Title: Stars
1Stars Galaxies
2Metric Review
SI Base Unit for Length
meter (m)
1000m 1km
1mile 1.6km
3Distance in Space
In space, distances are much larger than anything
we deal with on earth.
example the distance from Earth to the Sun is
93,000,000miles
Scientists have designated this distance 1
astronomical unit (AU).
1AU 93,000,000mi 149,668,992km
4Distance in Space
Even AU is a very small distance in space.
Normally, distance is measured in
Light Years
- the distance light is able to travel in one
year.
5the Speed of Light
light travels at a rate of 300,000km/s
or 300,000,000m/s
or 186,000mi/s
6One Light Year (ly) is the distance light can
travel in a years time
1ly 9,460,000,000,000km
or 6,000,000,000miles
or 63,239AU
7The closest star in our galaxy to the Sun,
Proxima Centauri, is 4.3ly away!
or 271,930AU
or 25,277,549,200,800 miles
8An even larger measurement of space distance is a
parsec (pc)
1pc 3.26ly
or 206,161AU
or 19,163,909,394,100 miles
9The distance from Earth to the center of our
Milky Way galaxy is 8,000 parsecs.
10Light
- energy that moves as a wave.
11Speed of Light
- all light travels at the same speed
- 300,000,000m/s
12Understanding Waves
13Understanding Waves
wavelength
- the distance between two crests
14Understanding Waves
frequency
- the number of crests
that pass a given point in one second.
15Which set of waves has the highest frequency?
wavelength?
16Frequency and wavelength are inversely related
- as wavelength increases, frequency decreases
- as wavelength decreases, frequency increases
17Light Energy
high energy light
- short wavelengths, high frequencies
low energy light
- long wavelengths, low frequencies
18Which set of waves has the highest energy?
19Light energy exists at every wavelength and
frequency this range of values is called the
Electromagnetic
Spectrum
20Visible Light
- we can only see a small fraction of all the
light frequencies that exist
700nm
400nm
nm nanometer 0.000000001m
21Less Energetic Light
(wavelengths longer than visible light)
Infrared
wavelengths 700nm to 1mm
- invisible, but felt as heat
22Less Energetic Light
(wavelengths longer than visible light)
Microwaves
wavelengths 1mm to 10cm
- used to cook food and for communication
23Less Energetic Light
(wavelengths longer than visible light)
Radio waves
wavelengths 10cm to 100km
- used for communication
24More Energetic Light
(wavelengths shorter than visible light)
Ultraviolet
wavelengths 400nm to 10nm
- emitted by the sun, harmful to tissue
25More Energetic Light
(wavelengths shorter than visible light)
X rays
wavelengths 10nm to 0.01nm
- used for medical diagnosis, emitted by objects
in space
26More Energetic Light
(wavelengths shorter than visible light)
Gamma rays
wavelengths 0.001nm to 0.000001nm
- emitted by objects in space and nuclear
reactions highly dangerous
27Light Review
Does light with longer or shorter wavelengths
have more energy?
28Light Review
Does light with higher or lower frequencies have
more energy?
29Light Review
700nm
400nm
What color of light has the most energy? the
least?
30the Doppler Effect
What happens to the sound of a train or car as it
approaches you? as it passes you and keeps going?
31the Doppler Effect
As a train approaches, its sound waves are
bunched up ahead of it. What does this do to
the wavelength?
32the Doppler Effect
As a train moves away, its sound waves are
stretch out behind it. What does this do to
the wavelength?
33the Doppler Effect
- The same is true for light
- as light waves approach, their wavelengths are
shorter - as they move away, their wavelengths are longer
34the Red Shift
- light moving away has longer wavelengths
- these wavelengths are lower energy or shifted
toward the red end of the spectrum
35the Blue Shift
- light traveling toward Earth has shorter
wavelengths - these wavelengths are higher energy or shifted
toward the blue end of the spectrum
36As astronomers began to study other galaxies,
they began to notice that the light from all of
them was shifted toward red. What does this mean?
37Scientists concluded that the universe is
expanding all galaxies are moving apart. This
led them to the
BIG BANG THEORY
38The Story of the
BIG BANG THEORY
The universe began 15-20 billion years ago
39All of the matter in the universe was squished
into one body as small as an egg
40The intense heat and pressure caused the matter
to explode outward
41The intense heat and pressure caused the matter
to explode outward
42The intense heat and pressure caused the matter
to explode outward
43The intense heat and pressure caused the matter
to explode outward
44The intense heat and pressure caused the matter
to explode outward
45The intense heat and pressure caused the matter
to explode outward
46The intense heat and pressure caused the matter
to explode outward
47The intense heat and pressure caused the matter
to explode outward
48The intense heat and pressure caused the matter
to explode outward
49The intense heat and pressure caused the matter
to explode outward
50The intense heat and pressure caused the matter
to explode outward
51The intense heat and pressure caused the matter
to explode outward
52The intense heat and pressure caused the matter
to explode outward
53The intense heat and pressure caused the matter
to explode outward
54The intense heat and pressure caused the matter
to explode outward
55The intense heat and pressure caused the matter
to explode outward
56The intense heat and pressure caused the matter
to explode outward
57The intense heat and pressure caused the matter
to explode outward
58The intense heat and pressure caused the matter
to explode outward
59The intense heat and pressure caused the matter
to explode outward
60With nothing to stop it, matter and energy shot
in all directions
61With nothing to stop it, matter and energy shot
in all directions
62With nothing to stop it, matter and energy shot
in all directions
63With nothing to stop it, matter and energy shot
in all directions
64With nothing to stop it, matter and energy shot
in all directions
65With nothing to stop it, matter and energy shot
in all directions
66With nothing to stop it, matter and energy shot
in all directions
67With nothing to stop it, matter and energy shot
in all directions
68Matter would have spread evenly throughout the
entire universe, but
69Gravity caused it to begin forming clumps
70INTERMISSION
- the force of attraction between all objects in
the universe
gravity
- the more mass an object has, the larger its
gravitational attraction
71back to our story...
72gigantic clumps of matter eventually formed into
galaxies
73smaller clumps within these large clumps formed
stars and planets
74even as galaxies form and exist, they are
continuing to race away from one another.
75What about the universe today?
76Possibility 1
we live in an open universe
77an open universe
Galaxies will continue to race outward until
they lose all their energy.
Billions of years from now, the universe will
become cold and dark.
78Possibility 2
we live in a closed universe
79a closed universe
Gravitational attraction will one day slow down
the galaxies and then cause them to start moving
back together.
Billions of years from now, all the matter will
be pressed together again, and there could be
another Big Bang.
80- most scientists think our universe is a Closed
Universe and believe that it bangs and then
contracts back onto itself over and over.
81the end...
for now
82Supporting the Theory...
1. red shift
- we know from observing light that galaxies are
moving apart.
83Supporting the Theory...
2. background radiation
- if energy spread evenly during the Big Bang,
then there should be about the same amount
everywhere scientists have observed this
consistent background energy all over the
universe.
84Supporting the Theory...
3. quasars
- the most distant objects we can see are 12
billion light years away
- that means the light of these star-like
bodies is 12 billion years old when we see it!
85Supporting the Theory...
3. quasars
- they are too small to be galaxies, but they
have 100 times more energy than any galaxy
- some scientists think they are pre galaxies
that existed soon after the Big Bang
86Star light, star bright...
Things we can learn from starlight
- star size
- what stars are made of
- temperature of stars
- brightness of stars
87Star
Medium Star(the Sun)
Size
Neutron Star
Giant Star
White Dwarf Star
Supergiant Star
88Star Size
Medium Stars
- the sun and stars 10 times larger or smaller
than it
- most of the stars in the universe
- the suns diameter is 865,000miles or
109 times bigger than Earth!
89Star Size
Giant Stars
- 10 to 100 times larger than the sun
Supergiant Stars
- up to 1000 times larger than sun!
- if it were our sun, it would reach past Mars!
90Star Size
White Dwarf Stars
- smaller across than the continent of Asia
Neutron Stars
- about 16 kilometers (or 10miles) across!
91question
If you hold a bright spotlight and a dim
flashlight next to each other, which appears
brighter?
92question
If a dim flashlight is shining right next to you,
and a bright spotlight is ½ mile away, which one
appears brighter?
93The brightness of stars that we can see from
Earth is called
Apparent Brightness
- depends on the stars size, temperature, and
distance from Earth.
94Scientists can calculate a stars
Absolute Brightness
- the brightness stars would have if they were
all the same distance from Earth.
95Some stars change brightness. These are called
Variable Stars
- ones that also change size are called pulsating
variables.example Polaris (the North Star)
changes with a 4 day cycle
96Composition of Stars
(what stars are made of)
- all elements give off particular colors of
light when burning in a flame.
- astronomers separate and study these colors
with a spectroscope
97Composition of Stars
(what stars are made of)
Examplesodium looks yellow burning in a flame
- with a spectroscope, we can see that sodium is
giving off two lines of yellow
98Composition of Stars
(what stars are made of)
Sodium Example
99Composition of Stars
(what stars are made of)
- all elements give off a unique set of lines
when seen through a spectroscope like a
fingerprint
- by studying the lines of starlight, we can tell
what elements are burning in the star
100Composition of Stars
(what stars are made of)
- the most common element in stars is hydrogen
makes up 60 to 80 of stars - helium is the second most common
- together, hydrogen and helium make up 96 to 99
of all stars
101question
What color is a cold electric stove? How can you
tell when it gets very hot? Which is hotter a
yellow or blue flame?
102Star Temperature
- just as different colors indicate different
temperatures for hot objects on Earth, a stars
color tells us about the temperature at the
surface of the star.
103(No Transcript)
104Star Temperature
- the surface temperature of a star, however,
does not tell us how hot the star is on the
inside.
105Star Temperature
Example our Sun is a yellow star with a surface
temperature of 6,000oC but the temperature at
its core is 15,000,000oC!
106Star light, star bright...
How do stars shine anyway?
107question
What were the two most common element in stars?
108Star Light
- the gravity inside the core of a star is so
strong that it forces hydrogen atoms to smash
into each other and join up to make helium atoms
109this process is called
Nuclear Fusion
- when the hydrogen atoms collide, they release
huge amounts of energy
110Nuclear Fusion
- this energy is released as heat and light,
which is why stars are hot and shine
111Nuclear Fusion
How much energy does fusion release?
- the fusion of 1 liter of hydrogen atoms gives
off more energy than burning one ton of coal
112Nuclear Fusion
How often does fusion occur?
- in our Sun, enough hydrogen atoms fuse every
second to fill a cube with each length the size
of a football field
113Nuclear Fusion
Does fusion occur on Earth?
- only if people make it happen the only use we
have right now is the hydrogen bomb, but someday
it may be an unlimited, clean source of power