Understanding the Thin & Gaussian Lens Equations

In summary, a lens is a tool used to focus or collimate light rays from an object, and there are various equations such as the Gaussian lens formula and thin lens equation used to relate the object and image distances and calculate the magnification. Additionally, the sign conventions and refractive index for different materials were discussed. It is important to note that a physical object is always real, but virtual objects can occur in multi-lens systems.
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Definition/Summary

A lens is most often used to focus light rays from an object to form an image. It can also be used to collimate light rays from an object, or to bring a collimated beam of light rays to a focus.

Equations

See "Extended explanation" for definitions of terms.

The well-known Gaussian lens formula uses the focal length to relate the object and image distances for a thin lens:

[tex]
\frac{1}{d_o} + \frac{1}{d_i} = \frac{1}{f}
[/tex]

Different notation is often used, so that the Gaussian lens formula is sometimes written:

[tex]
\frac{1}{s_o} + \frac{1}{s_i} = \frac{1}{f}
[/tex]

or

[tex]
\frac{1}{o} + \frac{1}{i} = \frac{1}{f}
[/tex]

Note that while the letter "o" resembles the number "0", it is NOT (in general) zero.

The thin lens equation or lensmaker's formula uses the lens's surface curvatures and refractive index:

[tex]
\frac{1}{d_o} + \frac{1}{d_i} =
(n_{lens}-1)(\frac{1}{R_L}-\frac{1}{R_R})
[/tex]

Note that the right-hand-side is equivalent to 1/f.

The image is magnified (with respect to the size of the object) by the factor

[tex]
m = - \ \frac{d_i}{d_o}
[/tex]

A curved mirror surface with radius of curvature R obeys the Gaussian lens formula with

[tex]
f = R/2
[/tex]

or, equivalently,

[tex]
1/f = 2/R
[/tex]

Extended explanation

Term definitions:

do (or so or o), the object distance, is the distance from the object to the lens
di (or si or i), the image distance, is the distance from the image to the lens
f is the focal length of the lens
nlens is the refractive index of the lens material
RL and RR are the radii of curvature for the left- and right-hand lens surfaces, respectively.Sign conventions:

do is positive for a real object and negative for a virtual object (See images below).
di is positive for a real image and negative for a virtual image (See images below).
do is ∞ if the incident rays are collimated, and di is ∞ if the outgoing rays are collimated.
f is positive for converging (eg. biconvex and plano-convex) lenses, and negative for diverging (eg. biconcave and plano-concave) lenses.
RL and RR are positive if the "bulge" (convex side) is toward the left, and negative when the bulge is toward the right:
( R is +
) R is -​
R = ∞ (and 1/R = zero) for a flat surface.
R and f are positive for a concave mirror and negative for a convex mirror.

For the common situation where the object and image are real (do and di both positive), the magnification is negative indicating an inverted image with respect to the object.

If the medium surrounding the lens has a refractive index other than 1, then replace the term
(nlens - 1)​
with
(nlens/nmedium - 1)​
in the thin lens equation.Real or virtual?

These figures illustrate the three most common situations where the object and image are real or virtual.

Lens_RealObj_RealImg.gif


Lens_RealObj_VirtImg.gif


Lens_VirtObj_RealImg.gif

Note: a physical object is always real. Virtual objects can occur in multi-lens systems, when the object for one lens results from the image of a previous lens.

The situation where both object and image are virtual is rare, at least in physics homework exercises. This is possible only for a negative (i.e. diverging) lens.Refractive index for common materials:

Vacuum: n = 1 exactly
Air: n = 1.0003, typically approximated by 1
Water: n = 1.34, average over visible range
Glass: n = 1.5 is typically used in optics homework problems
Fused silica (pure SiO2 glass): 1.46, average over visible range

* This entry is from our old Library feature, and was originally created by Redbelly98.
 
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Thanks for the overview of a lens
 

What is the Thin Lens Equation?

The Thin Lens Equation is a mathematical formula that relates the distance of an object from a lens, the distance of the image from the lens, and the focal length of the lens. It is used to calculate the magnification and position of an image formed by a thin lens.

What is the Gaussian Lens Equation?

The Gaussian Lens Equation is a more general form of the Thin Lens Equation that takes into account the curvature of the lens. It is used to calculate the position and size of an image formed by a lens with a curved surface.

How do the Thin and Gaussian Lens Equations differ?

The Thin and Gaussian Lens Equations differ in their assumptions and level of accuracy. The Thin Lens Equation assumes that the lens is thin (negligible thickness) and the Gaussian Lens Equation takes into account the curvature of the lens. The Gaussian Lens Equation is more accurate for lenses with a curved surface.

What factors affect the Thin and Gaussian Lens Equations?

The Thin and Gaussian Lens Equations are affected by the distance of the object and image from the lens, the focal length of the lens, and the curvature of the lens. They are also affected by the index of refraction of the medium in which the lens is placed.

How are the Thin and Gaussian Lens Equations used in real-world applications?

The Thin and Gaussian Lens Equations are used in various fields such as optics, photography, and engineering to design and analyze optical systems. They are also used in medical imaging, telescope design, and other applications that involve the use of lenses.

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