The idea of a focal point is actually an naive idealization.
In theory and in reality, one cannot construct a static lens or mirror that gathers all parallel light rays to an arbitrarily small point.
It would have violated the second law of thermodynamics because such a lens could generate an arbitrarily high temperature from a low temperature light source.
Mathematically it came from the conservation of volume in phase space $\Delta x \Delta p$ in classical mechanics.
Light rays will always miss each other slighlty around the focal point (i.e. slightly blurring the image) due to the above fundamental constraint from physics.
There are two types of lenses:
Coverging lens
Also known as convex lens or positive lens.
Thicker in the middle, thinner on the edge.
Focal length $f$ is always positive.
Diverging lens
Also known as concave lens or negative lens.
Thinner in the middle, thicker on the edge.
Focal length $f$ is always negative.
In this course we will only study symmetrical lenses, so both sides of the lenses are the same.
Converging (convex) lens. Also known as positive lens because $f\gt 0$.Light rays deflected by a converging lens.
There are 3 principle rays: simple rays that are used to find the image.
Click on the Switch Rays button below to see the rules for the principle rays.
Drag the focal point to the other side to change to a diverging lens.
Simulation - Converging and Diverging Lens: The Principle Rays
Drag to move the object, and to change the focal lengths.
Dragging the focal points to the other side of the lens will change the lens from converging to diverging and vice versa.
Click on "Switch Rays" to show one principle ray at a time.
This simulation focuses on showing the rules regarding the principle rays so the image is purposely omitted. See the next simulation to learn how to find the image.
The symbols for the converging lens (left) and diverging lens (right) in a ray diagram. The symbols allow you to draw the lens accurately using rulers.
Image formation
Image is located where the rays meet.
If the rays diverge on the right, then trace the rays backward. The meeting point of the extrapolated rays is the location of the image.
Real vs virtual image
Real image is an image that can be projected onto a screen without additional lenses or mirrors.
Virtual image is an image that cannot be projected onto a screen without additional lenses or mirrors.
Real image is formed when rays converge at a location.
Virtual image is formed when rays diverge, but can be extrapolated backward to a meeting point.
In the case of a single lens, real image is always on the right of the lens, and virtual image is always left of the lens. This is not true for multiple lenses.
Drawing ray diagrams
Draw the ray diagram in 1:1 scale unless you are specifically asked to do otherwise or if the dimensions are clearly too big to fit on a single page.
Use a pencil as opposed to a ball pen so you can erase and perfect your drawing.
Use rulers for every single line.
Light rays should have arrows on them to indicate their directions.
Always mark and label the focal points.
Measure and indicate the image distance on your diagram.
Two rays are sufficient to identify the location of the image. The third principle ray can be used to double check, or you can use the lens equation (see below) to confirm.
For curved mirrors (in later section) you will need a protractor for one of the principle rays.
One ray diagram per page so you have plenty of space.
Practice, practice, practice!
Simulation - Converging and Diverging Lens: Finding the Image
Drag to move the object, and to change the focal lengths.
Dragging the focal points to the other side of the lens will change the lens from converging to diverging and vice versa.
The location of the image can be found using the lens equation:
$$
\frac{1}{p} + \frac{1}{i} = \frac{1}{f}
$$
Always ensure the focal length obeys the rule:
$$
\left\{
\begin{eqnarray}
f &\gt& 0 \hspace{1cm} \text{(converging lens)} \\
f &\lt& 0 \hspace{1cm} \text{(diverging lens)}
\end{eqnarray}
\right.
$$
The image distance obeys the sign convention:
$$
\left\{
\begin{eqnarray}
i &\gt& 0 \hspace{1cm} \text{(image right of the lens)} \\
i &\lt& 0 \hspace{1cm} \text{(image left of the lens)}
\end{eqnarray}
\right.
$$
The red arrows are the images at different lateral magnifications. The postions of the images are arbitrary and are not meant to represent $i$.
Lateral magnification
The magnification is the ratio of the image size $h_i$ to the object size $h_o$, and can be found with the object and image distances:
$$
m = \frac{h_i}{h_o} = -\frac{i}{p}
$$
When $m \lt 0$, the image is inverted and $h_i \lt 0$.
When $|m| \lt 1$, the image is diminished.
When $|m| \gt 1$, the image is magnified.
Describing the image
If you are asked to describe the image, it means answering three questions:
Is the image upright or inverted?
Is the image magnified or diminished?
Is the image real or virtual?
Converging lens is complicated, but a diverging lens always produces images that are:
Upright.
Diminished.
Virtual.
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When the object is on the focal point of a converging lens (i.e. $p=f$, the case between the two exercises above), the outgoing light rays are parallel and therefore never meet. We either say "no image is formed", or "the image is at infinity".
A converging lens viewing objects far away ($p \gt f$). The image is inverted ($m \lt 0$). For $p\gt 2f$ (such as the house in the figure), the image is also diminished ($|m|\lt 1$).
A converging used as an magnifying glass when the object is put between $F$ and the lens ($p \lt f$). Note that the image is magnified ($m \gt 1$) and the object is upright ($m$ positive).
Drag to move the object, and to change the focal lengths.
Dragging the focal points to the other side of the lens will change the lens from converging to diverging and vice versa.
Curved Mirrors
A reflective surface acting as a diverging (convex) mirror.
Curved mirrors are sometimes inaccurately called parabolic or spherical mirrors, although they are usually not strictly parabolic or spherical in shape.
A curved mirror has only one focal point, as opposed to the two in a lens.
When the mirror is approximately spherical, the point $2F$ is sometimes called the center of curvature, denoted $C$. It represents the center of the sphere.
$R = 2f$ is called the radius of curvature.
There are two types of curved mirrors:
Coverging mirror
Also known as concave mirror or positive mirror.
Focal length $f$ is always positive.
Sole focal point $F$ lies in front of the mirror.
The ray diagram most analogous to that of the converging lens.
Diverging mirror
Also known as convex mirror or negative mirror.
Focal length $f$ is always negative.
Sole focal point $F$ lies behind the mirror.
The ray diagram most analogous to that of the diverging lens.
Can only produce upright, diminished, virtual images.
Principle rays
There are 3 principle rays: simple rays that are used to find the image.
Click on the Switch Rays button below to see the rules for the principle rays.
Drag the focal point to the other side to change to a diverging mirror.
Simulation - Converging and Diverging Mirrors: The Principle Rays
Drag to move the object, mirror, and to change the focal length.
Dragging the focal point to the other side of the mirror will change the mirror from converging to diverging and vice versa.
Click on "Switch Rays" to show one ray at a time.
This simulation focuses on showing the rules regarding the principle rays so the image is purposely omitted. See the next simulation to learn how to find the image.
The symbols for the converging mirror (left) and diverging mirror (right) in a ray diagram. The symbols allow you to draw the mirrors accurately using rulers.
The same equations apply for curved mirrors.
Lateral magnification:
$$
m = \frac{h_i}{h_o} = -\frac{i}{p}
$$
The lens equation:
$$
\frac{1}{p} + \frac{1}{i} = \frac{1}{f}
$$
Always ensure the focal length obeys the rule:
$$
\left\{
\begin{eqnarray}
f &\gt& 0 \hspace{1cm} \text{(converging mirror)} \\
f &\lt& 0 \hspace{1cm} \text{(diverging mirror)}
\end{eqnarray}
\right.
$$
The image distance obeys the sign convention:
$$
\left\{
\begin{eqnarray}
i &\gt& 0 \hspace{1cm} \text{(image left of (in front of) the mirror)} \\
i &\lt& 0 \hspace{1cm} \text{(image right of (behind) the mirror)}
\end{eqnarray}
\right.
$$
Simulation - Converging and Diverging Mirrors: Finding the Image
Drag to move the object, mirror, and to change the focal length.
Dragging the focal point to the other side of the mirror will change the mirror from converging to diverging and vice versa.
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View of a diverging mirror. The image is upright, diminished, and virtual.