For this farsighted person, an object must be 125
cm away from his eyes if he is to see it clearly. For a "normal"
person, the nearpoint is assumed to be 25 cm. The contact lens
must cause an image of the object at 25 cm appear to be 125 cm
on the incident side. This means that the image is erect and
virtual.
We have o = 25 cm and i = -125 cm. Using the lens equation
Thus the focal length of the lens must be f = +31.25
cm. The lens is positive or converging.
The power of a lens is defined
Accounting for the position of the glasses, the
object would be o = 25 cm - 2 cm = 23 cm and i = -(125 cm - 2
cm) = -123 cm.
Using the lens equation
Thus the focal length of the lens must be f = +28.29
cm. The lens is positive or converging.
The power of a lens is defined
For this nearsighted person, an object can be no
farther than 8 cm away from his eyes if he is to see it clearly.
If the object, the newpaper, is 50 cm away, the person needs
the image to be 8 cm away on the incident or object side of the
lens. This means that the image is erect and virtual.
We have o = 50 cm and i = -8 cm. Using the lens equation
Thus the focal length of the lens must be f = -9.52
cm. The lens is negative or diverging.
The power of a lens is defined
Accounting for the position of the glasses, the object
would be o = 50 cm - 2 cm = 48 cm and i = -(8 cm - 2 cm) = -6
cm.
Using the lens equation
Thus the focal length of the lens must be f = -6.86
cm. The lens is negative or diverging.
The power of a lens is defined
Let I0 be the initial light intensity,
then the later intensity when it is cloudy is I = ¼I0.
To properly expose film requires that a specific
amount of light reaches the film. The amount of light reaching
the film is governed by
where I is the intensity of the ambient light, D2
is a measure of the area of the aperture, and t is the time that
the aperture. The area is set by the f-number or f-stop of the
camera. The time is set by the shutter speed. Our adjustments
of the camera must be such that Lfilm is a constant.
(a) Changing only the shutter speed:
| Linitial | = Lfinal |
| I0D2t0 | = (¼I0)D2tf |
Solving for tf, we find
The nearest available shutter setting would actually be 1/60th s.
(b) Changing only the f-number:
| Linitial | = Lfinal |
| I0(D0)2t0 | = (¼I0)(Df)2t0 |
Solving for Df, we find
So we need to increase the aperture area by a factor of 4. Hence
we must move two f-stops, since the area changes by a factor of
two with each change of f-stop. As the f-stop number gets smaller
the area gets bigger, so we need f/2.8.
Let d = 18.0 cm.
(a) The magnification of a telescope is given by
where L = d - f0 - fe = 18.0 cm - 3.00 cm
- 0.20 cm = 14.8 cm and XNP is the nearpoint of the
"normal" person which is set at 25 cm. Thus the magnification
is
The minus sign indicated that the image will be inverted.
(b) In a telescope the object is placed in front of the objective so that the image created by the objective is formed at the focal point of the eyepiece.
We have fo = 0.20 cm and we want i = d - fe
= 18.0 cm - 3.00 cm = 15.0 cm. Note that since the image is on
the transmission side of the objective it is real and I is positive.
Using the lens equation,
Thus the object must be placed 0.203 cm in front of the objective.
The length of the telescope is given by L = f0 + fe.
We are told that
Thus fo = 3fe, and
Questions? mike.coombes@kwantlen.ca