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Newton s Laws of Motion Newton s Laws of Motionjfielder/11506week6slides.pdf10/3/11 1 Newton’s...

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10/3/11 1 Newtons Laws of Motion #1: A body continues at rest or in uniform motion in a straight line unless acted upon by a force. Why doesnt the soccer ball move on its own? What causes a soccer ball to roll to a stop on the grass? Newtons Laws of Motion #2: The amount of change in a bodys 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 Newtons 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. Whats 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 F g F g
Transcript

10/3/11

1

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

10/3/11

2

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

10/3/11

3

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

10/3/11

4

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

10/3/11

5

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?

10/3/11

6

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

10/3/11

7

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:

10/3/11

8

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

10/3/11

9

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.


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