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Our Solar System

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Order of the planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto ... Jupiter, Saturn, Uranus, and Neptune. Pluto doesn't quite fit ... – PowerPoint PPT presentation

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Title: Our Solar System


1
Chapter 23 "Our Solar System"
2
Facts about our Solar System
  • 99.85 of all the mass in our solar system is
    contained in the sun, which means all of the
    planets only add up to .15 of the mass within
    our solar system!!!
  • All planets move in the same direction around the
    sun counterclockwise.
  • My Very Educated Mother Just
  • Sold Us Nine Pizzas
  • Order of the planets Mercury, Venus, Earth,
    Mars, Jupiter, Saturn, Uranus, Neptune, Pluto

3
Planets Overview
  • Terrestrial Planets
  • Small and rocky, made from solid material
  • Mercury, Venus, Earth, and Mars
  • Jovian Planets
  • Huge gas GIANTS, made from dense gaseous material
  • Jupiter, Saturn, Uranus, and Neptune
  • Pluto doesnt quite fit into either
    category?!?
  • Why? It is terrestrial, but also composed of
    gaseous solid material (ice) due to its extreme
    distance from the sun.

4
Terrestrial vs. jovian
  • Size the most obvious difference between the
    two types
  • Terrestrial small compared with Jovian planets
  • Jovian giants
  • Density
  • Terrestrial densities 5 times the density of
    water
  • Jovian densities only 1.5 times that of water
  • According to its density,
  • Saturn would float on water!
  • Chemical makeup, and rate of rotation are two
    other ways in which the two types of planets
    differ.

5
Planetary data table
6
Interiors of the Planets
  • The substances that make up the planets are
    divided into three groups
  • 1. Gases hydrogen and helium
  • 2. Rocks silicate minerals and metallic iron
  • 3. Ices ammonia, methane, carbon dioxide, and
    water
  • Terrestrial planets are dense so they contain
    more of the rocky and metallic substances
  • Jovian planets are less dense so they contain
    large amounts of gases and ice.
  • They do have substantial amounts of rocky and
    metallic materials in their core however.

7
The Atmosphere of the Planets
  • A planets ability to keep an atmosphere is
    dependent on its mass and temperature.
  • The more mass a planet has, the great ability it
    has to retain an atmosphere (due to gravity!)
  • The hotter a planet is, the less ability it has
    to retain an atmosphere because the heat burns up
    the gases!
  • Jovian planets have thick atmospheres of
    hydrogen, helium, methane, and ammonia.
  • Terrestrial planets, including Earth, have
    very thin atmospheres in comparison to the Jovian
    planets.

8
The Formation of the Solar System
  • The Nebular Theory
  • The sun and planets formed from a rotating disk
    composed of dust and gases.
  • Nebula - cloud of gas and/or dust in space
  • Planetesimals - small, irregularly shaped bodies
    formed by colliding matter
  • Three Steps to the Nebular Theory
  • Step 1 The nebula cloud began rotating.
  • Step 2 Particles within the cloud condensed and
    formed into planetesimals
  • Step 3 Planetesimals continued to condense and
    formed into planets and moons.

9
The nebular theory
10
Evidence to Support the Nebular Theory
  • Orbits of the planets lie nearly in the same
    plane with the sun at the center
  • The planets all revolve in the same direction

Pluto is the only planet that does not orbit the
sun in the same plane, this is another idea that
supports that Pluto was once a moon of Neptune.
11
The Big Bang Theory
  • The most widely accepted theory explaining the
    formation of the universe.
  • Why? Because it is the only scientifically
    supported theory that we currently have
  • Step 1 All matter and energy in the universe was
    once located in a single dense point called a
    singularity.
  • Step 2 A HUGE explosion occurred!
  • Step 3 Matter and energy were propelled outward
    in all directions as the universe began to expand.

Step 4 Matter began to condense - forming
galaxies and these galaxies continue to move
outward today.
12
How The Big Bang Theory came to be
  • In 1927 Belgian priest Georges Lemaître proposed
    that the universe began with the explosion of an
    early atom.
  • His proposal came after observing the red shift
    (objects moving away from us) in distant nebulas.
  • Years later, Edwin Hubble found experimental
    evidence to help justify Lemaître's theory.
  • He found that distant galaxies in every direction
    are going away from us with speeds proportional
    to their distance.
  • NASA named the Hubble Space Telescope after Edwin
    Hubble due to his great contributions to
    astronomy!

13
Evidence for the Big Bang Theory
  • The Big Bang Theory explains why distant galaxies
    are traveling away from us at great speeds.
  • This theory also predicts the existence of cosmic
    background radiation the energy glow left over
    from the explosion.
  • The Big Bang Theory received its strongest
    confirmation when this radiation was discovered
    in 1964 by Arno Penzias and Robert Wilson, who
    later won the Nobel Prize for this discovery.

14
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15
Evidence for the Big Bang Theory
  • What continues to support this theory today?
  • The universe is currently expanding as observed
    by the movement of cosmic background radiation.
  • Most of the most distant stars observed to be in
    red-shift (they are moving away from Earth)
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