'Gas giants' diaporamas de présentation

EARTH SCIENCE FINAL

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2 pt

Earth. Moon. By the Numbers. Planets. Miscellaneous. 1pt. 1 pt. 1 pt. 1pt. 1 pt. 2 pt. 2 pt. 2pt. 2pt. 2 pt. 3 pt. 3 pt. 3 pt. 3 pt. 3 pt. 4 pt. 4 pt. 4pt. 4 pt. 4pt. 5pt. 5 pt. 5 pt. 5 pt. 5 pt. The position of the Earth from the sun. What is third ?.

812 views • 51 slides

2 pt

Earth. Moon. By the Numbers. Planets. Miscellaneous. 1pt. 1 pt. 1 pt. 1pt. 1 pt. 2 pt. 2 pt. 2pt. 2pt. 2 pt. 3 pt. 3 pt. 3 pt. 3 pt. 3 pt. 4 pt. 4 pt. 4pt. 4 pt. 4pt. 5pt. 5 pt. 5 pt. 5 pt. 5 pt. The position of the Earth from the sun. What is third ?.

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WHAT IS THE TRUTH?

WHAT IS THE TRUTH?. Click for next question. Which of the following is true?. The more force applied to a sound, the louder it is. When the Moon is larger than half but less then full it is called a waxing Moon. Click on the TRUE statement. This Statement is NOT TRUE !. Try Again.

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The Origin of the Solar System

Its Structure and Evolution. The Origin of the Solar System. How it all Began. Aristarchus of Samos was the first to speculate a heliocentric model of the cosmos. Miko?aj Kopernik was the first to give it a mathematical background.

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The Moons of the Gas Giants

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Interiors of Worlds and Heat loss

Interiors of Worlds and Heat loss. Differentiation -materials separate into layers. How do we learn about planetary interiors?. Measure moment of inertia & average density Observe seismic events Study planetary magnetic fields.

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Extra-Solar Planets

Extra-Solar Planets. Exoplanet - A large body orbiting a star other than the Sun. Topics in this lecture: Review of planet formation The Habitable Zone Basic properties of discovered exoplanets Hot Jupiters Super-Earths. How to make a planet . Large, cool cloud of gas and dust

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The Solar System

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The Outer Solar System

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Introduction to the Solar System

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How Big is the Universe?

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Evolution of the Solar System

Evolution of the Solar System. Matt Rogers AT350 9 September 2003. Overview. Evolution of a star Interstellar Nebula Formation of protostar and protostellar nebula Evolution of early sequences and dissipation of protostellar nebula. Overview (continued). Evolution of planets

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Chapter 20 Sections 1-3

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Restless Earth and Varves

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SOLAR SYSTEM FORMATION

SOLAR SYSTEM FORMATION. THE NEBULAR THEORY. 6- Steps to Form a Solar System. Step 1: Solar Nebula. Huge cloud of cold gas and dust. Spinning slowly. Step 2: Protosun. The solar nebula condenses into a dense central region and a less-dense outer region. Begins to spin faster and flatten.

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Planetary Ring Systems

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Touring our Solar System

Touring our Solar System. An Overview of our Planets. Terrestrial planets are small and rocky Mercury, Venus, Earth, and Mars Jovian planets are gas giants Jupiter, Saturn, Uranus, Neptune. An Overview of our Planets.

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Inner vs. Outer Planers

Inner vs. Outer Planers. By Bryan Nisbet. Inner Planets. Also called terrestrial planets F ew moons N o ring systems 3 of the 4 have atmosphere Has an asteroid belt. Outer Planets. Jovian Planets 99 percent of the mass known to orbit the Sun

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NEPTUNE!

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