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Planets of Our Solar System
Planets of Our Solar System

... like Earth) • 2 moons • No hot temperatures (range is -125C to 35C) ...
The Solar System - Kennesaw State University
The Solar System - Kennesaw State University

... Space Exploration ...
Untitled - IES Bachiller Sabuco
Untitled - IES Bachiller Sabuco

... across, they're no more than 1.5 kilometers. Their impressive appearance, there's really very little material in the rings. If the rings were compressed into a single body it would be no more than 100 km across. Saturn is the planet that has more comets near his orbit. ...
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... Radar Images of Surface ...
Vocabulary – Our Solar System
Vocabulary – Our Solar System

... The Moon is a large round rock that orbits the Earth once every 29 days. It is the fifth largest moon in our solar system. ...
The Solar System
The Solar System

... • Jupiter is the largest planet in the solar system, More than 1300 earths could fit inside it. • It has winds that go up to 400mph. • Jupiter is the 5th planet away from the sun{466 million miles} • It has 67 moons. • Jupiter's clouds are no more then 50 km in thickness. •Jupiter is one of the sola ...
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... too small to be called planets. Tens of thousands of these 'minor planets' are gathered in the main asteroid belt, a vast doughnut-shaped ring between the orbits of Mars and Jupiter. Asteroids that pass close to Earth are called nearearth objects. ...
27.4 Directed Reading Guide
27.4 Directed Reading Guide

... Original content Copyright © by Holt, Rinehart and Winston. Additions and changes to the original content are the responsibility of the instructor. ...
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4.2 The planets and their satellites

... missions to date. 4.2.1.1 Structure and dimension of the Solar System The Solar System contains a myriad of bodies ranging in size from the Sun to miniscule dust particles. The Encyclopedias of Planetary Sciences [97Shi] and the Solar System [99Wei] and the Planetary Companion [98Lod] are useful sou ...
3OriginofPlanetsandMoons
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... collided and aggregated into small, irregular shapes (planetesimals), and eventually formed into larger planets. •As the planets formed, the more dense ones were pulled closest to the sun. They are called Terrestrial Planets (Mercury, Venus, Earth, and Mars). •The less dense planets moved toward the ...
Unit 8.4 Solar System
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... 4. a. Pluto lost its status as a planet in 2006. b. Pluto is regarded as a dwarf planet because normal planets have enough gravity to sweep their orbits clear of debris, whereas the gravitational pull of dwarf planets is insufficient to do so. c. Two other dwarf planets are Eris and Ceres. 5. Terres ...
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... close to the Sun, its surface temperatures are extreme, ranging from 427°C (800°F) on the sunward side to –183°C (–297°F) on the side facing away from the Sun.  Mercury has no atmosphere and no surface water; the high temperatures prevent these from forming. EXCEPT-Frozen water was found at the pol ...
PHYS 390 Lecture 6 - A tour of the planets 6 - 1 Lecture 6
PHYS 390 Lecture 6 - A tour of the planets 6 - 1 Lecture 6

... the four Jovian planets also have rings. Four of Jupiter's moons were first observed by Galileo in 1610; their measured periods later allowed an independent determination of ...
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... of  the  Harvest  and  of  Time.   •  Father  of  Jupiter,  Neptune,   and  Pluto.   •  The  Roman  name  for  the   Greek  god  Cronos.   •  Saturnalia  was  the  mid-­‐ winter  fes1val  in  Saturn’s   honor.  It  lasted  seven  days, ...
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... because it rotates really fast. One year is 84 Earth years because it takes a long time to go around the sun. Uranus ...
Jupiter is 90000 miles in diameter. It is 10 times the size of the earth
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... Since Jupiter is a gas planet, it doesn't have a surface. This means that nothing can land on the planet because there is nothing solid to land on. The clouds that make up Jupiter are swirling around the planet, by winds that average over 322 kilometers. The winds create an pattern of storms.. So ...
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The Jovian Planets Sizes of Jovian planets compared to the Earth

... • Theory 1: a large moon strayed too close to its planet as a result of an impact. Problem: such an unlikely event would have to have happened to all of the Jovian planets • Theory 2: they formed from leftover chunks of rocks and ice that condensed into a disk of gas around the planet. Problem: thes ...
Solar system
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... place even somewhat like Earth. Our home planet is the only one we know of with large amounts of liquid water, room temperature climates, comfortable surface pressure, and ample natural resources. In short, Earth is still the only place in the universe we know of that can support life as we know it. ...
The Solar system
The Solar system

... Saturn's rings are made up of billions of pieces of rocks and dust. Saturn has the lowest density of all the planets in the solar system. Saturn is the second largest planet in the Solar System other than Jupiter. It is mostly made up of hydrogen and helium gas.  Saturn's rings are the only one ...
The affects of the Jovian planets
The affects of the Jovian planets

... • All the Jovian Planets have rings made from small chunks of rock and ice that have been broken off of larger objects in collisions. -These are pulled together by the strong gravitational pull of the planets • The Jovian Planets act as shields, protecting earth and other objects in the solar system ...
The solar system - MissWilsonastrounit
The solar system - MissWilsonastrounit

... 7) Earth’s Moon Why do we always see the same side of the moon from Earth? ...
Astronomical Figures
Astronomical Figures

... *considered the father of modern planetary science for his wide ranging studies of the solar system. *established the atmosphere of Saturn's moon, Titan, and discovered Saturn's moon, Miranda, and Neptune's Nereid. Kuiper's prediction of comets traveling near the orbit of Neptune, the Kuiper belt. ...
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Planets

... There were 13 planets. The 9 we are aware of (includes Pluto) and Ceres, Vesta, Juno, and Pallas. They were found in between Mars and Jupiter. One by one, they found many more objects like the 4 “new planets”. So, they changed them from “planets” to “dwarf planets” and identified their location as t ...
Trans Neptunian Objects (TNOs)
Trans Neptunian Objects (TNOs)

... There are many icy/rock objects (planetesimals) in the Kuiper Belt and an area called the Scattered Disc. If one of these has an orbit that crosses inside the orbit of Neptune, the object becomes classified as a Trans Neptunian Object (TNO). Pluto is the biggest TNO. Some of the Kuiper Belt Objects ...
Structure & Formation of the Solar System
Structure & Formation of the Solar System

... • It is by far the largest object in the Solar System. 700 times more massive than all of the other objects in the Solar System put together. • It is composed mostly of Hydrogen and Helium gas and traces of many other elements. • The Sun spins on its axis counter-clockwise. ...
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Naming of moons

The naming of moons has been the responsibility of the International Astronomical Union's committee for Planetary System Nomenclature since 1973. That committee is known today as the Working Group for Planetary System Nomenclature (WGPSN).Prior to its formation, the names of satellites have had varying histories. The choice of names is often determined by a satellite's discoverer; however, historically some satellites were not given names for many years after their discovery; for instance, Titan was discovered by Huygens in 1655, but was not named until 1847, almost two centuries later.Before the IAU assumed responsibility for astronomical nomenclature, only twenty-five satellites had been given names that were in wide use and are still used. Since then, names have been given to 129 additional satellites: 45 satellites of Jupiter, 43 of Saturn, 22 of Uranus, 11 of Neptune, 5 of Pluto, 1 of Eris, and 2 of Haumea. The number will continue to rise as current satellite discoveries are documented and new satellites are discovered.At the IAU General Assembly in July 2004, the WGPSN suggested it may become advisable to not name small satellites, as CCD technology makes it possible to discover satellites as small as 1 km in diameter. To date, however, names have been applied to all moons discovered, regardless of size.
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