Wednesday, October 3, 2012

Lenses Lab

The purpose of this lab is to study how converging lenses behave when a light source is present. For this lab we used a thin converging lens, a light box and a meter stick. We also needed a clear background so that the shape would be projected clearly.

We began by first finding out the focal length of the lens. To do this, we needed a light source that would offer infinite object distance, so we took the Sun as our light source.






We measured the focal length of the lens to be 4.8±.03 cm. Once the focal lenght was known, we set up a meter stick that worked as a rail on which the lens would be attached. The light source would make a projection that would go through the lenses, showing the shape of a plastic film in front of the light box. 



Having the focal lenght, we started placing the lens in intervals along the meter stick. First we started by placing the lens 4 focal length distances away from the light source. 



The distance was measured to be o = 20.0±.3 cm. 
We also measured the distance from the lens to the image on the clear surface to be di = 5.4±.2 cm. The height of the filament was recorded to be h = 9.2±.2 cm, whereas the height of the projected image was measured to be hi = 2.9±.2 cm. 

The magnification is equal to:

hi/ h = 2.9±.2 / 9.2±.2 =  0.32±0.023

Qualitatively, the projected image appeared inverted. The projection was a real image of the object.

Reversing the lenses did not changed the measurements obtained above. 

We then changed the distance so that the lens would be 2 focal length distances away.

This distance now was o = 10.0±.2 cm. with an image distance of di = 8.6±.2 cm.
The heights were measured to be the same h = 9.2±.2 cm. for the object, and hi = 7.3±.2 cm. for the image, and magnification M =  0.79±0.028.

The displayed image seemed to get bigger now that we were closer to the filament. Again, nothing changed when reversing the lens.

  
With now a distance of 1.5 focal lengths, the distance changed to be o = 7.5±.2 cm. and di = 10.5±.3 cm.

The heights measurements for the object were h = 9.2±.2 cm and hi = 13.0±.1 cm. and M=1.41±0.033 with no change in the reversed lens technique.

If the lens were to be covered in half, I predicted that only half the image would be visible. This turned out to be not right. When doing so, the complete image still went through the lens, but the projection was dimmer. This is probable due to the light rays traveling around the lens, but with decreased intensity due to the covered up portion. 



dâ‚’ (cm) d₁ (cm) hâ‚’ (cm) h₁ (cm) M  Type of image
5f = 25.0±.2 6.0±.2 9.2±.2 2.1±.1 0.23±0.012 Real/Inverted
4f = 20.0±.2 5.4±.2 9.2±.2  2.9±.2 0.32±0.023 Real/Inverted
3f = 15.0±.2 6.4±.2 9.2±.2 3.8±.2 0.41±0.024 Real/Inverted
2f = 10.0±.2 8.6±.2 9.2±.2 7.3±.2 0.79±0.028. Real/Inverted
1.5f =  7.5±.2  10.5±.3 9.2±.2 13.0±.1 1.41±0.033 Real/Inverted


When trying to measure a focal length of 0.5f, the image turned out to be quite big. This made measuring the image height impossible. However, when looking through the lens, the image was clear and small.






dâ‚’ (cm) d₁ (cm) hâ‚’ (cm) h₁ (cm) M  Type of image Inverse d₁ (cm^-1) Neg. Inverse dâ‚’ (cm^-1)
5f = 25.0±.2 6.0±.2 9.2±.2 2.1±.1 0.23±0.012 Real/Inverted 0.167±.0056 -0.0400±.00032
4f = 20.0±.2 5.4±.2 9.2±.2  2.9±.2 0.32±0.023 Real/Inverted 0.185±.0069 -0.0500±.00050
3f = 15.0±.2 6.4±.2 9.2±.2 3.8±.2 0.41±0.024 Real/Inverted 0.156±.0049 -0.0667±0.00089
2f = 10.0±.2 8.6±.2 9.2±.2 7.3±.2 0.79±0.028. Real/Inverted 0.116±.0027 -0.100±.0020
1.5f =  7.5±.2  10.5±.3 9.2±.2 13.0±.1 1.41±0.033 Real/Inverted 0.095±.0027 -0.133±.0036



When analyzing the data in this last graph, I had to take out the point (-0.0400±.00032,0.167±.0056) out of the population so that it would yield a better trendline. I treated that last point as foul data to yield a slope of 1.075±.1454. The y-intercept came out to be 0.2379±0.01353. This suggests the relationship 1/f = 1/s +1/s', and a expression of the form  d₁ = 1.075±.1454dâ‚’ + 0.2379±0.01353.

Potential sources of error for this experiment are the amount of uncertainty when trying to get perfect focus in measuring d₁. Determining the focal length can also influence the change for getting large uncertainties, and extra-ordinary data points in the graphs.

No comments:

Post a Comment