Optics and Ray Diagrams lab
docx
keyboard_arrow_up
School
Nassau Community College *
*We aren’t endorsed by this school
Course
101
Subject
Astronomy
Date
Dec 6, 2023
Type
docx
Pages
9
Uploaded by ChancellorBarracuda1362
Optics and Ray Diagrams
Ray Diagrams
Before you start your ray diagrams, watch the following video that I have made
explaining how to do a ray diagram.
You should also print out the note from
blackboard on Ray Diagrams (under the Lab Notes heading).
This has all the
definitions that I will describe on the video.
How to do a Ray Diagram:
https://youtu.be/jA6DSa7Doa0
For the following two problems, you will be creating a ray diagram for a lens with
the following characteristics:
f = 3 cm diameter
= 8 cm
Object height (h
o
) = 3 cm
Problem 1:
Object distance = 12 cm
Problem 2:
Object distance = 8 cm
For the next two ray diagrams, you will be creating a ray diagram for a lens with
the following characteristics:
f = 5 cm diameter
= 8 cm
Object height (h
o
) = 3 cm
Problem 3:
Object distance = 12 cm
Problem 4:
Object distance = 3 cm
Some of you may need help to complete problem 4, I have recorded the following
video to help you with this so just click the following link.
How to do a Ray Diagram for a Virtual Image:
https://youtu.be/5TN1sRotyCU
We have two types of images that can be created by a lens, a real image and a
virtual image.
A real image is an image that can be projected onto a screen.
A real
image is almost always on the opposite side of the lens and inverted when
compared to the object.
A virtual image is an image that appears to come from a
point but is not actually there.
This image almost always on the same side of the
lens and erect when compared to the object.
Using the images formed by your ray diagrams fill the information asked for in the
following table.
Problem
Real or
Virtual
Inverted or
Erect
Image Size
(cm)
Magnification =
h
i
/h
o
1
Real
inverted
0.8 cm
0.267
2
Real
inverted
1.9 cm
0.633
3
Real
inverted
1.7 cm
0.567
4
Real
inverted
1.875 cm
-0.625
Questions
1)
What is the relationship between the object distance from the lens and the image
size? - The relationship between the object distance and image size depends on
the type of lens and the position of the object relative to the lens. Converging
lenses can form both real and virtual images, and the image size varies based on
the object distance. Diverging lenses always form virtual, reduced-size images.
2)
What is the relationship between the focal length of the lens and the image size? -
Generally, for converging lenses (convex lenses), when the focal length
increases, the image distance increases, and the image size decreases.
Conversely, when the focal length decreases, the image distance decreases, and
the image size increases. For diverging lenses (concave lenses), the relationship
is a bit different. When the focal length increases, the image distance decreases,
and the image size also decreases. When the focal length decreases, the image
distance increases, and the image size increases.
Ray Diagrams of Telescopes
Figure #1: This figure shows the ray diagram of a telescope made with two lenses.
Use figure #1 and the following information to the to answer questions.
The object is 10 cm from the objective lens and is 3 cm in height.
The focal length
of the objective lens is 5 cm and is labeled as F
1
in the figure. The image the
objective produces is 2.7 cm in height.
The image of the objective lens is the object for the eyepiece (this is the same as if
we placed an object at this point).
The eyepiece has a focal length of 3 cm and the
image it produces is 8.5 cm in height.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help
3)
What type of image is produced by the objective? By this I mean real and
inverted, or virtual and erect. -
When the object is placed beyond the focal
length of a converging lens (like the objective lens in this case), the lens
converges the incoming light rays to form a real image on the opposite side of
the lens. The image will be inverted, meaning it is upside down compared to
the object. In summary, when the object is beyond the focal length of the
objective lens, the image formed will be real and inverted, regardless of the
object's height.
4)
What type of image is produced by the eyepiece? -
A virtual image is an image
that appears to be in a location where light does not actually reach. It cannot
be projected onto a screen. In the context of eyepieces, the eyepiece creates a
virtual image that appears to be at a certain distance from the eyepiece. This
virtual image is what the observer perceives when looking through the
eyepiece. So, the image produced by the eyepiece is virtual, meaning it's an
image that the observer sees through the eyepiece, and it is magnified to
enhance the details of the observed object.
5)
What type of image is produced by the telescope? -
The type of image
produced by the telescope can be real and inverted or virtual and erect,
depending on the specific design and components of the telescope.
Astronomical telescopes commonly produce inverted images, as the
orientation of celestial objects is not relevant for astronomical observations.
Terrestrial telescopes, on the other hand, often include additional optics to
produce virtual and erect images for convenient terrestrial viewing.
6)
Using the equation for magnification in the previous section, calculate the
magnification of the objective lens.
-
M
objective = −
Imageheight
(
h
1
)
Objectheight
(
h
)
-
m
objective =
−
2.7
cm
3
cm
= -0.9
-
The negative sign indicates that the image is inverted compared to the
object, which is a common convention in optics. So, the magnification of the
objective lens is mobjective= -0.9
7)
Calculate the magnification of the eyepiece? - Magnification of the eyepiece is
approximately 1.111
m
objective =
−
2.7
cm
3
cm
= -0.9
−1 = (−0.9) ×
m
eyepiece
m
eyepiece =
−−
1
−
0.9
m
eyepiece ≈ 1.111
8)
Knowing that the image seen through the eyepiece is the image of the
telescope, calculate the magnification of the telescope.
-
m
total=
m
objective ×
m
eyepiece
-
m
total = ( −0.9) × (1.111)
-
m
total ≈ −1
-
The negative sign indicates that the final image is inverted. The total
magnification of the telescope is approximately -1. This means that the image
seen through the telescope appears inverted and at the same size as the
original object, which is a common configuration for astronomical telescopes
.
9)
According to theory, if we multiply the magnification of the objective by the
magnification of the eyepiece we should get the magnification of the telescope.
Do this calculation to prove that this is true.
-
m
total =
m
objective ×
m
eyepiece
-
mtotal = (−0.9) × (1.111)
-
m
total ≈ −1
-
The calculated total magnification (
m
total) is approximately -1. This result
confirms that multiplying the magnification of the objective by the
magnification of the eyepiece yields the magnification of the telescope, as
per the theoretical expectation.
Optics
We have two types of lenses a convex or converging lens and a concave or
diverging lens.
These two lenses can be seen in Figure #2.
Figure #2 ray diagrams of a converging and a diverging lens.
A converging lens takes light that enters it and bends or refracts the light so that
they will meet at a single point.
If the light that enters the lens is infinitely far
away that point is called the focal length.
A diverging lens takes light rays that
enter it and spreads them out.
If you extend the rays that exit the lens backwards,
they will meet at a single point in front of the lens as seen in figure 2.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help
These two images are of two converging lenses.
The one on the left has a focal
length of 10 cm; the one on the right has a focal length of 20 cm.
In both images,
the object is placed 30 cm away from the lens.
10)
What is the relationship between the brightness of the image and the focal
length of the lens? -
The relationship between the brightness of the image and
the focal length of the lens is indirect. It is primarily determined by the size of
the lens's aperture. A larger aperture allows more light to pass through,
resulting in a brighter image, while a smaller aperture restricts the amount of
light, leading to a dimmer image. The focal length itself does not directly
influence the brightness; it is the aperture size that plays a key role in
determining the brightness of the formed image.
These two images show a 10 cm focal converging lens.
The photo on the right
shows the image resulting from the lens with its full aperture.
The image on the
left shows the same lens, but with an image formed using a 3 cm aperture.
11)
What is the relationship between image brightness and the aperture of the
lens? -
The relationship between image brightness and the aperture of the lens
is straightforward: a larger aperture allows more light, leading to a brighter
image, while a smaller aperture restricts light, resulting in a dimmer image.
Photographers often use different aperture sizes (expressed as f-numbers) to
control the exposure and depth of field in their photographs, understanding the
impact of aperture on image brightness is fundamental to capturing well-
exposed images.
If we were to build a telescope with two converging lenses, the magnification is
given by:
?
𝑜𝑏𝑗𝑒𝑐𝑡𝑖𝑣𝑒
𝑀=
?
𝑒𝑦𝑒𝑝𝑖𝑒𝑐𝑒
We have four lenses:
Lens
Focal Length (cm)
A
4
B
3.5
C
10
D
3
Calculate the magnification of the following combinations of lenses:
Objective
Eyepiece
Magnification
C
A
2.5
C
B
2.857
C
D
2.33333
From your answers in the table, what is the relationship between the focal length
of an eyepiece and the magnification of a telescope? -
As the focal length of the
eyepiece decreases, the magnification of the telescope increases. There is an
inverse relationship between the focal length of the eyepiece and the
magnification of the telescope: when the eyepiece focal length is shorter, the
resulting magnification is higher. This relationship is a fundamental principle in
telescope optics. Shorter focal length eyepieces provide higher magnification,
allowing you to observe distant objects in greater detail.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help