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Newton’s Laws of Motion #1: A body continues at rest or in uniform motion in a
straight line unless acted upon by a force. Why doesn’t the soccer ball move on its own? What causes a soccer ball to roll to a stop on the grass?
Newton’s Laws of Motion #2: The amount of change in a body’s motion is
proportional to the force acting on it, and along the same direction as the force.
F (force) = m (mass) × a (acceleration)
If I kick the ball this way
It will move in the same direction
If I kick the ball harder,
It will go faster
The more massive the body, the more force you need to
change its motion
Need a lot of force to move a bowling ball
Only need a little force to move a ping-pong ball
Newton’s Laws of Motion
#3: When one body exerts a force on a second body, the second body exerts an equal and opposite force back on the first body.
What’s happening at the moment
when I kick the soccer ball?
Hint: Think about what would happen if you kicked the ball really hard with no shoes on.
Gravity Lecture Tutorial: Pages 29-31
• Work with a partner or two • Read directions and answer all questions carefully.
Take time to understand it now! • Come to a consensus answer you all agree on before
moving on to the next question. • If you get stuck, ask another group for help. • If you get really stuck, raise your hand and I will
come around.
The Moon and Earth pull on each other with equal strength
and in opposite directions
Earth
Moon
Fg Fg
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You and Earth pull on each other with equal strength and
in opposite directions
Earth
Fg
Fg
The more massive the body, the more force you need to change its motion
Earth
Fg
Fg
Which one will move more: You or Earth?
a (acceleration) = F (force) m (mass)
Light and Matter: Reading Messages from the
Cosmos How do we experience light?
• The warmth of sunlight tells us that light is a form of energy
• We can measure the power, or flow of energy over time, of light in units of watts
• One watt is about the amount of power used to lift an apple over your head in 1 second
Colors of Light
• White light is made up of many different colors
How do light and matter interact?
• Emission • Absorption • Transmission
– Transparent objects let light through – Opaque objects block or absorb light
• Reflection or Scattering
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Reflection and Scattering
Mirror reflects light in a particular direction
Movie screen scatters light in all directions
What is light?
• Light can act either like a wave or like a particle
• Particles of light are called photons
Properties of Waves
• Wavelength is the distance between two wave peaks
• Frequency is the number of times per second that a wave vibrates up and down
wave speed = wavelength x frequency
Light: Electromagnetic Waves
• A light wave is a vibration of electric and magnetic fields
• Light interacts with charged particles through these electric and magnetic fields
Wavelength and Frequency
wavelength x frequency = speed of light = constant
Particles of Light
• Particles of light are called photons • Each photon has a wavelength and a
frequency • The energy of a photon depends on its
frequency
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Wavelength, Frequency, and Energy
λ x f = c λ = wavelength , f = frequency c = 3.00 x 108 m/s = speed of light
E = h x f = photon energy
h = 6.626 x 10-34 joule x s = Plank’s constant
What is the electromagnetic spectrum?
The entire possible range of wavelengths or frequencies light
can have
What is the electromagnetic spectrum? Gamma Rays • Very high frequency
• Very high energy
• Damaging to humans!
-The atmosphere takes care of us…
• Can only be studied from space
• Gamma ray bursts, nuclear reactions
X-rays
• Still pretty high energy
• Not as bad as gamma rays, too much is still bad
• Medical uses
• Can still only be studied from space
• Gas in galaxy clusters, supernova remnants, or the Sun’s corona
Ultraviolet (UV) Light
• Getting closer to visible light!
• Too much is still a bad thing (wear sun block…)
• Visible in supernova remnants and coming from very hot stars
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Visible Light
• Light our eyes can see!
• Wavelengths about as long as bacteria
• About 400-700 nanometers
• Produced in stars
Infrared (IR) Light • We glow in IR light!
• Beyond the range of human sight
• Night-vision goggles
• Given off by planets, some gas clouds, and moons
Radio • Very wide range of wavelengths / frequencies
• Subcategories: TV, AM & FM radio, RADAR, microwaves
• The CMB (cosmic microwave background) glows in microwaves
EM Spectrum Lecture Tutorial: Pages 45-47
• Work with a partner or two • Read directions and answer all questions carefully.
Take time to understand it now! • Come to a consensus answer you all agree on before
moving on to the next question. • If you get stuck, ask another group for help. • If you get really stuck, raise your hand and I will
come around.
Telescopes & Light
• Telescopes gather information from the entire EM spectrum
• Why do some objects glow in IR light? Why do some give off x-rays?
• Interactions between light & matter
Properties of Matter • Structure of matter • Phases of matter • How energy is stored in atoms
How do light and matter interact?
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What is the structure of matter?
Atom Nucleus
Electron Cloud
Atomic Terminology • Atomic Number = # of protons in nucleus • Atomic Mass Number = # of protons + neutrons
• Molecules: consist of two or more atoms (H2O, CO2)
Atomic Terminology • Isotope: same # of protons but different # of
neutrons. (4He, 3He)
What are the phases of matter?
• Familiar phases: – Solid (ice) – Liquid (water) – Gas (water vapor)
• Phases of same material behave differently because of differences in chemical bonds
Phase Changes • Melting: Breaking of rigid chemical
bonds, changing solid into liquid • Evaporation: Breaking of flexible
chemical bonds, changing liquid into gas
• Dissociation: Breaking of molecules into atoms
• Ionization: Stripping of electrons, changing atoms into plasma
How is energy stored in atoms?
• Electrons in atoms are restricted to particular energy levels (electron shells)
Ground State
Excited States
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Energy Level Transitions
• An electron can only go from one level to another, not in between
Allowed Not Allowed
A Simple Atom
• Only 2 energy levels – Ground (E1) – Excited (E2)
• Right now electron is at E1
E1
E2
Nucleus
A Simple Atom
• Excitation – Electron absorbs a
photon and jumps from E1 to E2
– Photon only absorbed if it has energy = (E2-E1)
E1
E2
Nucleus
Photon
A Simple Atom • Ionization
– Electron absorbs a photon and leaves!
– Only works if electron is in higher energy levels
E1
E2
Nucleus
Photon
A Simple Atom
• De-excitation – Electron emits a
photon of energy (E2-E1)
– Electrons like to be in the ground state
E1
E2
Nucleus
Photon
Spectrum: Wavelength vs. Intensity
• Visible:
• Intensity vs. wavelength plot:
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They show the same information “Dips” in color = black lines
Dips in intensity
Continuous Spectrum
• All wavelengths, no breaks • Rainbows!
Emission Spectrum
• Bright, individual lines • Also called bright-line spectrum • Electrons are moving to lower energy levels,
emitting photons of light
Absorption Spectrum
• Rainbow with dark lines on top • Also called dark-line spectrum • Atoms in the cloud are absorbing photons, moving to higher
energy levels
Kirchhoff’s Laws
I. A hot, dense substance will give off continuous spectrum
II. A hot, low-density gas will give off an emission spectrum
III. A cool, low-density gas in front of a continuous-spectrum source will give off an absorption spectrum
Chemical Fingerprints • Each type of
atom has a unique set of energy levels
• Each transition corresponds to a unique photon energy, frequency, and wavelength
Energy levels of Hydrogen
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Chemical Fingerprints • Downward
transitions produce emission lines
• Upward transitions produce absorption lines
Chemical Fingerprints
• Each type of atom has a unique spectral fingerprint, due to spacing of energy levels
Light and Atoms Lecture Tutorial: pages 63-67
• Work with a partner or two • Read directions and answer all questions carefully.
Take time to understand it now! • Come to a consensus answer you all agree on before
moving on to the next question. • If you get stuck, ask another group for help. • If you get really stuck, raise your hand and I will
come around.