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Our Universe

Published on Nov 19, 2015

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PRESENTATION OUTLINE

OUR UNIVERSE

A PRESENTATION By Mark Roster

OUR SOLAR SYSTEM

  • a collection of small and large bodies that orbit the sun
  • Consists of nine different planets
  • A planet is a spherical body that orbits the sun
  • Closest planets to sun are terrestrial planets
  • Earth, Mars, Venus, and Mercury

COMPOSITION OF TERRESTRIAL PLANETS

  • Small
  • Dense
  • Rocky

GAS GIANT PLANETS

  • Far away from the sun
  • Consists of Saturn, Jupiter, Neptune, and Uranus
  • Have small Rocky cores
  • Thick gassy atmospheres
  • Have rings made of dust, ice, and rock

DWARF PLANETS

  • Pluto is a dwarf planet (it is still in our solar system)
  • Dwarf planets are made out of rock and ice
  • There are five other Dwarf planets

THE UNIVERSE

  • Contains everything
  • is defined as space, matter and all energy in it
  • Has many stars
  • A light year is the distance that light travels in a year

SCALE DISTANCES OF THE UNIVERSE

  • Light travels through space at about 9.5 trillion km in 1 year
  • closest star to the Earth and sun is Proxima Centauri
  • Distance from Proxima Centauri to Earth is about 4.3 light-years

TIME OF SPACECRAFT TRAVEL

  • Our fastest spacecraft would take 75,000 years to reach Proxima Centauri

LIFE CYCLE OF HIGH MASS STARS

  • Hydrogen cycle ends
  • Other types of fusion begin
  • Involves fusion of nuclei in elements heavier than carbon
  • Star expands and becomes supergiant

CAUSE OF SUPERNOVA

  • A supernova is a gigantic explosion when a high mass star throws its outer layers

DEATH OF A HIGH MASS STAR

  • Core of star contracts under its own gravity
  • Contraction leads to increase in core's temerature
  • Energy is transferred to thin shell of surrounding hydrogen
  • Fusion radiates energy outward causing star to grow larger
  • Star begins ejecting matter, rapidly lose mass until core remains, the rest depends on star's mass

HOW TO USE HERTZSPRUNG-RUSSELL DIAGRAM

  • Hottest stars will be located on the left side of the diagram and are blue
  • Coolest stars will be located on the right side of the diagram and are red
  • Brightest stars on the top, dimmest stars on the bottom

THE MAIN SEQUENCE (H-R DIAGRAM)

  • Region of the diagram where stars spend most of their lives
  • Stars within this band are fusing hydrogen activley
  • These stars are called main sequence stars
  • Our sun is a main sequence star
  • Fusion ends, sun becomes a giant, moves to upper right, outer layers are lost, sun becomes white dwarf

THE END