Formation of the Solar System Carin Miranda SMS 6-1 2008.

Slides:



Advertisements
Similar presentations
Solar System. Sources t/sun/sun.htmlhttp://csep10.phys.utk.edu/astr162/lec t/sun/sun.html
Advertisements

Life Cycle of Stars. Omega / Swan Nebula (M17) Stars are born from great clouds of gas and dust called Stars are born from great clouds of gas and dust.
Solar System.
Structure & Formation of the Solar System
Ch Formation 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.
A Solar System Is Born Science Journal Entry Section 1
How our Solar System (and Moon) came to be…. Learning Objectives Be able to explain – How our solar system and moon came to be.
An Introduction to Astronomy Part VI: Overview and Origin of the Solar System Lambert E. Murray, Ph.D. Professor of Physics.
Formation of the Solar System
Our Solar System Chapter 28.
Our Solar System It's nice and all, but…... Each planet is about twice as far from the Sun as the planet before it.
Formation of the Solar System Chapter 27 page 684-
STRAND #1 – EARLY ASTRONOMY 1. Name the scientist that said the sun was the center of the solar system (and not the Earth) AND name the scientist that.
Chapter 27: Planets of the solar system
JOURNAL #17 – THE SOLAR SYSTEM 1.What is the order of the planets from the Sun outward? 2.If during a solar eclipse the moon must be between the Sun and.
THE STAR OF OUR SOLAR SYSTEM Solar radiation travels from the sun to the earth at the speed of light. The speed of light is km/s.
Formation of the Solar System
Survey of the Solar System
Notes The Sun. Stars an object that produces it own energy, including heat and light.
Astronomy The Solar System, Planetesimals, The Sun, Nuclear Fusion, Planetary Movement.
THE SUN. CLASSIFICATION OF THE SUN Class G Color Yellow Surface Temperature 5,000 – 6,000 ºC Elements hydrogen and helium Greek word for Sun is Helios.
Unit 2 Lesson 2 Gravity and the Solar System
MOTION OF THE PLANETS For many centuries, most people believed that the Earth was the center of the universe. In this geocentric model, the Sun, the planets.
Space and Astronomy Study Guide Standard 1
Formation of our solar system: The nebular hypothesis (Kant, 1755) Hydrogen (H), He (He) and “stardust” (heavier elements that were formed in previous.
Formation of the Solar System Chapter 3. A Solar System is Born Section 1 Vocabulary Nebula Solar Nebula.
Chapter 20 – The Formation of the Solar System
ACTIVITY 1. For distances to stars and galaxies, astronomers use a unit called a light- year. A light-year is the distance that light travels in a year.
The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these.
Life Cycle of Stars Birth Place of Stars:
Ch. 28 The SUN The Structure of the Sun 3 Parts 1.Core 2.Inner Zones Radiative Zone Convective Zone 3.Atmosphere.
Formation of the Solar System. The Age of the Solar System We can estimate the age of the Solar System by looking at radioactive isotopes. These are unstable.
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.
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.
EXPLAIN THE NEBULAR HYPOTHESIS OF THE ORIGIN OF THE SOLAR SYSTEM. DESCRIBE HOW THE PLANETS FORMED DESCRIBE THE FORMATION OF THE LAND, THE ATMOSPHERE, AND.
The Sun-Earth-Moon System. What is the moon? The moon is a natural satellite of Earth This means that the moon orbits Earth.
Chapter 27 Formation of the Solar System The sun and all of the planets and other bodies that revolve around the sun.
Formation of Solar System
Ch. 20 and 21.  Our solar system has been here for awhile  5 billion years!  It formed from a solar nebula  Clouds of dust in space that combined.
The Solar System. Solar system – consists of the sun and, planets, and other objects that orbit the sun Nebular model – states that the sun and planets.
11.2 The Sun and the Planets Our Sun, an average star in the universe, is the center of our solar system. Planets, moons, asteroids and comets revolve.
Warmup  What is the line of latitude that cuts through the center of the earth?  What is ZERO degrees longitude?  What is 180 degrees longitude?
27-1OBJECTIVES Explain the nebular hypothesis of the origin of the solar system Describe how the planets formed Describe the formation of the land, the.
The Formation of The Solar System. Nebulas Clouds that are a mixture of gases mainly helium, hydrogen, and dust made of elements such as carbon and iron.
Chapter 15 Formation of the Solar System Section 1 A Solar System Is BornA Solar System Is Born Section 2 The Sun: Our Very Own StarThe Sun: Our Very Own.
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.
Unit 2 Lesson 2 Gravity and the Solar System
Our Solar System.
12-2 Notes How Stars Shine Chapter 12, Lesson 2.
Survey of the Solar System
Common Assessment #10 The Sun And Other Stars.
Our Solar System.
The Lives of Stars.
The Lives of Stars.
Formation of a Solar System
A Solar System is Born.
Our Solar System.
A Solar system is born.
History of Our Solar System
The Sun and Earth.
Jeopardy Q $100 Q $100 Q $100 Q $100 Q $100 Q $200 Q $200 Q $200
Origin of the Universe.
The Vastness of the Universe
Formation of Our Solar System
A SOLAR SYSTEM IS BORN Chapter 16 – 1 Part 1.
Do Now: What do you already know about the different kinds of planets in our solar system? Do you already know something specific about them? Write.
Topic # 2 Term # 2 The Local System
Presentation transcript:

Formation of the Solar System Carin Miranda SMS

A Solar System is Born The solar system is composed of the sun, Earth, 7 other planets, and other cosmic bodies. Solar Nebula-dust and gas that clump together to form interstellar clouds.

What Holds it All Together Gravity pulls it together. Pressure pushes it apart. Because of these two forces nebula remain stable.

From Planetesimals to Planets Solar Nebula begins to collapse. It rotates, flattens, and gets warmer in the center. Bits of dust and gas begin sticking together forming planetesimals. Small planetesimals begin bumping into larger planetesimals and they combine. Remaining dust and gas is eventually removed leaving the planets.

Planets Outer plants are made of gas (except for Pluto which is no longer a planet). Inner planets are made mostly of rocky material because the heat from the sun.

Craters and Comets Collisions with smaller planetesimals and other cosmic bodies have left the inner planets with many craters. If the planetesimal is icy we call it a comet.

Planetary Motion The solar system is 4.6 billion years old. Rotation-Spinning on axis. 24 hours. Revolution-the motion of a planet around the sun. 365 days. Orbit- the PATH around the sun.

Newton’s law of Universal Gravitation Every object in the universe attracts every other object in the universe with a force dependent on its mass and the square of the distance between them. Example if you move objects twice as far apart the gravitational attraction between them will decrease by a factor of 2 X 2=4.

What Keeps Objects Being Pulled by Gravity from Crashing Into Each Other?

The Sun It is a star. The Center of our Solar System. Gives us light and warmth. Made of gas

Layers of the Sun Corona-sun’s outer atmosphere. Only visible during a total solar eclipse. Chromosphere-below the corona. Only visible during a total solar eclipse. Photosphere-Visible layer of the sun. Convective zone-Gases circulate in convective currents. Radiative zone-very dense region below the convective zone. Core-center of the sun. Where the sun’s energy is produced.

Layers of the Sun

Energy Production Burning for 4.6 billion years. Nuclear Fusion- Process by which two or more nuclei join together. Energy is released.

Activity on the Sun’s Surface Sunspots-cool dark spots on the sun. Solar Flares-giant storms on the surface of the sun.

The Earth Takes Shape Gravity gives planets their spherical shape. Heat causes part of the interior of Earth to remain molten.

Layers of the Earth Heavier elements sank into the core. It is in the center of the Earth. The mantle forms the middle layer Less dense objects rose to the outer layer forming the crust.

Layers of the Earth

Earth’s Atmosphere Today the atmosphere is 21% oxygen, 78% nitrogen, and 1% argon. Early in Earth’s history the planet may have been molten. Impacts with comets brought elements such as carbon, hydrogen, nitrogen, and even water.