Today the study of exoplanets, planets around suns beyond our own, is one of the most rapidly advancing in all of astronomy. As new and improved techniques for finding these worlds come into oper ...
The Solar System
The Solar System

... • Earth is our home, the third planet out. • It’s not to hot and not to cold. • And it is the only planet with life as far as we know. ...
Planet Review
Planet Review

... -Two Moons – Phobos and Deimos (captured asteroids?) ...
A. Comet: dust and rock particles combined with frozen water
A. Comet: dust and rock particles combined with frozen water

... breaks up, pieces spread out. The dust and rock fragments are called Meteoroids. ...
Planets of the Solar System
Planets of the Solar System

... • Mars' orbit is significantly elliptical. ...
Solar System Do you think our planet is the only place in the
Solar System Do you think our planet is the only place in the

... is an oval-shaped red spot in the clouds. Astronomers think this spot is a big storm that has been raging for hundreds of years! Saturn is the second largest planet and the sixth planet from the Sun. It has bright rings around it. Uranus and Neptune look like smooth blue balls. Methane gas gives the ...
Overview of our Solar System 1112 notes
Overview of our Solar System 1112 notes

... • At the center of our solar system • Contains 98.5% of all of the mass of the solar system • The first thing formed in our solar system • The largest and only star in our solar system • Provides almost all of the energy used in the solar system • Earth only gets 0.000000001% of the sun’s total ener ...
Solar System Science
Solar System Science

... Hints: The results may vary if the mix of planets is different in each system. The teacher should help students sum up the results, noting similarities and differences among the schemes. Most planetary scientists organize planets into two divisions: terrestrial (like Earth) and Jovian (like Jupiter) ...
1. Pre and Post test 2. Schedule of the orbits of the planets in our solar
1. Pre and Post test 2. Schedule of the orbits of the planets in our solar

... Pre-Post Test 1. How many planets have been discovered? a) more than 8 b) more than 12 ...
Planets and Other Space Rocks Notes
Planets and Other Space Rocks Notes

... • A year is 29.5 Earth years, and a day is 10.2 hours. • The temperature at the top is −178℃. • It has a tilt, so it has seasons like Earth, but they are mild. ...
Review Worksheet - Mrs. Sepulveda's Classes
Review Worksheet - Mrs. Sepulveda's Classes

... planetology and discuss its importance to solar system studies. Comparative planetology is the approach we use to study and understand our solar system. It involves comparing the worlds of our system, including planets, moons, asteroids, and comets, to one another. Its basic premise is that the simi ...
Other Objects in the Solar System
Other Objects in the Solar System

Heliocentric Model –The sun is the center of the solar system
Heliocentric Model –The sun is the center of the solar system

11 - Known Universe
11 - Known Universe

... Milky Way to the other. 12. There are over ____________________ galaxies in the cosmos. 13. In each galaxy there are hundreds of billions of _____________. 14. In the 1990’s we had not yet discovered other ______________ beyond our solar system. 15. We discovered other planets by watching stars ____ ...
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Nice model



The Nice model (/ˈniːs/) is a scenario for the dynamical evolution of the Solar System. It is named for the location of the Observatoire de la Côte d'Azur, where it was initially developed, in Nice, France. It proposes the migration of the giant planets from an initial compact configuration into their present positions, long after the dissipation of the initial protoplanetary gas disk. In this way, it differs from earlier models of the Solar System's formation. This planetary migration is used in dynamical simulations of the Solar System to explain historical events including the Late Heavy Bombardment of the inner Solar System, the formation of the Oort cloud, and the existence of populations of small Solar System bodies including the Kuiper belt, the Neptune and Jupiter Trojans, and the numerous resonant trans-Neptunian objects dominated by Neptune. Its success at reproducing many of the observed features of the Solar System means that it is widely accepted as the current most realistic model of the Solar System's early evolution, though it is not universally favoured among planetary scientists. One of its limitations is reproducing the outer-system satellites and the Kuiper belt (see below).
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