'Solar system formation' diaporamas de présentation

Chapter 8 Formation of Planetary Systems Our Solar System and Beyond

Chapter 8 Formation of Planetary Systems Our Solar System and Beyond. Where did the solar system come from?. According to the nebular theory, our solar system formed from a giant cloud of interstellar gas. ( nebula = cloud). Evidence from Other Gas Clouds.

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3-6 Asteroids

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Solar System Dynamics

Solar System Dynamics. Instructor Alice Quillen Seminar class AST570 TR12:30-1:45pm B+L315 http://astro.pas.rochester.edu/~aquillen/ast570/ Dynamics of circumstellar disks, planetary systems, solar system formation and evolution, exoplanets Overlap with Galactic Dynamics

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EART160 Planetary Sciences

EART160 Planetary Sciences. Francis Nimmo. Last Week - Volcanism. How and why are melts generated? Increase in mantle potential temperature; or Reduction in solidus temperature (e.g. water); or Thinning of the lithosphere How do melts ascend towards the surface?

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Chapter 2

Chapter 2. Spectroscopy / Review . Outline. Test Wednesday Spectroscopy Check posted grades!. Misc. If you received a C- or below (or any grade you have questions about) for your mid-term grade, please come by my office to discuss your situation. Lab notes. No Inside lab this week

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Solar System Formation

Solar System Formation. The processes by which stars and planets form are active areas of research in modern astrophysics The formation of our own solar system is central to the first half of our course, and important to the second half as well when we study the formation of stars.

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The Mythology Of Modern Dating By Paul Nethercott Creation Ministries International June 2014

The Mythology Of Modern Dating By Paul Nethercott Creation Ministries International June 2014. www.creation.com. Introduction How reliable is radiometric dating? We are repeatedly told that it proves the Earth to be billions of years

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The Sun and the Origin of the Solar System

The Sun and the Origin of the Solar System. Mid-sized, G-type main sequence star Distance: 1 AU = 150 million km away Size: Actual radius 700,000 km = 100 Earths Temperature, Luminosity (surface) T = 6000 K http://www.nasa.gov/multimedia/videogallery/index.html.

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How did the Solar System form?

How did the Solar System form?. 3. What are the broad general characteristics or physical features of our Solar System and how do they illuminate Solar System formation?. How did the Solar System form?. 4. How did the terrestrial planets form and why is the Solar System differentiated? .

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Chapter 6 The Solar System: Comparative Planetology 1

Chapter 6 The Solar System: Comparative Planetology 1. Learning Goals. What is comparative planetology ? Describe the scale & structure of our solar sytem Summarize the basic differences between the terrestrial & jovian planets

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A Planetary Overview

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EART160 Planetary Sciences

EART160 Planetary Sciences. Francis Nimmo. Last Week. Volcanism happens because of higher temperatures, reduced pressure or lowered solidus Conductive cooling time t = d 2 / k Planetary cooling leads to compression Elastic materials s = E e.

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Rocks Older Than Solar System By Paul Nethercott Creation Ministries International April 2013

Rocks Older Than Solar System By Paul Nethercott Creation Ministries International April 2013. www.creation.com. Introduction How reliable is radiometric dating? We are repeatedly told that it proves the Earth to be billions of years

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GEOL 208 Lecture 1b

CON U

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Overview of the Solar System

Overview of the Solar System. The solar system consists of the Sun, eight known planets (+ Pluto!), many satellites of the planets, and a large number of interplanetary bodies (comets, asteroids, meteoroids, interplanetary dust particles)

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Solar system formation

Adam Marth -Earth Science. Solar system formation. Energy can neither be created nor destroyed; Only Transformed. Claims the origin of the solar system came from a rotating cloud of interstellar gas (or a nebula) Believed to be remnants of dead star systems long before the birth of ours

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Solar System Formation

Solar System Formation. This is a nebula. This is where stars are forming. . These are little solar nebulae!. Proto-sun and accretion disk. Accretion. Dus grains stick together through electricity to form planetessimals.

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Test question 7.1

Test question 7.1. In the solar system, the temperature difference between terrestrial planets and gas giants is due to vTheir distance from the sun, xThe number of their moons xThe length of their days xTilt of their spin. Test question 7.2.

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