Tuesday, November 29, 2011

IB Physics - IA Example: Data Collection and Processing

!±8± IB Physics - IA Example: Data Collection and Processing

For anyone who has difficulty writing up their practicals, this article helps to explain the data collection and processing component of writing an IB Physics Practical.

Basically, the practical involved calculations of momentum using a machine that allowed collisions with minimal friction. The aim was to verify the law of conservation of momentum.

Below is an example of one such practical:

Data collection and Processing:

Qualitative Observations:

It was noticed that the metal of the ramp heated up slightly after each recording and that unless the ramp was adjusted, the glider would move due the metal changing shape. By adjusting the knob at the bottom of the ramp, the height of the ramp can be shifted so that the ramp is roughly parallel to the ground, but since the track has bent, the glider is likely to be influenced by the effects of gravity on the sides of the ramp. This would have added to the uncertainty of the experiment, since the effects of gravity would now be taking effect.

Furthermore, the VELA records the acceleration based on infra-red light readings during two separate times. The glider consists of two pieces of metal that block out the infra-red light and the time that it is blocked out is used by the machine to calculate the acceleration. However, the two pieces of metal reflect light and may have reflected some of the natural light in the room, onto the reader. This may also have added to the uncertainty in the experiment.

When the ramp was set such that it was horizontal and the glider was placed in the centre, the glider oscillated back and forth. The air rising from the holes in the ramp would brush up against the edge of the glider and push it back. Then the air behind the glider would also brush against the edge of the glider and push it forward.

After the collision of the two gliders, it was noticed that the gliders' final speeds (separating after the collision) was similar to their initial speeds (before the collision). This suggests that the value of the final momentum should be similar to the value of the initial momentum.

After the string between the gliders was cut, the magnetic force of repulsion between the magnets attached to them caused them to travel in separate directions. It was noticed that the heavier glider had a slower speed than the lighter glider. This is necessary for their momentum to be equal (and opposite since their directions are opposite), since p = mv. If m is greater, v will need to be smaller for p to be equal for both gliders.

Raw Data:

Note: The units will be converted into the correct SI units in the processed data.

There were 2 gliders, glider A and glider B. Glider A had a mass of 261g. Glider B had a mass of 309g. Let the uncertainty be half the last digit since the scales used can only measure accurate to 1 gram.

Glider A will always be on the left initially and Glider B will always be on the right initially. Let the direction of the velocity to the right be positive.

The uncertainty of the mass of each glider is +/- 0.5 grams since the scales can only measure accurately to that degree. The uncertainty of the initial and final velocities would in theory be +/- 0.05 mms-1. This will be recorded into the raw data.

However, there are more uncertainties involved in this measurement. It is not possible for the slope of the ramp to be perfectly horizontal, therefore gravity will take effect. Furthermore, the air rising from the holes would also alter the measurement slightly. The light reflecting off the metal plates may also interfere with the result. Also, the light recorder calculates the velocity based on the length of the metal plates. The length of these plates is 100mm +/- 0.5mm. Thus there is much more uncertainty than +/-0.05mms-1.

The uncertainty cannot be quantified, but it would mean that the data can no longer be measured to 4 significant digits. Thus a rough estimate of the uncertainty will be 5mms-1. This is half the last digit of a measurement to 3 significant figures.

The correct number of significant digits will be used in the processed data. For now, it will be left as 4 significant digits since it is the raw data.

Collision Experiment

Glider

Mass+/-0.05(g)

u +/-5(mms-1)

v +/-5(mms-1)

A

261

+1493

-836.0

B

309

-1186

+780.0

Magnetic Repulsion Experiment

Glider

Mass+/-0.05(g)

u+/-5(mms-1)

v+/-5(mms-1)

A

261

0.000

-280.0

B

309

0.000

+230.0

Processed Data: The data will now be converted into SI units as well as their uncertainties.

The mass in the raw data will need to be converted into kg. Thus the uncertainty will become+/-0.0005kg.

The velocity in the raw data will be converted into ms-1. This will only be to 3 significant digits, as explained above and the uncertainty will be 0.005ms-1.

Collision Experiment

Glider

Mass+/-0.0005(kg)

u+/-0.005(ms-1)

v+/-0.005(ms-1)

A

0.261

+1.49

-0.836

B

0.309

-1.19

+0.780

Magnetic Repulsion Experiment

Glider

Mass+/-0.0005(kg)

u+/-0.005(ms-1)

v+/-0.005(ms-1)

A

0.261

0.000

-0.280

B

0.309

0.000

+0.230

Calculating Momentum:

Let the mass of glider A be mA and its initial velocity be uA and its final velocity be vA Let the mass of glider B be mB and its initial velocity be uB and its final velocity be vB

Let the initial momentum of glider A be piA and the final momentum be pfA. Let the initial momentum of glider B be piB and the final momentum be pfB.

Collision Experiment:

piA= mAuA = 0.261x 1.49 = 0.389 Ns

The uncertainty can be calculated by adding the relative uncertainties of the mass and the initial velocity:

Relative error of mass = 0.0005/0.261 = 0.002 Relative error of initial velocity = 0.005/1.49 = 0.003 Sum of relative errors = 0.005 or 0.5% Absolute error = 0.005 x 0.389 = 0.002

Thus piA = 0.39 +/- 0.002 Ns

Using the same method, the other values of momentum, as well as their absolute error can be calculated:

pfA= mAvA = (0.261+/-0.0005) x (-0.836+/-0.005) = - 0.22+/- 0.002 Ns

piB= mBuB = (0.309+/-0.0005) x (-1.19+/-0.005) = - 0.36 +/- 0.002 Ns

pfB= mBvB = (0.309+/-0.0005) x (0.780+/-0.005) = 0.24 +/- 0.002 Ns

Magnetic Repulsion Experiment:

Since uA and uB are both equal to 0, the initial momentum of glider A and glider B are both equal to 0. This is because pi = mu, and m x 0 = 0.

pfA= mAvA = (0.261+/-0.0005) x (-0.280+/-0.005) =- 0.07 +/- 0.001 Ns

pfB= mBv­B = (0.309+/-0.0005) x (0.230+/-0.005) = 0.07 ­+/- 0.002 Ns


IB Physics - IA Example: Data Collection and Processing

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Thursday, November 24, 2011

Orion AstroView 6 Equatorial Reflector Telescope

!±8±Orion AstroView 6 Equatorial Reflector Telescope

Brand : Orion
Rate :
Price : $429.99
Post Date : Nov 25, 2011 06:24:07
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If you're ready to graduate from a small scope or want your first scope to have more light-gathering power than typical starter scopes, step up to the AstroView 6. Its 150mm parabolic mirror has a focal length of 750mm (f/5), so it offers generous wide-field views of deep-sky objects when used with the included 25mm Plossl. For lunar and planetary study, use the 10mm Plossl (also included). The AstroView's EQ-3 equatorial mount features manual slow motion controls, which allow you to center and track objects in the viewing field. An optional single- or dual-axis EQ-3 DC drive is also available for electronic guiding. Built in to the equatorial head is a polar-alignment scope for precise orientation on celestial north or south. The mount couples to a sturdy adjustable aluminum tripod with accessory tray. Includes 6x30 finder, rack-and-pinion focuser, and four-vane adjustable secondary mirror support.

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Monday, November 21, 2011

What Are Reflecting Telescopes Used For?

!±8± What Are Reflecting Telescopes Used For?

Telescopes are scientific instruments. And in a way, backyard astronomy telescopes are also scientific instruments, though on a lesser scale than the Hubble! But, what are reflecting telescopes used for? Are there more uses for a backyard astronomy telescope, than simply pointing and looking? Join me as we take a look at what are reflecting telescopes used for.

There is no doubt that telescopes are scientific instruments. Whether it is NASA or your own telescope, you can look into the heavens and do a lot more than simply see what Jupiter looks like.

The simplest way to use a telescope is to simply point and look. There is some science in it. You need to discover where the object is, and actually find it, and view it.

Another level to this could be the addition of a notebook. Now astronomy gets even more fun! You can now instead of simply viewing Jupiter, draw a picture in your notebook. You can write out your findings.

Over days, and weeks, months and years, these drawings and writings will allow you to get much more out of astronomy. Why? Because each day, each week, there is a change. And this change can be seen.

In the example with Jupiter, the red spot can tell you how long it takes Jupiter to do a revolution - with keen observation. You can measure information about Jupiter's moons and so much more.

We have not even scratched the surface. We have only looked at Jupiter! Imagine looking at Saturn, seeing it closer, seeing it further away, seeing the rings at certain angles, and other times the ring hardly looks like it is there.

This is science at its best, especially with backyard astronomy, and you can fully participate in it. You may not find a planet; however, you will be learning, rather than simply viewing.

A lot of what we know of the Universe is here, because astronomers of the past did these very acts. They took their small telescopes, pointed it to the heavens, and recorded. Today, that information allows us with ease to know where a planet is, its size, and even its mass!

For more advanced studies and findings, you can actually participate in science by searching for meteors and asteroids which may pose a danger to Earth. You can also measure the speed of light, and find out for yourself the size and mass of the planets, and even what they are composed of. However, that will be something that will need your research, passion, and effort to find.

There is a lot to do with reflecting telescopes, and with a bit of investigation, you can get much more out of backyard astronomy. The question is how deep do you want to get into backyard astronomy.


What Are Reflecting Telescopes Used For?

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