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Our Universe
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Published on Nov 19, 2015
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PRESENTATION OUTLINE
1.
OUR UNIVERSE
A PRESENTATION By Mark Roster
2.
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
3.
COMPOSITION OF TERRESTRIAL PLANETS
Small
Dense
Rocky
4.
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
5.
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
6.
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
7.
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
8.
TIME OF SPACECRAFT TRAVEL
Our fastest spacecraft would take 75,000 years to reach Proxima Centauri
9.
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
10.
CAUSE OF SUPERNOVA
A supernova is a gigantic explosion when a high mass star throws its outer layers
11.
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
12.
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
13.
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
14.
THE END
Mark Roster
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