Tuesday, December 7, 2010

Exam Details


(This is a copy of an e-mail I sent to the class.)

Here are the room numbers for the Physics 140 (copied from SIMS, so no mistake)

D100 We 12:00PM - 3:00PM SUR5240 Exam 2010/12/8

D200 We 12:00PM - 3:00PM SUR5280 Exam 2010/12/8

Remember that you can use your own Activity Guides and Homework during the exam. There's also a  formula sheet with the exam and it's posted on WebCT.  You should bring a basic scientific calculator. A ruler and protractor might be useful. 

For additional practice here's a good source of exams and solutions:

There should be enough there to keep you busy. (Just skip any problems not covered in our course.)
Right now I can't find the solutions to the posted exam, but if I do I'll post them. 


Wednesday, November 17, 2010

Rotational Terminology

Our textbook Understanding Physics is derived from Fundamentals of Physics by Halliday and Resnick and therefore uses the somewhat nonstandard terminology such as "rotational velocity" instead of "angular velocity" etc. In particular the term "rotational inertia" is used instead of "moment of inertia". I cannot teach this without slipping up occasionally. For this reason and just so the you'll be able to understand the more common terms it's important to make a table comparing H&R terms with the conventional terms.

I also notice that the word "translational" is often used where "linear" may be more common. For example, "translation momentum" is used instead of "linear momentum".

I do think the H&R terminology is more consistent and logical, but it's almost never used anywhere else. Too bad.

Terminology for Rotational Motion

Sunday, November 7, 2010

Signs

There was some confusion in the definition of gravitational potential energy used in Unit 11. This is understandable because of the way that the sign of the fall distance was used.

In this course we'll always take the value of g to be +9.8 m/s2. Therefore when something falls its acceleration is −g. However, when something falls there's always the option of using the positive sign for the downward direction. That seems to be what was done in Unit 11 where y is used for the fall distance. The result was that gravitational potential energy comes out as

Epot = −mgy


That's not not exactly wrong, but is probably confusing because almost everywhere else the sign is positive; so you probably remember this:

Epot= +mgh

I've tried to repair this  confusion by defining the distance of fall as Δy and
as being negative. That way all is more conventional.

Other issues were using the notation Epot for gravitational potential energy whereas Ug is more usual.

Ug = mgΔy

The textbook uses Ugrav which is close. Similarly K is more convenient and usual for Kinetic Energy than Ekin.

I've rewritten the unit's Activity Guide with these changes and I hope it won't be so confusing now. Have a look and let me know what's not clear:

Revised Unit 11

Wednesday, November 3, 2010

Homework 10 Deadline

The deadline for Unit 10 has been extended to Nov 9, after the exam. That way you can keep Unit 10 to study and turn in the Activity Guide and Homework after the exam is finished.

Sunday, October 31, 2010

Midterm 2

Believe it or not it's time to think about the next midterm on Nov. 9

Here are the room numbers:

D100 12:30—13:50 SUR 5380
D200 15:30—16:50 SUR 5280

The format will be the same as before with 10 multiple choice questions and 4 written problems. The total will be worth 50 points for 15% of the final mark. One difference is that we may use Exam Booklets and Bubblesheets so that our printing load will be less. This is due to a possible staff shortage in the Surrey "Document Solutions" service.

All units up through Unit 10 are fair game for this exam. I suggest studying the calculations you did in the activity guides and be prepared for variations of those types of calculations. Make sure you understand the reasons they were done the way they were. Also it would be good to  study the problem examples in the textbook and textbook problems similar to those assigned in homework.

As usual bring a pencil, pen, simple scientific calculator, ruler and a protractor for vectors. You can bringyour own activity guides and homework.

Update
Please turn in your Unit 10 homework and Activity Guide after the exam.

Sunday, October 17, 2010

Friction

Tomorrow's session will deal with friction. It's not my favourite topic, it's not really fundamental physics and the treatment at this level is a little fictitious.

As a challenge you can review your results of the inertial mass measurement in Unit 5 Session 3.  (You measured the accelerations of a fan-cart with and without a bar of known mass on it.) The mass you calculated was systematically wrong because friction was neglected.

Try to figure out how to take friction into account...
  1. How would you experimentally measure the coefficient of kinetic friction in the movement of the fan cart?
  2. How can you correct the mass calculations using the measured coefficient of kinetic friction?
  3. How could you have modified the expriment of Unit 5 so that the systematic error due to friction would have been reduced?

Wednesday, October 13, 2010

Decimal Time, Republican Calendar and other Lost Causes

A decimal clock face made shortly after
 the French revolution. (From Wikipedia)
The decimal time system that was the subject of the first problem on the midterm was actually used for about 2 years after the French Revolution. It's mandatory period of use was less than a year: 22 September 1794 to 7 April 1795. Here is a clock face from the wikipedia article on decimal time.
Republican Date on the door.
(From Wikipedia)
The Republican Calendar lasted a little longer: 12 years. This calendar system had weeks that were 10 days long. One month was three republican weeks. Thus 12 Republican months made for 360 days and there were several holidays at the end of the year to fill out the rest of the 365 or 366 days. Evidence of its use can still be seen on public buildings in France. For example, the door of the famous École Normale Supérieure displays the date 9 Brumaire III, the date of its establishment decree.  (The building was built later.)  Despite the best of intentions, the system was not popular, probably because a 9-day work week replaced one of 6 days.

Can you image the confusion that we would be experiencing if only part of the world had actually adopted--and stuck with--the decimal time and calendar systems? For example the date of the midterm exam, Oct. 8, 2010, would have been called 17 Vendémiaire CCXIX.

All attempts after the French revolution to change units of measurement were based on the premise that dividing units into tens or hundreds makes calculating easier in our base-10 number system. 
But hold on. There's a society that wants to change our number system to base 12! Why?
There are several reasons discussed on the  Dozenal Society website. Here's a hint: in decimal the fraction 1/3 is 0.3333333... and goes on forever. In the dozenal system it's just 0.4.  Exactly.  Wonderful!
Definitely worth the trouble to switch.



Finally, here's in intriguing book: The Measure of the World: A Novel. It tells the story of the project to establish the value of the metre by accurately triangulating the distance from Dunkirk to Paris to Barcelona from hilltop to church steeple to hilltop etc.  Two expeditions set out to do it ---- and they did. We still use the value they determined. (This book is a novelization based on the real project.)


Saturday, October 9, 2010

Midterm Exam Grades

Update
The midterm grades are posted in the webct gradebook.  There are four parts: labelled "Midterm 1 MC", "Midterm 2 probs" and "Midterm 1 response". These report the following:

  • "Midterm 1 MC": The Multiple-choice score out of 20, 
  • "Midterm 2 probs": The Problem score out of 30, 
  • "Midterm 1 total": The total out of 50.  Y
  • "Midterm 1 response": Your multiple choice responses and the correct answers. 
    • The format is [NNNN]xxxxxxxxxx{yyyyyyyyyy}, where NNNN is the version of the exam, yyy... are the correct answers and xx...x is either a dot if you got it right, or your response if it is wrong.
Class average is 34.2/50 with at standard deviation of 7.65.


Earlier post

I'm going to grade these exams myself so it may take a day or so. I'll try to get them done by Tuesday.
In the meantime, please enjoy the Thanksgiving holiday.

Unit 6 AGs and Homework are due on Tuesday.  (sorry)


Monday, October 4, 2010

Midterm Exam Rooms

         
Phys140 D100    10/08/2010  F     12:30 PM       SUR 2600 
Phys140 D200    10/08/2010  F     03:30 PM       SUR 5240  

The Gravity Conspiracy


The last part of Unit 6 Session 1 was dancing around a really interesting coincidence in our world: There are two ways to measure mass. Even though they are completely different, the values the two ways give just happen to be the same. Coincidence? 

All measurements of mass depend on comparing an unknown mass to a standard one. The two ways are
Comparing masses two ways: gravity and inertia.
The mass of a certain volume of water could be
used as the "standard".

  1. Put the object you're measuring on a scale and compare the force of gravity on it to the force on another standard mass.
  2. Try to accelerate it with a force that you can reproduce and compare the acceleration that you get to what you get when you try to accelerate a standard mass with the same force.
These two measurements always give equivalent results. This is so surprising that it has been checked over and over again to high accuracy. When such coincidences seem to occur in nature it's probable that it's not a coincidence, but there is something behind it. That's what Einstein thought and he managed to figure out a logical connection.

To understand the basic idea of Einstein's theory of gravitation imagine that you had a little laboratory in a box with no windows. You can put this laboratory on earth and do experiments with balls and carts and pendulums....whatever.  Then you could put this imaginary lab-in-a-box in a ship and floating far from any gravitational pull and you'd expect the balls not to fall, the pendulums not to swing etc etc, But now fire up the rockets and make the lab accelerate at 9.8 m/s/s and all your experiments would turn out exactly like they would on earth. Einstein took this as a postulate which he called the principle of equivalence.
Experiments on an accelerating rocket ship would seem the same as if gravity were present.
(Figure from Wikipedia)
So gravity acts just like the "fictitious" force that you would feel in an accelerating frame of reference. Similarly the forces you feel on a carousel or centrifuge are proportional to mass, just like gravity — and, in fact, you can use a spinning device to measure mass.

Somehow, mass creates something like an acceleration.  This is accomplished by having mass cause space to warp.  Everything travels in a straight line -- which means the path of shortest distance between two points -- but the space is warped by mass so that the lines are not straight in the Euclidean sense. 

To see how this works in 3 dimensions we have to imagine it in 2D where we can visualize warped space. Then the analogy to 3D can be accepted.  Formally what is done is that the mathematics of warped space is developed that can be used in any number of dimensions so we won't have to be able to visualize what's going on in order or predict what's happening.

So in 2 dimensions a flat universe would have familiar properties as postulated by Euclid: Parallel lines never meet, the interior angles in a triangle add up to 180° and so forth.  Now imagine that the flat space is warped somewhat like a fabric that is poked with your finger.


Mass causes the space near it to warp.
This is a 2D model to help you imagine what's going on in 3D.
(Figure from Wikipedia.)

In this case, draw a triangle, add up the angles and the sum is not 180°. What's important here though is that the shortest distance between two points tends to bend to conform with the curvature of the fabric. The line of shortest distance is called the geodesic and is familiar on our spherical earth as what is called the great circle route that airplanes take when trying to navigate.  In Einstein's universe the curvature of space depends on the mass that is present in the space and the trajectory of an object following the geodesic in the curved space is about the same as what Newton's law of gravitation predicts.

Notice I said "about" the same. Actually there are some small differences between Newton's gravity and Einstein's.  One example is the precession of the perihelion of Mercury's orbit.  The orbit of Mercury does precess as Einstiein's theory predicts and Newton's does not.

Another prediction is that light should be pulled by gravity. Imagine a little hole in one wall of the lab in the rocket ship. If light comes in that hole while the ship is accelerating then the light will hit the other wall a little lower down because of the ship's acceleration. The light beam will seem to "fall".  So by the principle of equivalence, gravity should cause light to "fall". A very careful observation of the light of stars that comes close to the sun shows that this light does bend because the sun's gravity attracts it. This observation has to be done during a total eclipse of the sun and the first time it was done was during an expedition organized by Sir Arthur Eddington in 1910 to test Einstein's prediction.  The bending was confirmed in that the stars whose light came near the sun seemed to shift position from where they should have been.

If you're interested in more about this on a popular level look at the references below --- they're probably in the public library or university library.  If you want to understand the rigorous theory, keep studying physics and math.


References
  1. Hyperspace: A Scientific Odyssey Through Parallel Universes, Time Warps, and the 10th Dimens ion, Michio Kaku
  2. One Two Three . . . Infinity: Facts and Speculations of Science, George Gamow
  3. Mr Tompkins in Paperback (Canto imprint) (containing Mr. Tompkins in Wonderland and Mr. Tompkins Explores the Atom), George Gamow
  4. The Universe and Dr. Einstein, Lincoln Barnett (introduction by A. Einstein)

Wednesday, September 29, 2010

Inertial Mass Measurement

While I was checking the worksheets at the end of class I was noticing that a few groups had "interesting" values for their cart masses on the final table of Unit 5.

  • The mass values you put in the table derive from the accelerations you measure, not the spring scale measurements
  • If you did things right then the Force column (the forces from the fan) should be the same for all cases where the same number of batteries were used.
  • The masses you calculate this way are systematically wrong because you ignore friction.  But if they are wrong by more than about 20% then they are too wrong. (Later we'll learn how to correct for the friction to get a better value.)
  • If they are too wrong then check your method of calculation. The ratio of accelerations should be equal to the ratio of the total mass that is being accelerated. That means you have to do some algebra to solve for the mass of the fan-cart in terms of the bar's mass.
  • The question asking for g want the value implied by your data. If you measured the weight of the cart with a spring scale that weight would be in newtons. If you used to the spring scale and read the mass scale you have to use g = 9.8 N/kg to get the weight. Then you report another value of g  in the question which will be somewhat wrong because friction was ignored.
  • If you find you just can't get any reasonable values from your data then try to understand what's wrong and explain your analysis of the issues. We don't expect you to always get perfect results or to fudge your data and we don't necessarily grade on the nearness of your answer to the "right" answer.

Assignment Dates

There was an inconsistency in the assignment for Unit 5. Originally this unit was 3 sessions and the worksheets on force and motion were to be done over those three sessions.  Because of our short semester, and well-educated students, I have shortened unit 5 to 2 sessions but forgot to edit the assignment list and there was a reference to session 5-3. That's fixed now and all the force-and-motion worksheets are due on Friday, Oct 1.

The general rule is that all the work from a unit is due on the first day of the next unit. The course schedule has the due dates on it too.  The only exception is that there was one extra day allowed for the 11 kinematics problems of Unit 4. The other thing is that on WebCT we recommend that you should do some of the assignments before the due date in order to be able to ask questions in class and to avoid starting too late.

This may be a confusing because normally SFU classes have one assignment per week. I apologize, but this is the most logical way to do things for this course. We have a shorter semester than many universities in North America and we need to compress the schedule to cover all that needs to be covered in a semester.

Sunday, September 26, 2010

Another time, another place

When you try to fit real data with the Fundamental Kinematic Equation (FUNKE) you may run into an issue trying to estimate two parameters, x0 and v0, if the segment of data you're trying to fit starts a long time after t=0.  That's because x0 and v0 are the position and velocity the cart would have had at t=0 if the acceleration had been constant all the way back to t=0. So these values may be a little weird.  For example if you wait 5 seconds before starting the cart at the origin with a constant acceleration of +1 m/s/s, then x0 would be 12.5 m and v0 would be −5 m/s! — because that's where the cart would have had to start, and the velocity it would have had, if it had started 5 seconds earlier and travelled with a constant acceleration all the time.
Position vs time graph of a cart starting at x=0 at t=5s. The actual motion is in blue, the motion extrapolated back to t=0 is in red.

It might be easier to estimate the parameters if one expresses the FUNKE in a different way: use t0, which is the time at which the parabola reaches its extreme value (either maximum or minimum) and xp, the position at that time. In other words, the time and the position of the parabola's apex. Then the FUNKE becomes:


Your fitting parameters are xp, t0 and a,  and a is the same as in the original form. Notice that v0 is not in this equation because at the apex the velocity is zero.

You can do your modelling assignment with this equation. It is another correct way of expressing motion with constant acceleration. As long as you explain what you're doing you'll get full credit if it's right and partial credit if it's wrong and we understand what you're getting at.

There are many right ways of doing most problems. Unfortunately, there are many more wrong ways.

Can you find the mathematical relationship between x0, v0a and xp, t0, a ?
Expand and collect terms

from which



For example if a = 1 m/s2 and the curve reaches the minimum xp = 0 at t0 = 5 s. 

What is x0 and v0?

Saturday, September 25, 2010

the FUN-damental Equation?

In class you used a formulaic method to convince yourselves that the "fundamental kinematic equation" makes sense.  You used the derivative of a polynomial to get the velocity equation from the position equation. You are supposed to instantly recognize the velocity equation that you get as self-evident:
= v(t)
Do the derivatives to get the self-evident equation:

v(t) = ...

(I'm leaving the result out because you're supposed to think it through yourself.)

There's another way to justify the FUNKE (That stands for FUNdamental Kinematic Equation.) Start from the idea that displacement is the area beneath the v(t) graph. Draw the graph for a typical case of constant acceleration and figure out the displacement Δx:

From my Phys100 webpage.

Now I'll colour-code the equation so you can see where each term comes from.


You only need to do some simple substitutions in notation to transform it to the form of the FUNKE at the start:
  • Δx = x(t) - x0
  • Δt = t (lazy notation)
  • v1 = v0
Now our graph that helped us get the equation was just to aid our thinking. It shows a positive a. But nothing in the derivation of the equation assumed that acceleration was positive so the result is general and holds for negative acceleration too.

As an exercise draw the figure for a negative a and see how it works out.

What about negative initial velocity and positive a?

There's one more case. What is it?








Wednesday, September 22, 2010

π, Exhaustion, Method of

When you study calculus they usually do differentiation and then integration. Historically the order was different.

In school you learned what the number π stands for and you probably memorized its value to a few digits.  But could you figure out what it was if you had to?

The story of how people figured out the value of π is the story of integration.  We can start in ancient Egypt where an approximate value was got my measuring circles. It was a Greek guy, Eudoxus of Cnidus, who starting thinking about how to figure it out exactly. He developed the Method of Exhaustion to find the areas of various shapes and another Greek dude, Archimedes,  used the Method of Exhaustion to nail down the value of pie (oops, π) to a small range:
 3 10/71 < π < 3 1/7.

Square-Circle-Square
(Yes it's a circle)
To understand how he did it imagine a circle with radius r. Draw a square outside it with sides of length 2r. Now draw another square  inside whose diagonal has length 2r. The sides of this square have length 2r/√2.
The area of the outer square, 4r2, is obviously larger than that of the circle. The area of the inner square, 2r2, is obviously smaller than the circle'In t. Therefore,

2 < π < 4.

We can narrow down the range by doing the same thing with hexagons, octagons and regular polygons with more and more sides:

Archimedes continued this until he got to a 96-sided polygon and that's how he computed the result above.  After that he was exhausted.

One-question physics test

There's a one-question physics test that lets me know if we're making progress. It's the last question of Unit 3.  
"Consider the ball toss carefully. Assume that upward is the positive direction. Indicate in the table that follows whether the velocity is positive, zero or negative during each of the three parts of the motion. Also indicate if the acceleration is positive, zero or negative."
Why?

Learning physics requires revising preconceptions we come to the class with.  The meaning of acceleration illustrates one such preconception. As commonly used, the word acceleration means moving faster. The reasoning goes like this: 
If you're not moving then you can't be accelerating. Zero velocity means not moving doesn't it? — therefore if v = 0 then a = 0.   

Right? 

Wrong!

The precise definition of acceleration in the physics context is the rate of change of velocity: a= dv/dt
The velocity can be instantaneously at zero, but if the velocity is changing then acceleration is not zero.

If you understand this then you're changing your preconceptions based on your physics lessons. If not then either you're not listening, or you hear but don't want to accept something that violates your sense of what's right.

The reason we need to get this is that forces lead to acceleration and physics is all about forces and what they do to things.


If you think you got it then try this question:

Mike jumps out of a tree and lands on a trampoline. The trampoline sags 0.5 m before launching Mike back into the air. At the very bottom, where the sag is the greatest, Mike’s acceleration is:
A. Upward B. Downward C. Zero

Have the courage of your convictions and enter your answer as an (anonymous) comment. Say why.

Update  For answer click here.

Sunday, September 19, 2010

Troubleshooting

The concepts Friday were easy, but sometimes the equipment didn't cooperate. If you're having trouble with the equipment, it's probably a good idea to check out a few of the usual suspects before you panic. It might take us instructors a while to get over to help you and a little easy troubleshooting can save time.


  1. Check the power: 
    • Is the block plugged into powerbar? 
    • Is the powerbar switch on? 
    • Make sure that the little power plug is pushed all the way into the LabPro interface. (If you push it in and you hear the LabPro jingle, then it wasn't pushed in enough.)
    • If there's power, then there should be some lights on inside.
  2. Check the USB cable. The USB cable should be plugged into the LabPro and the other end to the computer. It might go to the USB port in the monitor instead of the computer, but people tell me this is less reliable. And make sure it's going to the USB port of your computer.
  3. Make sure the sensor is plugged into the correct port. For example the Motion Sensor should normally be plugged into the DIG/SONIC 1 port for the setup file that's recommended in unit 3.  (It can work in the other port but you have to change the setting in LoggerPro software under "Setup Sensors...".)
  4. If you lose your LoggerPro tool bar, click on the little button in the upper right-hand corner of the Logger Pro window.
  5. If the sensors were not plugged in when you loaded the setup file then try reloading the setup file again after the sensors are plugged in. Many of the sensors are auto-detected, but not all. Later on you'll have to learn how to tell LoggerPro by hand which sensor is on what port. That's under the menu item "Setup Sensors...".
  6. If you're getting noisy motion data, then clear out all extra stuff from nearby your track like pencil boxes, bags, books etc. Keep your hands away from the track while measuring. Try adjusting the tilt of the detector and put it on narrow beam to measure cart motion.

Thursday, September 16, 2010

New Problems Proposed

Last year I changed Unit 2 but did not write replacements for problems 2-4 and 2-5.  Here are two PROPOSED problems. They are not assigned this year but I post them here for the record and discussion.

SP2-4

Make a table showing the probabilities that the sum of the roll of 3 dice are  3, 4, 5, 6, 7, ...18. You have already done 11 in the activity guide. Explain your method of calculation. Hint: You can use a symmetry argument to shorten the calculations. The probability for getting 3 is the same as for 18, the probability of getting 4 is the same as for 17, etc. 


SP2-5

Instead of measuring the background level in one run of 80 1-minute intervals you do 2 experiments, measuring 30 1-minute intervals and then 50 1-minute intervals. The results are as follows:
  30 intervals: average = 11.8 counts/minute, SD = 4.2  counts/minute
  50 intervals: average = 12.2 counts/minute, SD = 3.8 counts/minute
Use the formulas for the average and Standard Deviations to determine what the average and SDs would have been if you had done this experiment as a single experiment of 80 1-minute intervals.

Level of Confidence?

Here is a question I received from a student by e-mail.

"Could you clraify exactly what it means to estimate the level of confidence of our conclusion. What is our conclusion on (which part of the guide) and how are we to estimate the level of confidence of the conclusion if it is a written statement."


My answer:

"You are trying to answer the question:

'Is there a significant difference between the number of counts/minute detected when the nu-salt is present compared to when the nu-salt was not present?'

You need to use the statistical quantities we measured for the number of counts/minute both with and without the nu-salt present: average, standard deviation, number of counts and standard deviation of the mean. The level of confidence will depend on how far apart the averages of the two experiments are compared to the standard deviations of the means."

In other words, if the means differ by about 1 SDM then you can conclude that the difference is real to a 68% level of confidence. If they differ by 2 SDM then they differ to a 95% level of confidence.  If they differ by something between 1 SDM and 2 SDM  then you conclude that the difference is real to something between 68% and 95% level of confidence.

Wednesday, September 15, 2010

Unit 2 Bugs

On WebCT there is an Activity 2-11 upload but there is no Activity 2-11.  That was something I forgot to delete after I revised Unit 2 last year. It is not there now and is not due -- don't worry about it.   Furthermore, there is no SP2-4 and SP-5, yet.

(I was thinking about assigning a problem on calculating the probabilities of all possible outcomes of throwing three dice, but I wonder if that would be too hard?)




This is a copy of a class email.

Monday, September 13, 2010

The Standard Deviation vs Standard Deviation of the Mean...

Today we encounered the concept of the Standard Deviation. The Standard Deviation of the Mean is coming tomorrow. Understanding the distinction is a real brain teaser, but important.

There's a lot to do tomorrow so we'll try not to waste so much time at the beginning of class. One source of random numbers is radioactive decay.  I'll show how some common stuff you can get in the supermarket has radioactivity significantly above the background level.

Friday, September 10, 2010

Bowling Data

The bowling data serve as grist for plotting a graph using Excel. One of the homework problems is to superimpose a mathematical model. To ease this task there is a downloadable spreadsheet file called the "Modeling Worksheet". (Look on WebCT under Unit 1.)  Another spreadsheet file, the "Modeling Tutorial", shows an example of how to use it.
The Modeling Tutorial Spreadsheet

The model you'll want to use is



x0 is the intercept (b, cell C2) on the vertical axis and vavg is the slope (m, cell C1).  The position of the ball is x(t) and the time from the start is t.


(This model ignores the slowing of the ball as it rolls.)


You can use the Modeling Tutorial spreadsheet as a template for assignment problem SP1-2
To enter in this formula, you type in the first cell of y-theory (cell C8)

=$C$1*A8 + $C$2


You should see the theoretical value for the first data point calculated in cell C8. If you made a mistake there's an error message and you'll have to fix it before going on.


Copy this formula down the column to the end of the data.  A8 will change to A9, A10, etc but the references to $C$1 and $C$2 do not change because placing the dollar sign in front of the column letter and row number makes these references Absolute References instead of Relative References. After you copy the formula a line should appear on the graph representing the theoretical model.


Now you need to change the numbers in cells C1 and C2 until the line passes through the data points so that it represents a reasonable model of the position vs time which is consistent with the data.


(I know there is an automatic "Trendline" feature in Excel, but you should do the procedure described here so that you can understand and appreciate the automatic process better.)

Wednesday, September 8, 2010

Asteroid Buzz

You probably didn't notice but two small asteroids came close to Earth on Wednesday. (http://www.nasa.gov/topics/solarsystem/features/asteroid20100907.html). 
Their orbit took them within the moon's orbit of the earth. Small means 10 to 20 m in diameter.
 Image credit: NASA/JPL-Caltech

This apparently happens all the time but until recently we didn't know. The rate of asteroid detection has escalated recently as shown by this movie:


Asteroid Discovery From 1980 - 2010




Most of those asteroids are pretty far from Earth, but there are a lot  too close for comfort.

Ignorance was bliss.

PS: This will not be on the exam.

Tuesday, September 7, 2010

First Day was O.K.

Because I wore my rain jacket and left the sunglasses at home the weather cleared up.  Both classes were able to go to Holland park and pitch the baseballs in the sun -- even the grass wasn't wet.


A cellphone video of the baseball activity.

The main point of this exercise was to get some practice using a spreadsheet to analyse data. Homework SP1-1 requires averaging the data, finding the minimum and maximum speed and sorting. I found out that Firefox changes tabs to spaces in text files so that you can't just copy and paste the data. Using "Paste Special".. "text" does the job the most easilty. Alternatively you can paste data and then use the "Text to Columns" feature.

Friday we bowl. It's going to rain Friday, I'm sure, even if I wear all my rain gear. So it's good that we do that in doors in our Studio room not the bowling alley, unfortunately. Then we'll learn how to make a graph in Excel.  

One can also do these exercises in OpenOffice if one wants their own capable speadsheet application which is reasonably compatible with Excel.  There are a few differences, especially when it comes to graphics, but free is good.




Sunday, September 5, 2010

2 days to go

It's Labour Day Weekend and the Schedule is set, WebCT configured and the handouts printed.  The only question is the weather on Tuesday.  The first day is the only day we do something outdoors and reports show rain is possible. Normally we go outdoors and measure how fast we can pitch a baseball.  Alternative activities are now being contemplated.

I've just learned from a student that the Chemistry 121 exam in Burnaby is just before the Physics 140 exam in Surrey.  There may be several students afflicted by this scheduling fiasco, so we'll have to make some provision.

Friday, August 27, 2010

This is the first post on the Physics 140 blog.  I'm still configuring the WebCT container and figuring out the semester's schedule.  There's only a little more than a week until we start and I'm wasting time starting this blog. So much for efficiency.