Vernier Optics Expansion Kit User Manual

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Sample Experiments: Real Image Formation

The thin lens equation is

o

i

f

1

1

1

where f is the lens focal length, i is the image to lens distance, and o is the object to
lens distance. Sign convention for f is positive for converging lenses, negative for
diverging. The variable i is positive if the (real) image is in back of the lens, and
negative if the (virtual) image is in front. The variable o is positive if the (real) object
is in front of the lens, and negative if the (virtual) object is behind the lens.
This relationship can be verified using the Optics

Expansion Kit. Place the light source near the end

of the track, with the luminous source facing along

the longer length of the track. Insert the 100 mm

focal length lens into a holder, and place it 15 cm

from the light source plane. Place the screen on the

side of the lens opposite the light source. Where do

you find a sharp image? Is it where you expect it

using the thin lens equation?
The linear magnification M of a lens is

o

i

h

h

o

i

M

where h

i

is the image height, and h

o

is the object height. Use a ruler to measure the

height of the image and object. Does the linear magnification you observe match the

prediction?

Sample Experiments: Inverse Square Law

This experiment requires a light sensor, interface, and associated software. In this

example we will use Logger Pro software, a Go! Link, and a Vernier Light Sensor.
Position the light source so that the LED is exposed and is facing down the length of

the track. Read the position using the back edge of the carriage for the light source.
Attach a light sensor to the light sensor holder. Insert a Vernier Light Sensor until it

reaches the stop. The location of the sensor can then be read from the arrows on the

base. Position the sensor so it is pointing directly at the light source. Allow the light

source to stabilize for 15 minutes before collecting data. The intensity falls slightly

as the LED warms, so for this experiment, warm-up time is required.







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Collect intensity data as a function of distance. Sample data with curve fits are

shown in the following two graphs.

The light intensity follows the expected inverse-square relationship well. Another
way to show this relationship is to graph light intensity vs. the inverse of the squared
distances. The resulting graph should be a direct proportionality. The next graph
shows this result.

The room was partially darkened during data collection. If there is substantial

background light, both graphs would be shifted upward, and the fits would require

an additive term.

Additional Experiments

 Make a telescope by combining convex lenses at the sum of focal lengths.
 Study the effect of lens size and shape on image formation. Set up the luminous

source, a converging lens, and the screen so that you see a real image on the

screen. Position the aperture plate as close to a lens as possible, and observe the

effect of different size apertures. You may need to dim the room lights to see the

changes. What will happen with the D-shaped opening?

 Study depth-of-field by casting a real image of the two slits on the screen, and

then take it out of focus by moving the screen until you can no longer resolve the

two lines. Use the aperture plate to make the working diameter of the lens

smaller. How does this change the image?

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