Concepts of Science Exam 1 Study Guide

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159 Terms

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Johannes Kepler
\-Took over after Tycho Brahe’s death

\-Established three laws based on the data he collected
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Kepler’s First Law
Planets move in elliptical orbits with sun at 1 focus
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Kepler’s Second Law
Line connecting planet/sun sweeps out equal areas in equal times

\-planets move slower when further away from the sun and faster when closer to sun
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Kepler’s Third Law
Square of period (time planet takes to go around sun) is proportional to cube of the semimajor axis (distance from center through focus
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Galileo Galilei
\-First to record observations with a telescope

\-Supported a sun-centered universe
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Speed
The distance an objects travels divided by the time it takes to travel that distance
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Velocity
The same value as speed, but includes information about direction (60 m/s northeast) because it is a vectoral quantity
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Velocity Equation
distance/time
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Speed Equation
distance/time
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Acceleration Equation
(final velocity-initial velocity)/time
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Velocity of an Accelerating Object
constant a \* time
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Acceleration Constant (at 90 degrees)
9\.8 m/s^2

\*This only applies to objects on Earth’s surface
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Distance Traveled Equation
1/2 \* acceleration \* t^2
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Time Equation
distance/velocity
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Newton’s First Law
Moving objects will continue moving in straight lines at constant speed, & stationary objects will remain at rest, unless acted on by an unbalanced force
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Newton’s Second Law
\-The acceleration produced on a body by a force is proportional to the magnitude of the force and inversely proportional to the mass of the object

\-The greater the force, the greater the acceleration

\-The more massive an object, the smaller the acceleration
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Force Equation
mass \* acceleration
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Newton’s Third Law
\-For every action there is an equal and opposite reaction

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\-Interacting objects exert equal but opposite forces upon each other

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\-The results of the interactions of the objects may be different

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\-The equal and opposite forces do not cancel because they are acting on different objects
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Momentum Equation
mass \* velocity
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Conserved
A physical quantity doesn’t change
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Newton’s Universal Law of Gravitation
Between any two objects in the universe there is an attractive force (gravity) that is proportional to the square of the distance between them
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Force of Gravity (N) Equation
(Gravitational Constant \* mass 1 \* mass 2)/distance^2
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Universal Gravitational Constant (G)
6\.67 \* 10^-11 N \* (m^2/kg^2)
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g
\-Gravitational acceleration on Earth’s surface

\-9.8 N/kg
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Equation for Work (joules)
force \* distance
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Energy
The ability to do work
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Power
The rate at which work is done
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Power (watts) Equation
work/time or energy/time
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Energy Equation
power \* time
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Kinetic Energy Equation
1/2 \* mass \* speed^2
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Potential Energy
Energy waiting to be released
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Potential Energy Equation
mass \* g \* height
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Heat is transferred from…
hot to cold
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Hot objects have…
high kinetic energy
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Types of Wave Energy
Water waves, sound waves, seismic waves, electromagnetic radiation (light)
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Sound waves are created when…
atoms/molecules in the air are set in motion.
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Seismic waves carry…
potentially destructive energy of moving atoms/molecules in the Earth that can be unleashed in earthquakes.
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Electromagnetic radiation has energy stored in the form of…
alternating electric and magnetic fields.
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Is mass a form of energy?
Yes
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Equation for potential energy of objects at rest
Energy = mass \* (the speed of light)^2

or

E = m\*c^2
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First Law of Thermodynamics
In an isolated system, the total amount of energy is conserved.
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Open Systems in Thermodynamics
There is exchange of matter and energy with surroundings.
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Closed or Isolated Systems in Thermodynamics
There is no exchange of matter and energy with surroundings
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Fahrenheit
Daniel Fahrenheit used the coldest mixture of ice and salt water he could produce as 0 degrees
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Celsius
0 degrees is the freezing point of water

100 degrees is the boiling point of water
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Kelvin
Uses the same temperature distribution as Celsius, but 0 Kelvin is -273 degrees C
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Fahrenheit to Celsius
(1.8 \* degrees C) + 32
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Celsius to Fahrenheit
(degrees F/1.8) - 32
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Conduction
\-Movement of heat by atomic scale collisions

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\-Heat flows at different rates in objects depending on their thermal conductivity

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\-Metal is a great heat conductor and wood is a great heat insulator
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Conduction Example
• If a piece of metal is heated on one end, atoms there begin to move faster

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• By colliding with neighboring atoms, some of the kinetic energy is transferred & atoms further away progressively begin to move faster
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Convection
Transfer of heat by bulk motion of a gas/fluid
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Convection Example
\- Boiling water

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– Water near bottom of pot expands becomes less dense

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– Cooler, more dense water above sinks

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– Hot water rises in bulk, carrying faster moving molecules



– Heat then transferred to air & cycle repeats
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Are things that are bad heat conductors good insulators?
Yes
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Radiation
\-Transfer of heat by electromagnetic waves

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\-It can be transmitted through empty space
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Second Law of Thermodynamics
\- The behavior of energy is regular and predictable

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\-Heat energy can flow by conduction, convection, and radiation

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– Heat will not flow spontaneously from a cold to a hot body

* Doesn’t mean it is impossible for heat to flow from cold to hot object, just that it won’t occur spontaneously & requires the input of additional energy

– You cannot construct an engine that does nothing but convert heat to useful work

* Some energy is lost to surroundings

– Every isolated system becomes more disordered with time
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Efficiency
Term to quantify amount of energy loss in an engine
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Efficiency Equation
((𝑇ℎ𝑜𝑡 ―𝑇𝑐𝑜𝑙𝑑)/𝑇ℎ𝑜𝑡) × 100
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Ordered vs. Disordered System
• In an ordered system, objects are arranged in a regular predictable pattern

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• In a disordered system, objects are arranged randomly

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• Because there are more ways to arrange things randomly, disorder is more probable & easily
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Entropy
\- Term given to quantify the amount of a system’s disorder

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\- 2nd Law can be restated that the entropy of an isolated system remains constant or increases
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Static Electricity
\-Force between charged objects (charges) was named electricity from Greek word for amber (electro)

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\-This force can be attractive or repulsive, which is very different from gravity (which is always attractive)

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\-Electrons can be transferred to other objects giving them a negative charge while the original thing now has a positive charge so they now stick together
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Coulomb’s Law
Force between 2 electrically charged objects is proportional to the product of their charges divided by the square of the distance between them
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Coulomb’s Law Equation
Force = (Charge 1 \* Charge 2)/distance^2
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How many poles does every magnet have?
2; north and south
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What happens when a magnet is placed on a magnetic field?
It will rotate and align its poles along the field. The density of the lines indicate the strength of the field.
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Electric Circuit
An unbroken path of material that carries electricity that is made of electrical conductors
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What are the three components of an electric circuit?
– A source of energy (e.g., a battery)

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– A closed path through which current flows

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– A device that uses the electrical energy
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Current
\- Amount of charge that flows per unit time

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\- Measured in amps

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\- 1 amp of current = 1 coulomb of charge per second
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Voltage
Amount of “electrical pressure” in circuit
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Electrical Resistance
\-Describes the ease with which current flows in a wire

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\-Measured in Ohms
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Ohm’s Law
The greater the resistance in a wire, the more electrical kinetic energy is lost as heat
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Ohm’s Law Equation
voltage = current \* resistance
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Power Equation
Power = current \* voltage
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Series Circuit
two or more loads are linked along a single loop of wire
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Parallel Circuit
different loads are situated on different wire loops
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Maxwell’s Equations State
– There are no magnetic monopoles in nature

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– Coulomb’s law: like charges repel, unlike attract

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– Electrical phenomena can be produced by magnetic effects

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– Magnetic phenomena can be produced by electrical effects
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Wavelength
The distance between crests (highest points) of adjacent waves
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Frequency
The number of wave crests that go by a given point per unit time (cycles per second or hertz, Hz)
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Period
The time between adjacent waves (inverse of frequency, measured in seconds per wave)
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Velocity (waves)
The speed & direction of the wave
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Velocity of a Wave Equation
wave velocity = wavelength \* frequency
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Amplitude
The height of the wave crest above the undisturbed position (midpoint between crest and trough)
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Transverse Wave
motion of the medium is perpendicular to the wave direction
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Longitudinal Wave
motion of the medium is parallel to the wave direction
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Electromagnetic Waves
\-consist of alternating electric and magnetic fields that are perpendicular to each other and the direction the wave is moving

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\-can move through empty space without a medium

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\-light is an example which slows down when passing through matter
\-consist of alternating electric and magnetic fields that are perpendicular to each other and the direction the wave is moving

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\-can move through empty space without a medium

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\-light is an example which slows down when passing through matter
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Interference
\-The process by which waves from different sources overlap and affect each other

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\-The observed height at point where two waves come together is the sum of the individual amplitudes

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\-Waves can enhance one another/add constructively (constructive interference) or cancel each other out (destructive interference)
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The Doppler Effect
\-When a source emits a wave, stationary observers will detect the same pitch

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\-If source is moving, the detected pitch will increase/ decrease as the source moves towards/away from the observer
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Electromagnetic Spectrum
Maxwell’s equations predicted electromagnetic waves beyond what was seen should be possible
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Radio
\- Have longest wavelengths (from bigger than Earth to few meters long)

\- Frequencies from kilohertz to hundreds of megahertz

\- Broadcasters transmit information in narrow frequency ranges (radio stations)

\- Radio waves carry signals encoded by amplitude or frequency modulation
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Microwave
• Have wavelength range from 1 meter to 1 millimeter

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• Travel readily in air but absorbed/reflected by rocks/metal objects

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• Used in aircraft radar & cell phones

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• Many satellites broadcast signals in microwave range

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• Can be used to stimulate the rotation of molecules (e.g., H2O)

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• Microwave ovens accelerate electrons to generate microwaves and heat water in food
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Infrared
• Have wavelength range from milimeters to microns

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• Corresponds to the vibrational energy levels of molecules

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• Warm objects emit infrared radiation

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• Infrared detectors can be used for missile guidance systems and for night vision

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• Can be used to find heat leaks in buildings

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• Eyes of many insects & nocturnal animals sensitive to infrared light and use it to see in the dark
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Visible
• Contains the colors of the rainbow from 700 nanometers (red) to 400 nanometers (violet) light

• Sunlight is especially intense in this region

• Eyes of diurnal animals sensitive to this thin slice of the electromagnetic spectrum
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Ultraviolet
• Have wavelength range from 400 to 100 nanometers

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• Longer UV light can cause changes in skin pigments leading to tanning, while shorter wavelengths can cause cellular radiation damage (sunburn, cancer)

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• Often used as a sterilization technique to kill bacteria

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• The sun produces UV light, though the atmosphere absorbs of this light

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• If in sun too long, should protect skin with sun-block that absorbs/reflects UV light

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• Fluorescent materials can absorb UV light & emit visible light
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X-Ray
• Have wavelength range from 100 to 0.1 nanometers, smaller than a single atom

• Penetrate into most matter, but absorbed differently

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• Allow for medical imaging techniques to visualize bones/organs

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• Generated with a “lightbulb” where a tungsten filament is heated to emit electrons that are moved through the tube using a high voltage & smash into a metal plate; the rapid deceleration produces X-rays

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• Intense X-rays made at synchrotrons, where electrons are accelerated in a circle
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Gamma
• Most energetic electromagnetic radiation

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• Wavelengths range from size of atom (0.1 nm) to size of nucleus (a trillionth of a meter)

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• Emitted on Earth in high-energy nuclear/particle reactions, but produced abundantly in stars

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• Used in nuclear medicine by giving patients radioactive chemicals that accumulate in certain parts of body emit gamma rays

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• Can be used to treat cancer (kill cancer cells)
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Transmission
Light passing unaltered through matter (e.g., through a window or the Earth’s atmosphere)
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Refraction
Light bending as it passes from one medium to another (e.g., moving from air through water, lenses, or a prism); the “bend angle” depends on the wavelength
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Absorption
Light being soaked up by matter, which is typically converted to heat (e.g., asphalt during summer); black/dark colors absorb more visible light
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Scattering
Light absorbed & reemitted in other directions (e.g., diffuse scattering by clouds); white objects scatter all visible wavelengths, colored objects scatter some and absorb others
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Reflection
Light bouncing off a surface, which creates a “mirror image” of the emitting objects
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In the periodic table, elements are organized in columns/rows by…
their weights/properties