Tuesday, 31 May 2016

Avogadro’s number

Avogadro’s number

mole is simply Avogadro's number of things. In chemistry, those "things" are atoms or molecules. In theory, you could have a mole of baseballs or anything else, but given that a mole of baseballs would cover the Earth to a height of several hundred miles, you'd be hard-pressed to find good practical use for a mole of anything bigger than a molecule [source: Hill and Kolb]. So if the mole is only used for chemistry, how did Amedeo Avogadro and chemistry cross paths  Born in Italy in 1776, Avogadro grew up during an important period in the development of chemistry. Chemists like John Dalton and Joseph Louis Gay-Lussac were beginning to understand the basic properties of atoms and molecules, and they hotly debated how these infinitesimally small particles behaved. Gay-Lussac's law of combining volumes particularly interested Avogadro. The law stated that when two volumes of gases react with one another to create a third gas, the ratio between the volume of the reactants and the volume of the product is always made of simple whole numbers. Here's an example: Two volumes of hydrogen gas combine with one volume of oxygen gas to form two volumes of water vapor (at least when temperatures are high enough) with nothing left over, or:
2H2 + O2 --> 2H2O
Tinkering around with the implications of this law, Avogadro deduced that in order for this to be true, equal volumes of any two gases at the same temperature and pressure must hold an equal number of particles (Avogadro's law). And the only way to explain that this law could be true for any example, including the one we just mentioned, is if there was a difference between atoms and molecules and that some elements, like oxygen, actually exist as molecules (in oxygen’s case, O2 rather than simply O) Granted, Avogadro didn't have words like "molecule" to describe his theory, and his ideas met resistance from John Dalton, among others. It would take another chemist by the name of Stanislao Cannizzaro to bring Avogadro's ideas the attention they deserved. By the time those ideas gained traction, the Italian with the crazy long name had already passed away.
So where does Avogadro's number fit into this? Because Avogadro's law proved so critical to the advancement of chemistry, chemist Jean Baptiste Perrin named the number in his honor. Read on to see how chemists determined Avogadro's number and why, even today, it's such an important part of chemistry.

Area Formulas

Area Formulas


Square = a 2 
Rectangle = ab 
Parallelogram = bh 
Trapezoid = h/2 (b1 + b2
Circle = pi r 2 
Ellipse = pi r1 r2 

triangle =one half times the base length times the height of the triangle
  
equilateral triangle =

triangle given SAS (two sides and the opposite angle)= (1/2) a b sin C
triangle given a,b,c = sqrt[s(s-a)(s-b)(s-c)] when s = (a+b+c)/2 (Heron's formula)
regular polygon = (1/2) n sin(360°/n) S2
   when n = # of sides and S = length from center to a corner
   Units
Area is measured in "square" units. The area of a figure is the number of squares required to cover it completely, like tiles on a floor.
Area of a square = side times side. Since each side of a square is the same, it can simply be the length of one side squared.
If a square has one side of 4 inches, the area would be 4 inches times 4 inches, or 16 square inches. (Square inches can also be written in2.)

Be sure to use the same units for all measurements. You cannot multiply feet times inches, it doesn't make a square measurement.

Volume Formulas

Volume Formulas


cube = a 3 
rectangular prism = a b c 
irregular prism = b h 
cylinder = b h = pi r 2 h 
pyramid = (1/3) b h 
cone = (1/3) b h = 1/3 pi r 2 h 
sphere = (4/3) pi r 3 
ellipsoid = (4/3) pi r1 r2 r3 


Units
Volume is measured in "cubic" units. The volume of a figure is the number of cubes required to fill it completely, like blocks in a box.
Volume of a cube = side times side times side. Since each side of a square is the same, it can simply be the length of one side cubed.
If a square has one side of 4 inches, the volume would be 4 inches times 4 inches times 4 inches, or 64 cubic inches. (Cubic inches can also be written in3.)
Be sure to use the same units for all measurements. You cannot multiply feet times inches times yards, it doesn't make a perfectly cubed measurement.

Monday, 23 May 2016

Fluid Mechanics - Law of Continuity

 Law of Continuity

Any fluid moving through a pipe obeys the Law of Continuity, which states that the product of average velocity (v), pipe cross-sectional area (A), and fluid density (ρ) for a given flow stream must remain constant:
 
Fluid continuity is an expression of a more fundamental law of physics: the Conservation of Mass. If we assign appropriate units of measurement to the variables in the continuity equation, we see that the units cancel in such a way that only units of mass per unit time remain:
 
This means we may define the product ρAv as an expression of mass flow rate, or W:

In order for the product  to differ between any two points in a pipe, mass would have to mysteriously appear and disappear. So long as the flow is continuous (not pulsing), and the pipe does not leak, it is impossible to have different rates of mass flow at different points along the flow path without violating the Law of Mass Conservation. The continuity principle for fluid through a pipe is analogous to the principle of current being the same everywhere in a series circuit, and for equivalently the same reason1.
We refer to a flowing fluid as incompressible if its density does not substantially change2. For this limiting case, the continuity equation simplifies to the following form:


Examining this equation in light of dimensional analysis, we see that the product Av is also an expression of flow rate:


Cubic meters per second is an expression of volumetric flow rate, often symbolized by the variable Q:

 
The practical implication of this principle is that fluid velocity is inversely proportional to the cross-sectional area of a pipe. That is, fluid slows down when the pipe’s diameter expands, and visa-versa. We see this principle easily in nature: deep rivers run slow, while rapids are relatively shallow (and/or narrow).
For example, consider a pipe with an inside diameter of 8 inches (2/3 of a foot), passing a liquid flow of 5 cubic feet per minute. The average velocity (v) of this fluid may be calculated as follows:
 

Solving for in units of square feet:
 

Now, solving for average velocity v:
 
 
1In an electric circuit, the conservation law necessitating equal current at all points in a series circuit is the Law of Charge Conservation.
2Although not grammatically correct, this is a common use of the word in discussions of fluid dynamics. By definition, something that is “incompressible” cannot be compressed, but that is not how we are using the term here. We commonly use the term “incompressible” to refer to either a moving liquid (in which case the actual compressibility of the liquid is inconsequential) or a gas/vapor that does not happen to undergo substantial compression or expansion as it flows through a pipe. In other words, an “incompressible” flow is a moving fluid whose ρ does not substantially change, whether by actual impossibility or by circumstance.

Kepler's Laws

Kepler's Laws


Johannes Kepler, working with data painstakingly collected by Tycho Brahe without the aid of a telescope, developed three laws which described the motion of the planets across the sky.

1. The Law of Orbits: All planets move in elliptical orbits, with the sun at one focus.
2. The Law of Areas: A line that connects a planet to the sun sweeps out equal areas in equal times.
3. The Law of Periods: The square of the period of any planet is proportional to the cube of the semimajor axis of its orbit.

Kepler's laws were derived for orbits around the sun, but they apply to satellite orbits as well.

The Law of Orbits

All planets move in elliptical orbits, with the sun at one focus.

This is one of Kepler's laws. The elliptical shape of the orbit is a result of the inverse square force of gravity. The eccentricity of the ellipse is greatly exaggerated here


Orbit Eccentricity

The eccentricity of an ellipse can be defined as the ratio of the distance
between the foci to the major axis of the ellipse. The eccentricity is zero for a circle. Of the planetary orbits, only Pluto has a large eccentricity.

Examples of Ellipse Eccentricity

Planetary orbit eccentricities
Mercury.206
Venus.0068
Earth.0167
Mars.0934
Jupiter.0485
Saturn.0556
Uranus.0472
Neptune.0086
Pluto.25

The Law of Areas

A line that connects a planet to the sun sweeps out equal areas in equal times.

This is one of Kepler's laws.This empirical law discovered by Kepler arises fromconservation of angular momentum. When the planet is closer to the sun, it moves faster, sweeping through a longer path in a given time. 

The Law of Periods

The square of the period of any planet is proportional to the cube of the semimajor axis of its orbit.

This is one of Kepler's laws.This law arises from the law of gravitation. Newton first formulated the law of gravitation from Kepler's 3rd law.
Kepler's Law of Periods in the above form is an approximation that serves well for the orbits of the planets because the Sun's mass is so dominant. But more precisely the law should be written
In this more rigorous form it is useful for calculation of the orbital period of moons or other binary orbits like those of binary stars.

Data: Law of Periods

Data confirming Kepler's Law of Periods comes from measurements of the motion of the planets.
Planet
Semimajor
axis
(1010m)
Period
T (y)
T2/a3
(10-34y2/m3)
Mercury5.790.2412.99
Venus10.80.6153.00
Earth15.012.96
Mars22.81.882.98
Jupiter77.811.93.01
Saturn14329.52.98
Uranus287842.98
Neptune4501652.99
Pluto5902482.99
The quantity T2/a3 depends upon the sum of the masses of the Sun and the planet, but since the mass of the Sun is so great, adding the mass of the planet makes very little difference.
Data from Halliday, Resnick, Walker, Fundamentals of Physics 4th Ed Extended.

Intercooler

Intercooler


An intercooler is an intake air cooling device commonly used on turbocharged and supercharged engines.


An intercooler cools the air compressed by the turbo/supercharger, reducing its temperature and thereby increasing the density of the air supplied to the engine.


As the air is compressed by a turbo/supercharger it gets very hot, very quickly. As its temperature climbs, its oxygen content (density) drops, so by cooling the air, an intercooler allows denser, more oxygen rich air to the engine, allowing more fuel to be burned, thus improving combustion and giving more power. It also increases reliability as it provides a more consistent temperature of intake air to the engine which allows the air fuel ratio of the engine to remain at a safe and steady level.
There are two types of intercoolers; Air-to-Air and Air-to-Water.
An Air-to-Air intercooler extracts heat from the compressed air by passing it through its network of tubes with cooling fins. As the compressed air is pushed through the intercooler it transfers the heat to the tubes and, in turn to the cooling fins. The cool air from outside, traveling at speed, absorbs the heat from the cooling fins reducing the temperature of the compressed air. The advantages of this system are simplicity, lower cost and light weight. These factors make it by far the most common form of intercooling. The down sides can be a longer intake length (as the intercooler is usually at the front of the car) and more variation in temperature than the Air-to-Water type.
An Air-to-Water intercooler uses water as a heat transfer agent. In this setup cool water is pumped through the air/water intercooler, extracting heat from the compressed air as it passes through. The heated water is then pumped through another cooling circuit (usually a dedicated radiator) while the cooled compressed air is pushed into the engine.
These intercoolers (also known as heat exchangers) tend to be smaller than their Air-to-Air counterparts making them well suited to difficult installations where space, airflow and intake length are an issue. Water is more efficient at heat transfer than air and has more stability so it can handle a wider range of temperatures.
On the downside the Air-to-Water system is complex, heavy and has the added cost of a radiator, a pump, water and transfer lines. Common applications for these are industrial machinery, marine and custom installs that don’t allow the easy fitment of an air to air intercooler, such as a rear-engined vehicle.
Intercooler placementThe best placement for an air to air is in the at the front of the vehicle. The “front-mount” is considered to be the most effective placement.
When the engine layout, or type of the vehicle do not permit the “front-mount” placement, an intercooler can be mounted on top of the engine, or even on its side, but these are not considered as effective as the air flow is not as good and the intercooler can suffer from heat soak from the engine when the external airflow drops. These placements will often require additional air ducts or scoops to route the air directly into the intercooler.

Subaru’s trademark top-mount requires a scoop in the bonnet to route the airflow onto the intercooler.
The Air-to-Water system can be mounted anywhere in the engine bay, as long as the radiator is mounted in a position where it receives good airflow, and/or with a thermo fan attached to it.

The Steady Flow Energy Equation (SFEE)

The Steady Flow Energy Equation (SFEE) is used for open systems to determine the total energy flows.
It is assumed that the mass flow through the system is constant.
It is also assumed that the total energy input to the system is equal to the total energy output.
The energies that are included are;
          internal, flow, kinetic, potential, heat and work.
The equation is shown below where suffix 1 is the entrance and suffix 2 the exit from the system.




where:
u          =          internal energy (J)
P          =          pressure (N/m2)
v          =          volume (m3)
C          =          velocity (m/s)
g          =          acceleration due to gravity (m/s2)
Z          =          height above a datum (m)
Q         =          heat flow (J)
W         =          work (J)

The term P .v  represents the displacement or flow energy.
The term  C/ 2   represents the kinetic energy.
The term g. Z  represents the potential energy.

 
In thermodynamics the changes in potential energy are usually small except for example a water reservoir supplying water to a low level turbine.
In the following examples we can omit the potential energy term thus simplifying the equation to;



u1  +  P1v1  +           +  Q   =    u2  +  P2v2  +            +  W


Also the term  ( u  +   P.v ) is also known as specific enthalpy (h), so the equation is now written;



h1  +            +  Q   =    h2  +            +  W


Example 1

In a steady flow open system a fluid flows at a rate of 4 kg/s.
It enters the system at a pressure of 6 bar, a velocity of 220 m/s, internal energy
2200 kJ/kg and specific volume 0.42 m3/kg.
It leaves the system at a pressure of 1.5 bar, a velocity of 145 m/s, internal energy
1650 kJ/kg and specific volume 1.5 m3/kg.
During its passage through the system, the fluid has a loss by heat transfer of 40kJ/kg to the surroundings.
Determine the power of the system, stating whether it is from or to the system.
Neglect any change in potential energy.


u1  +  P1v1  +                +    Q   =       u2  +  P2v2  +               +   W


Power from the system (kW)   = Work output (kJ/kg) x mass flow rate of fluid (kg/s)

Work output (kJ/kg) can be found by rearranging the SFEE.

We can work in kilojoules (kJ). This means that the  kinetic energy section of the SFEE will be divided by 103 to put it in kJ.


W  =   ( u1  -  u2)   +  ( P1v1  -    P2v2 ) +   (                 )  +  Q




2 x 103
 
W   =   ( 2200  -  1650 )  +  ( 600  x  0.42    -   150  x  1.5 )  +  (                     )   – 40

W  =    550     +      27         +         13.69          -    40

W   =    550.69  kJ/kg

This is positive so it is energy output from the system.

Power from the system (kW)   =           W    x  m
                                   
                                                =          550.69   x   4 kg/s

                                                =          2202.76 kW

Difference between stress and strain

What is the difference between stress and strain? Answer: Stress is the internal resistance force per unit area that opposes deformation, w...