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______ is our ONLY source of information for distant objects (the broader universe)
Light
What is light?
an electromagnetic wave that behave like a particle
Nothing travels faster than the speed of
light
Repeat distance
Wavelength
Visible light has ___ wavelengths
small
Frequency is measured in
Hertz
The speed of light in a vacuum is
300,000 km/s
The formula for speed of light is?
Wavelength x frequency
Colors to which the human eye is sensitive is referred to as the ______ with the color determined by the lights ______
visible light spectrum, wavelength
The longest visible wavelength
Red, 700nm
The shortest visible wavelength
Violet 400nm
Electromagnetic Spectrum is made up of
radio waves, microwaves, infrared gamma rays, UV rays, x rays
Shortest wavelength in the Electromagnetic Spectrum is
gamma rays
What are ways light interacts with matter?
Emission, Absorption, Transmission, Reflection/Scattering
Stars __ light
emit
An example of lights interaction with matter determining what we see is the answer to "Why is the Earth blue?'
The Earth's atmosphere scatters blue light more effectively than red light because blue wavelengths are shorter
The sun appears red at sunset because?
The sun is at a different angle to the blue light is reflected through space instead of through the earth
Passing light through a prism makes a
Spectrum
The word spectrum means
Phantom in Latin
You can learn more about an object when it has a _____ and ______
emission line and absorption line
When passing light through a prism, you can notice what in the spectrum?
the missing elements
Hot objects produce a
continuous spectrum
What is a continuous spectrum?
light emitted at all wavelengths
What is created when atoms in gas absorb light if certain wavelengths producing lines in the spectrum
absorption line spectrum
What is created when atoms in a gas cloud reemit absorbed light energy at the same wavelengths at which they absorbed it?
Emission line spectrum
We can determine what things from the light of an object?
Chemical composition, temperature, and doppler motion
When matter is heated, electrons move _____ levels
energy
Electrons moving either up or down energy levels creates a unique
spectral fingerprint
A spectral fingerprint is expressed as _____ and _____ lines in an object's spectrum
emission and absorption
Temperature and ____ correlate
color
What color is the coolest?
red
As you increase the temperature of an object the wavelength gets
shorter
Wien's law states
increasing temperature decreases wavelength
Absolute 0 on the Kelvin scale means
the particles have completely quit moving
The sun supposedly can reach up to
15 million Kelvin
When matter becomes so hot, the particles are no longer repulsed by each other because they are moving so fast they can slam into each other and become
one
Short wavelength have a _____ pitch
higher
Long wavelength have a _____ pitches
lower
Redshift occurs when an object is moving ______ from you
away
Blue shift occurs when an object is moving _____ you
toward
If we could see an asteroid crashing into earth it would be
blue shift
If we could see an asteroid moving away from earth it would be
red shift
The light from all other galaxies in the universe outside of the milkyway is red shifted meaning
the galaxies are moving away from us
A light year is a unit of
distance NOT time
Speed of light is
300,000 km/s
The sun is _____ away from earth
8.3 light MINUTES
The moon is _____ away from earth
1.3 light SECONDS
We can only ever see how the sun looked
8 minutes ago
The further we look away from our planet, the further we
travel back in time
We cannot see more than 13.7 billion light years away from earth because we would be looking back to
before the universe was formed
The most important thing a telescope can do is
collect more light than your eyes
Telescopes use _______ or _______ to focus light
mirror, lenses
What is needed for Collecting Power of a telescope?
Light
What is needed for Focusing Power of a telescope?
Mirrors or Lenses
What is needed for Resolving Power of a telescope?
Lenses and Magnification
________ telescopes are better
Reflecting
________ telescopes take light from a distant object and bend in down to your eye piece
Refracting
Refracting telescopes are best for objects that
produce their own light
_________ telescopes collect more light and bounce them down to your eyepiece off of mirrors
Reflecting
Why do we put telescopes in space?
To avoid light pollution, to avoid turbulence/twinkling, and because our atmosphere absorbs most of the electromagnetic spectrum
Light from stars twinkle because
it has to make its way through our moving atmosphere
Telescopes are NOT put in space to be closer to the stars, the whole point is to
get away from our atmosphere
Cold gas clouds radio in the ____ waves
radio
Dust clouds radiate in the _____ waves
infrared
Hot gasses around black holes emit _____ waves
x rays
We can see a lot of the galaxy by being able to detect
the non visible wavelengths
Hubble telescope is pretty much just
a ground base telescope, but better
EVE captures ____ light
UV
Spizer captures
heat/infrared
Chandra captures
X rays
James Webb Telescope 2018 will work in ____ and produce ____
infrared, optical pictures
Hubble telescope has been in space since
the early 2000s
The sun is very similar to
all the other stars in the universe
Our sun is just special to us because
it is closest to us
Our sun is just
a ball of hot gas bound by gravity
Our sun is made of
hydrogen and helium and trace amount of other elements like calcium and potassium
What keeps our sun going?
fusion
Every second our sun converts 600 million tons of Hydrogen into 596 million tons of Helium, that missing 4 million of material
powers and heat ours planet and solar system
Our sun shines not because it is on fire, but because it is powered by
nuclear energy FUSION
Atomic number
number of protons in nucleus
Atomic Mass
number of protons and neutrons in nucleus
Taking protons and neutrons in the nucleus of an item and combining them to make something bigger
Fusion
Splitting the atom
fission
The atomic bomb is
fission
Our sun uses what (fusion or fission)
Fusion
Our sun is a ____ mass star
low
Proton Proton Chain
fusing four hydrogen nuclei into one Helium nuclei
What does the equation of Proton Proton Chain look like?
4H =>1 He + energy
We can figure out the rate of fusion in our sun by counting
neutrinos
CNO cycle
high mass main sequence stars fuse H to He at a higher rate using Carbon, Nitrogen, and Oxygen as catalysts/fuel (runs out of fuel faster)
Our sun is stable because of
fusion which pushes out on the gravity
Gravity and Fusion create ____ with our sun
gravitational equilibrium
A flow of charged particles from the surface of the sun
Solar Wind
Outermost layer of the Sun's atmosphere
Corona
Middle layer of the sun's solar atmosphere that is the first part in the visible light spectrum
Chromosphere
Visible surface of the sun, 5,800K
Photosphere
Why is the sun yellow?
because the surface/Photosphere is 5,800K
Energy is transported upward by rising hot gas
Convection Zone
Energy Transported upward by photons
Radiation Zone
10% most centralized part of the sun and is the hottest, energy generated by nuclear fusion 15 million K
Core