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Origin of the Solar System

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Rotating cloud of matter contracts under its own gravity and flattens into a disk ... Contracts and forms spinning disk. Spins faster leaving blob in center ... – PowerPoint PPT presentation

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Title: Origin of the Solar System


1
Origin of the Solar System
2
Early Hypotheses
  • Catastrophic
  • Passing star hypothesis
  • Passing star pulled material off of our star to
    form solar system

3
Early Hypotheses
  • Evolutionary
  • Nebular hypothesis
  • Rotating cloud of matter contracts under its own
    gravity and flattens into a disk
  • Solar nebula hypothesis
  • Planets form at the same time from the same cloud
    as the star.

4
Forming a Theory
  • Hypothesis, theory or model?
  • Once data is collected from observable planetary
    systems, a theory can be developed from the
    hypothesis and data collected.

5
Solar Nebular Theory
  • Dust cloud
  • Disruption supernova
  • Contracts and forms spinning disk
  • Spins faster leaving blob in center
  • Planetesimals formed by two processes.
  • Condensation
  • Accretion
  • Temperature influences type of planet formation

6
Solar Nebular Theory
  • Nuclear reactions in core of star caused by
    radiation pressure cause star to heat up and
    become more luminous -expels gas and dust cocoon.
  • Planetesimals collide and grow gas giants
    already formed
  • After 100 millions years, planets in solar system
    are formed.

7
Solar Nebular evidence
  • Predicts many stars have planetary systems
  • Observations of extrasolar planets
  • Wobble of star produces shift in spectrum
  • Changes in brightness of star
  • Many stars appear to have disk of gas and dust.

8
Properties of Solar System
  • Disk shape
  • Common rotation and revolution.
  • Two types of planets
  • Terrestrial
  • Jovian
  • Ring systems for all Jovian planets.
  • Space debris such as asteroids, comets and
    meteoroids
  • Age of solar system from Moon, Mars, and
    asteroids.
  • Age of solar system from Sun.

9
Our Solar System
10
Our Solar System
  • How do we compare planets?
  • Density mass/volume
  • Density of water 1000 kg/m3
  • Density of rock 2000-4000 kg/m3
  • Atmosphere and chemical composition
  • Magnetic field strength
  • Number of moons
  • Mass
  • Size
  • Orbits
  • Rotation and Revolution periods

11
Our Solar System
  • Two categories of planets
  • Terrestrial
  • Mercury
  • Venus
  • Earth
  • Mars

12
Our Solar System
  • Two categories of planets
  • Jovian
  • Jupiter
  • Saturn
  • Uranus
  • Neptune

13
Terrestrial Jovian
  • Closely spaced orbits Largely spaced orbits
  • High density Low density
  • Few moons Many moons
  • Rocky Gaseous
  • Weak magnetic fields Strong magnetic fields
  • Small mass Large mass
  • Small radius Large radius
  • Long rotation period Short rotation period
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