The Formation of the Solar System. The Nebular Hypothesis The Solar System formed ~ 4.6 billion years ago Evidence from:  meteorites (4.5-4.6 billion.

Slides:



Advertisements
Similar presentations
Formation of the Solar System. Our solar system was born from the collapse of a great cloud of gas. A nebula that formed from hydrogen gas and the remnants.
Advertisements

Chapter 8 Formation of the Solar System
Formation of the Solar System
ASTRONOMY 161 Introduction to Solar System Astronomy Class 13.
Chapter 6 Our Solar System and Its Origin
Origin of Our Solar System
ORIGIN OF THE SOLAR SYSTEM Chapter 12. MAJOR PROPERTIES OF THE SOLAR SYSTEM l Each planet is isolated about twice as far from the Sun as its inward neighbour.
ASTR100 (Spring 2008) Introduction to Astronomy The Formation of Planets Prof. D.C. Richardson Sections
Copyright © 2012 Pearson Education, Inc. The Formation of the Solar System.
This Set of Slides This set of slides covers age and formation of solar system, exoplanets. Units covered: 33, 34.
The Solar System Section 23.1 Pg
1 Chapter 2 Creation of Oceans. 2 Supporting Evidence for the Big Bang Edwin Hubble discovered spreading of galaxies. Cosmic background radiation (the.
Chapter 8 Welcome to the Solar System. 8.1 The Search for Origins Our goals for learning What properties of our solar system must a formation theory explain?
“How Did Our Solar System Form?” Ch Space is not really empty. There is gas and dust in between the stars. This gas is mostly hydrogen, left over.
Our Solar System and Its Origin. What does the solar system look like?
Chapter 6 Formation of Planetary Systems Our Solar System and Beyond
Our Solar System It's nice and all, but…... Each planet is about twice as far from the Sun as the planet before it.
Chapter 8 Formation of the Solar System
Formation of the Solar System Q of D: How did the solar system form?
Chapter 6: Formation of the Solar System
Chapter 8 Welcome to the Solar System. 8.1 The Search for Origins Our goals for learning What properties of our solar system must a formation theory explain?
Lecture Outline Chapter 6: Formation of the Solar System © 2015 Pearson Education, Inc.
CH 25.5 Solar System Formation
Survey of the Solar System
Solar Nebula Hypothesis
AST 111 Lecture 15 Formation of the Solar System.
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.
Chapter 8 Formation of the Solar System. 8.1 The Search for Origins Our goals for learning: What properties of our solar system must a formation theory.
Formation of our solar system: The nebular hypothesis (Kant, 1755) Hydrogen (H), He (He) and “stardust” (heavier elements that were formed in previous.
Solar System Formation And the Stuff that was Left Over.
Grades will be posted in MyUCFGrades Quiz for Ch. 6 has been posted and is due next Mon. night (as usual)
© 2010 Pearson Education, Inc. Formation of the Solar System.
© 2010 Pearson Education, Inc. Solar System Overview Earth, as viewed by the Voyager spacecraft.
Formation of the Solar System
Copyright © 2012 Pearson Education, Inc. Chapter 6 Formation of Planetary Systems: Our Solar System and Beyond.
Exam 1 next time !!!! Bring your #2 pencils!!!. Where did the solar system come from? Nebular theory.
Formation of the Solar System. A model of the solar system must explain the following: 1.All planets orbit the sun counterclockwise 2.All planets orbit.
© 2010 Pearson Education, Inc. Chapter 8 Formation of the Solar System.
Formation of the Solar System
Origin of Our Solar System
Our Solar System and Its Origin. 6.4 The Formation of Planets Our Goals for Learning Why are there two types of planets? Where did asteroids and comets.
THE BIRTH OF THE SOLAR SYSTEM. MODELS OF THE SOLAR SYSTEM Geocentric - Everything revolved around earth. (Aristotle and Ptolemy) Heliocentric – Planets.
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.
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?
Formation of the Solar System
The Gas Giant (Jovian) Planets Jupiter Uranus Saturn Neptune The Terrestrial (Rocky/Metal) Planets Mercury Earth Venus Mars.
Fig. 2-CO, p. 40. Fig. 2-1, p. 41 Fig. 2-2, p. 42.
The Formation of Our Solar System The Nebular Hypothesis.
© 2010 Pearson Education, Inc. Chapter 4 Origin of the Solar System.
Origin and Evolution of the Solar System. 1.A cloud of interstellar gas and/or dust (the "solar nebula") is disturbed and collapses under its own.
Nebular Theory 9/4/2015. © 2005 Pearson Education Inc., publishing as Addison-Wesley Nebular Theory of the Solar System 1.Large bodies in the Solar System.
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.
The solar system Topic # 2 Term # 2 The Local System.
Our Solar System and Its Origin
Chapter 8 Formation of the Solar System
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
Our Solar System and Its Origin
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.
Daily Routine Sit in your appropriate seat quietly
Formation of a Solar System
A Solar system is born.
Chapter 6 Our Solar System and Its Origin
2. THE SOLAR SYSTEM’S EARLY HISTORY
Our Solar System and Its Origin
3A Objectives Describe the nebular theory in detail.
NEBULAR THEORY.
Topic # 2 Term # 2 The Local System
Presentation transcript:

The Formation of the Solar System

The Nebular Hypothesis The Solar System formed ~ 4.6 billion years ago Evidence from:  meteorites ( billion years old)  moon rocks (~4.0 billion years old)  Earth Rocks(~3.9 billion years old) sedimentary minerals ~ 4.2 by

The Beginning All stars, including our sun come from nebulae Nebulae are the remains of old stars that have exploded Nebulae contain all of the natural elements Eggs in nebula are where stars are born

The Big Spin - An external force causes the “egg” to spin counterclockwise The gas cloud initially rotated slowly Gravity pulls the cloud inward Conservation of Angular Momentum As the cloud begins to shrink, it spins faster Think of a ice skater Quickly rotating objects become flattened.

The contraction of the solar nebula made it spin faster and heat up. (Compressed gas gets hotter.) Temperature of solar nebula: > 2000 Kelvin near Sun; < 50 Kelvin far from Sun.

The Disc Over 90% of the material was in the center Less than 10% of the material was in the disc surrounding it SUN Planets, comets, Asteroids, Moons

The Formation of the Planets Accretion: particles in the disc condensed forming ice and rock these particles continued to collide and combine into large planetesimals Continuing to spin, compress and collide the planets and moons formed

Accretion of Planetesimals Many smaller objects collected into just a few large ones

Inside the frost line: Too hot for hydrogen compounds to form ices. Outside the frost line: Cold enough for ices to form. Fig 9.5 Why two types of planets?

The Formation of the Sun Within the center of the disc: Compression and Friction Temperature Increase Sun “turned on” Hydrogen fusion began

The Solar Wind blew excess gas toward the outer planets leaving the inner planets rocky ending the period of planet formation

What makes this a good hypothesis? All of the planets travel in the same direction (counterclockwise) All of the planets are in the same plane Angular Momentum is clearly understood Nebula are very real and very common

How do we explain “exceptions to the rules”?

Heavy Bombardment Leftover planetesimals bombarded other objects in the late stages of solar system formation

Odd Rotation Giant impacts might explain the different rotation axes of some planets

Origin of Earth’s Water Water may have come to Earth by way of icy planetesimals from outer solar system

Captured Moons Unusual moons of some planets may be captured planetesimals

How do we explain the existence of Earth’s moon?

Giant Impact Hypothesis

Giant Impact Giant impact stripped matter from Earth’s crust Stripped matter began to orbit Then accreted into Moon

Was our solar system destined to be? Formation of planets in the solar nebula seems inevitable But details of individual planets could have been different