Forming Planets CEA Saclay simulation.

Slides:



Advertisements
Similar presentations
The Story of Our Solar System
Advertisements

How all the stuff in the solar system was created.
ASTR100 (Spring 2008) Introduction to Astronomy The Formation of Planets Prof. D.C. Richardson Sections
This Set of Slides This set of slides covers age and formation of solar system, exoplanets. Units covered: 33, 34.
Origin of the Solar System
1 Chapter 2 Creation of Oceans. 2 Supporting Evidence for the Big Bang Edwin Hubble discovered spreading of galaxies. Cosmic background radiation (the.
1 a little physics SESAME Astronomy Winter 2011 week 2.
Formation of the Solar System  This is a picture of the Eagle Nebula taken by the Hubble Telescope in  A nebula is a cloud of gas and dust in space.
The Origin of the Solar System
Pre-solar nebula Protoplanetary disk: condensation and accretion Solar wind (beginning of fusion) Collisions continue Planetary migration (orbits shifting)
CH 25.5 Solar System Formation
Any theory about the origin of the solar system must explain why all of the planets’ orbits lie more or less in a plane and all of the planets orbit the.
Origin of Solar System Lecture 15. Key Properties of our Solar System Any theory of the origin of the solar system must be able to explain following key.
Formation of our solar system: The nebular hypothesis (Kant, 1755) Hydrogen (H), He (He) and “stardust” (heavier elements that were formed in previous.
© 2010 Pearson Education, Inc. Formation of the Solar System.
NOTES: The Solar System: Origin: the nebular theory fits most of the facts. The nebular theory: 1. The Big Bang produced lumpy clouds--COBE satellite.
Formation of the Solar System
Recap: Death of Stars: Low and Medium Mass Red Giant Main Sequence Star Planetary Nebula White Dwarf Black Dwarf ?? Red Dwarf Low Mass Medium Mass.
THE BIRTH OF THE SOLAR SYSTEM. MODELS OF THE SOLAR SYSTEM Geocentric - Everything revolved around earth. (Aristotle and Ptolemy) Heliocentric – Planets.
A Solar System is Born 4/25/14 IN: What do you think the planets are made of? 19-1a pgs
Universe The universe is all existing matter and space considered as a whole. The universe is all existing matter and space considered as a whole.
Solar System Formation Solar System Comprised of a star and the planets that orbit the star Binary – Two stars at center of system –Eclipsing is when.
Ch 15 – The Formation of the Solar System Modeling the origin of the solar system.
Solar System Formation Solar System Comprised of a star and the planets that orbit the star Binary – Two stars at center of system –Eclipsing is when.
2 nd Law of Thermodynamics 1 st Law – conservation of energy 2 nd Law – no cyclic process which converts heat entirely into work is possible. Can’t build.
The Formation of the Solar System The Nebular Hypothesis.
CH 25.5 Solar System Formation Objectives: How did our solar system form? What evidence supports our ideas?
Solar System Formation
Fig. 2-CO, p. 40. Fig. 2-1, p. 41 Fig. 2-2, p. 42.
A disk of dust and gas orbiting a newly formed star.
The Formation of the Solar System. The Nebular Hypothesis The Solar System formed ~ 4.6 billion years ago Evidence from:  meteorites ( billion.
FORMATION OF THE SOLAR SYSTEM The Stellar Nebula Hypothesis.
25.5. Any theory about the origin of the solar system must explain why all of the planets’ orbits lie more or less in a plane Why all of the planets orbit.
Our Solar System & Exoplanets (Chapter 15). Student Learning Objectives Identify and locate objects in our solar system Describe planet formation processes.
The solar system Topic # 2 Term # 2 The Local System.
Unit 2 Lesson 2 Gravity and the Solar System Copyright © Houghton Mifflin Harcourt Publishing Company.
Introduction to The Sun Our sun is a star located at the center of our Solar System. It is a huge, spinning ball of hot gas and nuclear reactions that.
Our Solar System.
Our Solar System and Its Origin
Formation of the Solar System and The Universe
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
Our Solar System and Its Origin
Formation of the Solar System
The Solar System 1 star 8 planets several dwarf planets many moons
Solar System Formation
Chapter 11 The Formation of Stars
check activities page Kirkwood link for times and dates
Any theory about the origin of the solar system must explain why all of the planets’ orbits lie more or less in a plane and all of the planets orbit the.
Friday 5/18/18 Notebook Entry: If you could travel to any object in our Universe where would you go and WHY?
Our Solar System & Exoplanets
Formation of the Solar System
Daily Routine Sit in your appropriate seat quietly
Formation of a Solar System
Monday 5/22/17 Fill out your assignment notebook for the week for your period. Notebook Entry: If you could travel to any object in our Universe where.
The Birth of a Solar System
Our Solar System.
A cloud of space dust or gas.
A Solar system is born.
History of Our Solar System
A presentation by Jessica Booth
Origin of the Earth.
Chapter 6 Our Solar System and Its Origin
2. THE SOLAR SYSTEM’S EARLY HISTORY
3A Objectives Describe the nebular theory in detail.
Our Solar System & Exoplanets
Formation of the Solar System
Formation of Our Solar System
Star Formation CH. 5.
A SOLAR SYSTEM IS BORN Chapter 16 – 1 Part 1.
Topic # 2 Term # 2 The Local System
Presentation transcript:

Forming Planets CEA Saclay simulation

New Worlds How long does it take to make a solar system? A. 1 million years. B. 10 million years. C. 100 million years. D. 1 billion years.

Gases in Space Supernova stars explode and create clouds of gas and dust. The gas includes hydrogen, helium, nitrogen, oxygen, etc. Crab Nebula, 1000 years old

Formation of the Sun Stars are formed by a gas/dust cloud contracting due to gravity. Orion Nebula, 1 million years old

Protoplanetary Disk Gases begin to swirl around the star. Inward from gravity Outward from heat Angular momentum is conserved. HR 4796A, 10 million years old

Collisions and Accretion From 10 to 100 million years, dust begins to stick together. This is called accretion, and is aided by gravity. Solid accretion toward star Gas accretion outward Radio image of Epsilon Eridani, 500 million years old

Migration There is more gas and dust near the star for formation. A planet moving outward can slow the spin of a star. Conservation of angular momentum Protoplanet 6 MJ, 2 million years old Keck telescope, 2011

Frost Line The heat of a star melts minerals that are close. Frozen “ices” dominate at greater distances. U Hawaii