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Transcript review - Uplift North Hills

𝛾=
βˆ†π‘‰
𝑉0 βˆ†πœƒ
(K-1 or oC-1)
Ξ³-coefficient of
volume expansion
βˆ†πœƒ increase in temp.
Solving problems relevant to energy transformations
Wind generator. air density ρ, wind speed v, a rotor blade radius of r
assumption: wind is stopped by the wind turbine, which is not the case,
so not all of KE of the wind is turned into electricity.
r
To calculate how much energy there is in the wind,
we consider a cylinder of air with a radius the
same as the radius of the turbine as shown.
If the velocity of air is v then in βˆ†π‘‘ π‘ π‘’π‘π‘œπ‘›π‘‘π‘  it will
move a distance v βˆ†π‘‘. The volume of air passing by
the turbine per second is v βˆ†π‘‘ Ο€ r2.
The mass of this cylinder of air, m = ρ v βˆ†π‘‘ Ο€ r2
where ρ is the density of air.
The KE of this air = ½ mv2 = ½ ρ v βˆ†π‘‘ Ο€ r2 v2
= ½ ρ Ο€ r2 v3 βˆ†π‘‘
Since this is the KE of air moving past the turbine
per βˆ†π‘‘ second, the power in the wind is KE/ βˆ†π‘‘.
P = ½ ρ Ο€ r 2 v3
Hydroelectric power
gravitational PE of water
β†’ KE of water β†’ KE of turbines β†’
electrical energy
The energy stored in a lake is gravitational PE = mgh. h is the height difference between the
outlet from the lake and the turbine. Since not all of the water in the lake is the same height,
the average height is used (this is assuming the lake is rectangular in cross section).
The rate of change of the potential energy converted
into kinetic energy is
P=
mgh
(ρV)gh
V
=
= ρ gh = ρ Q g h
t
t
t
Q is known as the volume flow rate (m3/s )
ρ – density of the water
V – volume of the lake
Intensity I of the Sun’s radiation incident on a planet at
distance r from the Sun is the power radiated received at
distance r per unit area
Astrophysics: apparent brightness b
The power from the star received (incident) per m2 of the
L
Earth’s surface. If the energy radiated by a star is emitted
b = 4π𝑑2
uniformly in all directions, then apparent brightness is
where L is luminosity (power radiated) of the star and d its distance from the Earth.
Albedo: Some of the radiation received by a planet is
reflected straight back into space. The fraction that is
reflected back is called the albedo, 
Ξ±=
total (reflected) scaterred power
total incident power
Earth’s albedo varies daily and is dependent on season (cloud formations) and latitude. Oceans
have a low value but snow has a high value. The global annual mean albedo is 0.3 (30%) on Earth.
If the temperature of a planet is constant, then the power being absorbed by the planet must equal
the rate at which energy is being radiated into space. The planet is in thermal equilibrium.
Surface heat capacity is the energy required to raise
the temperature of unit area of a planet’s surface by
one degree, and is measured in J m-2 K-1
CS =
energy
area of surface x temperature change of surface
If the incoming radiation power and outgoing radiation power are not equal, then the change of the
planet’s temperature in a given period of time is:
Ξ”T =
(incoming radiation intensity βˆ’ outgoing radiation intensity)× time
Cs
A black body is a theoretical object that absorbs all incident
electromagnetic radiation. Therefore it reflects no radiation and
appears perfectly black. It is also a perfect emitter of radiation.
It would emit at every wavelength of light, and the β€œblack body
radiation” distribution as a function of wavelength, known as
Planck’s law, depends upon its temperature.
Although stars and planets are not perfect emitters, their radiation
spectrum is approximately the same as black-body radiation.
WIEN’S LAW
wavelength at which the intensity of the radiation is
a maximum, Ξ»max, is inversely to the temperature of
the black body
2.9×10-3
max (m) ο€½
T(K)
STEFAN - BOLTZMANN LAW
The total power ((total energy per unit time) radiated by a black
body is proportional to 4th power of surface temperature
(astrophysics: luminosity)
P = ΟƒAT4
 = Stephan - Boltzmann constant
A – surface area of the emitter
T – absolute temperature of the emitter (in Kelvin)
The Earth and its atmosphere are not a perfect black body.
Emissivity, e, is defined as the ratio of power radiated by an
object to the power radiated by a black body at the same temperature.
e=
power radiated by an object
power radiated by black body at the same temperature
There are only two ways to transfer energy from one body to another β€” either by doing work or
by transferring thermal energy.
Thermal energy may be completely converted to work in a single process, but that continuous
conversion of this energy into work requires a cyclical process (use of machines that are
continuously repeating their actions in a fixed cycle) and the transfer of some energy from the
system (to the surroundings and therefore no longer available to perform useful work).
Degraded energy is energy that has become less useful (unavailable), i.e. cannot perform
mechanical work due to being transformed
into other forms of energy, e.g. thermal energy (in accordance with the second law of
thermodynamics)
Sankey diagrams are used to represent different ways of producing useful energy.
Fuel is a substance that can release energy by changing its chemical or nuclear structure.
All possible sources of energy:
β–ͺ The Sun’s radiated energy
β–ͺ Gravitational energy of the Sun and the Moon
β–ͺ Nuclear energy stored within atoms
β–ͺ The Earth’s internal heat energy
β—‹ The Sun is the prime energy source for the world’s energy.
Energy density is the amount of energy that can be extracted per kilogram of fuel. Unit: J kg -1
Conduction, convection and thermal radiation
β–ͺ When two solids of different temperatures touch, thermal energy is transferred from the
hotter object to the cooler object through a process called conduction.
β–ͺ When atoms of one portion of a material are in contact with vibrating atoms of another
portion, the vibration is transferred from atom to atom.
HC
O
O
TL
D
d
H
O
T
β–ͺ Since we associate motion with temperature, high T portions vibrate more than low T
portions, so we can imagine the vibration β€œimpulse” to travel through the material, from high T
to low T.
β–ͺ Metals are good heat conductors because they have lots of free electrons (the same reason
they are good electrical conductors).
β–ͺ The rate Q / t at which heat energy is transferred depends directly on the crosssectional area A and inversely with the length d of the conductor.
β–ͺ That rate, Q / t, is also proportional to the difference in temperature T, between
the two ends.
βˆ†π‘„
βˆ†π‘‡
= βˆ’π‘˜π΄
βˆ†π‘‘
𝑑
Thermal conduction:
The rate of transfer of internal energy Q is
proportional to temperature gradient:
Chain reaction: β–ͺ Energy is required to split a U – 236 nucleus. This can be supplied by adding a
neutron to the U –235 nuclei, which destabilizes the nucleus U – 236
(formed after a neutron is caught by U – 235) and causes it to split in two.
β–ͺ Extra neutrons are produced, which can go on to react with other U – 235 nuclei
in a self-sustaining chain reaction.
However neutrons must be first slowed down to less than 1 eV.
Too fast neutrons are not likely to make reaction.
Critical mass: the minimum mass required for a chain reaction. (atomic bomb: mass > critical mass)
Fuel enrichment: β–ͺ Uranium comes naturally as 99.3% U-238. However only U – 235 is used
in the reaction process.
β–ͺ The process of increasing the percentage of U-235 in the material to make
nuclear fission more likely is called enrichment.
β–ͺ 3% U-235 must be reached in order to power a nuclear reactor.
http://www.nrc.gov/materials/fuel-cycle-fac/ur-enrichment.html
Controlled nuclear fission (power production) and uncontrolled nuclear fission (nuclear weapons)
In naturally occurring uranium, there is vastly more of the uranium-238 isotope than of
the uranium-235 isotope. The latter makes up only a fraction of a percent of the overall
mass of the ore.
Most nuclear reactors require a much higher percentage of uranium-235 in order to
maintain a nuclear reaction. This is where uranium enrichment is important β€” giant
rows of centrifuges slowly increase the amount of uranium-235 in a sample of uranium,
allowing it to be used in power plants or weapons.
However, some reactors that use heavy water can use unrefined uranium as a fuel,
removing the expensive and time consuming enrichment process. These reactors also
tend to produce more plutonium as a waste product that can be used in weapons.
This is why heavy water reactors are a concern, and why we are talking about heavy
water this week.
Talk about resonance absorption of KE
very efficient momentum transfer, similar conceptually to
the collision of two billiard balls
Main energy transformations in a nuclear power station:
nuclear energy β†’ thermal energy β†’ mechanical energy β†’ electrical energy
Three important components in the design of all nuclear reactors are
moderator, control rods and heat exchanger.
β–ͺ Moderator is a medium that slows down fast neutrons to make them suitable for reaction
(water, graphite, heavy water).
β–ͺ Control rods are movable rods that readily absorb neutrons. They can be introduced or
removed from reaction chamber in order to control the rate of fission of
uranium and plutonium. Made of chemical elements capable of absorbing
many neutrons without fissioning themselves (cadmium, hafnium, boron, etc)
β–ͺ Heat exchanger is used to seal off the place where nuclear reactions take place from the rest
of the environment. In some nuclear power plants, the steam from the
reactor goes through a heat exchanger to convert another loop of water
to steam, which drives the turbine.
The advantage to this design is that the radioactive water/steam never
contacts the turbine.
http://hyperphysics.phyastr.gsu.edu/hbase/nucene/ligwat.html
Neutron capture by a nucleus of uranium-238 results in the production of a nucleus of
plutonium-239
In addition to uranium – 235, plutonium – 239 is also capable of sustaining fission reactions. This
nuclide is formed as a by - product of a conventional nuclear reactor. A uranium – 238 nucleus
can capture fast moving neutrons to form uranium – 239. This undergoes Ξ² – decay to neptunium
– 239 which undergoes further undergoes further Ξ² – decay to plutonium – 239
238
239U
1
U
+
𝑛
β†’
0
92
92
239
239
U β†’ 93Np + βˆ’10𝛽 + 𝜈
92
239
93
Np β†’
239
0
94Pu + βˆ’1𝛽 + 𝜈
Plutonium-239 is used as a fuel in other types of reactors.
Problems associated with producing nuclear power using nuclear fusion: the reaction
requires creating temperatures high enough to ionize atomic hydrogen into a plasma state.
Currently the principal design challenges are associated with maintain and confining the
plasma at sufficiently high temperature and density for fusion to take place.
Solar Power
β–ͺ Solar panel (active solar heater) is used for central heating or for making hot water for
household use, placed on roofs of houses, consisting of metal absorber, water pipes,
and glass. It converts solar energy into thermal energy of water.
β–ͺ A photovoltaic cell converts solar radiation into electrical energy. Produces very small voltage
The greenhouse effect is the warming of a planet due its atmosphere allowing in ultraviolet
radiation from the Sun, but trapping the infrared radiation emitted by the warm Earth.
Temperature of the Earth’s surface will be constant if the rate at which it radiates energy
equals the rate at which it absorbs energy.
Short wavelength radiation is received from the sun and causes the surface of the Earth to
warm up. The Earth will emit infra-red radiation (longer wavelengths than the radiation
coming from the sun because the Earth is cooler than the sun). Some of this infra-red
radiation is absorbed by gases in the atmosphere and re-radiated in all directions.