'Terrestrial planets' diaporamas de présentation

The Search for Life in the Solar System

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The Solar System - Its Origin and Early Development

The Solar System - Its Origin and Early Development. Sun and eddy. Solar System. The Solar System consists of the Sun and the other celestial objects gravitationally bound to it: the eight planets, three dwarf planets and their 165 known moons. 4 terrestrial planets or inner planets

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Terrestrial Planets

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Detecting Extrasolar Planets

Detecting Extrasolar Planets. Radial Velocity Measurements. First Proposed in 1952. Radial Velocity Variations. https://upload.wikimedia.org/wikipedia/commons/5/59/Orbit3.gif. Radial Velocity Variations. Radial Velocity Variations.

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THE MOON

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Solar System Objects

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Chapter 23 Objectives

Chapter 23 Objectives. List the differences between Jovian and Terrestrial planets. Describe the major characteristics of all planets. Discuss possible theories on the formation of the universe. List and define the other minor members of the solar system. . NEED TO KNOW.

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A Planetary Overview

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Ch. 9 and 10: the other Terrestrial Planets

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The Terrestrial Planets, Part II

The Terrestrial Planets, Part II. The Earth. EARTH. Physical Data. Diameter: 12,756.3 km Mass: 5.976x10 27 g Density: 5.518 g/cm 3 Rotation Period: 23.9 hours Tilt of Axis: 23.5 o Surface Temperature: 200-300 K. Physical Data. Orbital Semi-Major Axis: 1.49x10 11 m (1 AU)

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Our Solar System

Our Solar System. Chapter 28. Formation of the Solar System. 28.1. A collapsing interstellar cloud. Stars and planets form from interstellar clouds They appear dark because of dust blocking out the light The light can cause it to glow, or even become heated

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Solar System

Solar System. Introduction. The Solar System consists mostly of empty space!. The Sun 1 M ? The Nine Eight Planets ( ? 0.001 M ? ) Asteroids and Rocky Debris (Negligible mass) Comets (?). Planets in the Solar System come in two varieties. TERRESTRIAL. and.

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Solar System History Ch 9

Solar System History Ch 9. Big Bang Theory Solar Nebula Planetesimals Terrestrial Planets. Big Bang Hypothesis.

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Pages 193 - 207

Pages 193 - 207. Mariner 10: Mission to Mercury 1973 - 1974. Mariner 10 mosaics of Mercury (inbound = left; outbound = right. *. *. *. *. *. *. Average speed of gas molecules increase with increasing T. The average speed of gas molecules decreases with increasing mass.

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Terrestrial planets vs. Jovian planets

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The terrestrial planets

The terrestrial planets. What is terrestrial planet?. The four inner planets are considered terrestrial planets Terrestrial means made of rock Inner planets have a rocky composition compared to the outer planets. Mercury. Closest planet to the sun 0.39 AU from sun 0 moons

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Structure & Formation of the Solar System

Structure & Formation of the Solar System. What is the Solar System? The Sun and everything gravitationally bound to it. There is a certain order to the Solar System. This gives us information on its formation. The planets to scale with a portion of the Sun visible in the background.

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Lindsley, 8/99

High P and T at center of Solar nebula cause hydrogen atoms to fuse together to form helium Solid particles condense and collide to form planetesimals which accrete into planets. Lindsley, 8/99. Solar system: outer jovian planets, inner terrestrial planets, Pluto the oddball. Lindsley, 8/99.

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The Inner Planets

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