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Minimum deviation
View on WikipediaIn a prism, the angle of deviation (δ) decreases with increase in the angle of incidence (i) up to a particular angle. This angle of incidence where the angle of deviation in a prism is minimum is called the minimum deviation position of the prism and that very deviation angle is known as the minimum angle of deviation (denoted by δmin, Dλ, or Dm).



The angle of minimum deviation is related with the refractive index as:
This is useful to calculate the refractive index of a material. Rainbow and halo occur at minimum deviation. Also, a thin prism is always set at minimum deviation.
Formula
[edit]This section needs expansion with: the derivation of the expression for minimum deviation using Calculus. You can help by adding to it. (June 2020) |
In minimum deviation, the refracted ray in the prism is parallel to its base. In other words, the light ray is symmetrical about the axis of symmetry of the prism.[1][2][3] Also, the angles of refractions are equal i.e. r1 = r2. The angle of incidence and angle of emergence equal each other (i = e). This is clearly visible in the graph below.
The formula for minimum deviation can be derived by exploiting the geometry in the prism. The approach involves replacing the variables in the Snell's law in terms of the Deviation and Prism Angles by making the use of the above properties.
From the angle sum of ,
Using the exterior angle theorem in ,
This can also be derived by putting i = e in the prism formula: i + e = A + δ
From Snell's law,
[4][3][1][2][5][excessive citations]
(where n is the refractive index, A is the Angle of Prism and Dm is the Minimum Angle of Deviation.)
This is a convenient way used to measure the refractive index of a material(liquid or gas) by directing a light ray through a prism of negligible thickness at minimum deviation filled with the material or in a glass prism dipped in it.[5][3][1]
Worked out examples:
The refractive index of glass is 1.5. The minimum angle of deviation for an equilateral prism along with the corresponding angle of incidence is desired.
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Answer: 37°, 49° Solution: Here, A = 60°, n = 1.5 Plugging them in the above formula,
Also,
This is also apparent in the graph below. |
If the minimum angle of deviation of a prism of refractive index 1.4 equals its refracting angle, the angle of the prism is desired.
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Answer: 60° Solution: Here,
Using the above formula,
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Also, the variation of the angle of deviation with an arbitrary angle of incidence can be encapsulated into a single equation by expressing δ in terms of i in the prism formula using Snell's law:
Finding the minima of this equation will also give the same relation for minimum deviation as above.
Putting , we get,
, and by solving this equation we can obtain the value of angle of incidence for a definite value of angle of prism and the value of relative refractive index of the prism for which the minimum angle of deviation will be obtained. The equation and description are given here

For thin prism
[edit]In a thin or small angle prism, as the angles become very small, the sine of the angle nearly equals the angle itself and this yields many useful results.
Because Dm and A are very small,
Using a similar approach with the Snell's law and the prism formula for an in general thin-prism ends up in the very same result for the deviation angle.
Because i, e and r are small,
From the prism formula,
Thus, it can be said that a thin prism is always in minimum deviation.
Experimental determination
[edit]This section needs expansion with: virtual simulation, video, detailed explanation, etc. You can help by adding to it. (May 2020) |
Minimum deviation can be found manually or with spectrometer. Either the prism is kept fixed and the incidence angle is adjusted or the prism is rotated keeping the light source fixed.[6][7][8]
Minimum angle of dispersion
[edit]
This section needs expansion. You can help by adding to it. (May 2020) |
The minimum angle of dispersion for white light is the difference in minimum deviation angle between red and violet rays of a light ray through a prism.[2]
For a thin prism, the deviation of violet light, is and that of red light, is . The difference in the deviation between red and violet light, is called the Angular Dispersion produced by the prism.
Applications
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One of the factors that causes a rainbow is the bunching of light rays at the minimum deviation angle that is close to the rainbow angle (42°).[3][9]

It is also responsible for phenomena like halos and sundogs, produced by the deviation of sunlight in mini prisms of hexagonal ice crystals in the air bending light with a minimum deviation of 22°.[3][10]
See also
[edit]References
[edit]- ^ a b c d "Chapter Nine, RAY OPTICS AND OPTICAL INSTRUMENTS". Physics Part II Textbook for Class IX (PDF). NCERT. p. 331.
- ^ a b c "Optics-Prism". A-Level Physics Tutor.
- ^ a b c d e Mark A. Peterson. "Minimum Deviation by a Prism". mtholyoke. Mount Holyoke College. Archived from the original on 2019-05-23.
- ^ a b "Refraction through Prisms". SchoolPhysics.
- ^ a b "Prism". HyperPhysics.
- ^ "Angle of Minimum Deviation". Scribd.
- ^ "Experimental set up for the measurements of angle of minimum deviation using prism spectrometer". ResearchGate.
- ^ "Theory of the Prism Spectrometer - Experiment | UKEssays.com". www.ukessays.com. Retrieved 2025-03-11.
- ^ "Rainbow". www.schoolphysics.co.uk.
- ^ "Halo 22°". HyperPhysics.
External links
[edit]- Minimum Deviation Part 1 and Part 2 at Khan Academy
- Refraction through a Prism in NCERT Textbook
- Minimum Deviation by Prism Archived 2019-05-23 at the Wayback Machine by Mark A Peterson, Mount Holyoke College
Minimum deviation
View on GrokipediaFundamentals
Definition and Principles
Minimum deviation in the context of prism optics refers to the smallest angle by which a ray of light is deflected when passing through a prism, achieved under specific conditions of incidence that result in a symmetric path of the light ray inside the prism. This phenomenon occurs when the angle of incidence on the first face of the prism equals the angle of emergence from the second face, leading to equal angles of refraction at both surfaces and a balanced bending of the light path.[4][5] The total deviation is minimized because the light ray travels in a way that the refractions at the two faces contribute equally to the overall deflection, avoiding the larger bends that occur with asymmetric incidence angles.[6] The underlying principles stem from the refraction of light at the boundaries between media of different refractive indices, governed by Snell's law, which describes how the direction of a light ray changes upon entering or exiting the prism material. When monochromatic light enters a prism, it bends toward the normal at the first face due to the higher refractive index of the glass compared to air, travels straight through the interior, and then bends away from the normal at the second face upon emergence. The net effect is a deviation of the emergent ray from the original incident direction, with the minimum deviation representing the optimal configuration for the least overall angular shift.[7][8] The systematic application of minimum deviation in optical spectroscopy emerged in the early 19th century, building on earlier work such as Isaac Newton's 17th-century prism experiments, notably through the work of Joseph von Fraunhofer, who in 1814 employed high-quality prisms to analyze the solar spectrum and identify dark absorption lines, laying foundational techniques for spectral dispersion.[9] Fraunhofer's precise prism-based observations utilized minimum deviation to achieve clear separation of wavelengths without excessive light bending, influencing subsequent developments in astronomical and chemical analysis.[9] A typical ray diagram for minimum deviation illustrates a light ray entering the prism at an angle such that the internal path is parallel to the base in an equilateral prism, with the incident and emergent rays forming symmetric angles relative to the prism apex; in contrast, diagrams for higher deviations show asymmetric paths where the ray strikes one face more obliquely than the other, resulting in greater total bending.[6] This symmetry underscores the principle that minimum deviation corresponds to the condition where the prism's dispersive effect is maximized relative to the angular spread.[4]Angle of Deviation in Prisms
When a ray of light passes through a prism, refraction occurs at both the incident and emergent faces according to Snell's law, which states that for the first face, , and for the second face, , where and are the refractive indices of the surrounding medium and prism material, respectively, and are the angles of incidence and emergence, and and are the angles of refraction inside the prism.[10] These relations determine the bending of the ray at each interface, with the sum of the internal refraction angles equaling the prism's apex angle .[3] The total angle of deviation represents the net change in direction of the light ray after traversing the prism, calculated as , where is the angle of incidence at the first face, is the angle of emergence at the second face, and is the fixed apex angle of the prism.[10] This deviation arises from the cumulative refraction effects at the two non-parallel faces, altering the ray's path relative to its initial direction.[3] The magnitude of is influenced by several key factors: the prism angle , which directly scales the deviation as it widens the angular separation between faces; the refractive index of the prism material, where higher enhances bending and thus increases ; and the wavelength of the incident light, since varies with wavelength (dispersion), leading to greater deviation for shorter wavelengths like blue light compared to longer ones like red.[10][3] A typical plot of versus the angle of incidence exhibits a characteristic curve that decreases to a minimum value before increasing again, with the curve displaying asymmetry due to the nonlinear relationship between incidence and emergence angles governed by Snell's law. This minimum point corresponds to the condition of minimum deviation, where the ray path through the prism is symmetric.[10]Theoretical Framework
Condition for Minimum Deviation
The condition for minimum deviation in a prism occurs when the angle of incidence equals the angle of emergence , resulting in a symmetric ray path through the prism.[1][11] In this configuration, the light ray experiences equal refraction at both faces of the prism, minimizing the total angular deviation . For an equilateral prism with apex angle , this symmetry implies that the ray travels parallel to the base inside the prism.[12] This minimum arises because the deviation angle as a function of the angle of incidence exhibits a graphical minimum at the symmetric point, as observed in plots of versus .[13] Physically, the equal bending at the two refracting surfaces ensures that the total deflection is as small as possible for a given prism material, avoiding asymmetric paths that would increase the overall deviation. This condition can also be understood through the principle of least action or calculus of variations, where the symmetric path represents the extremum in ray trajectory.[1] Under the minimum deviation condition, the angles of refraction at the two faces satisfy , where is the prism's apex angle, further reinforcing the internal symmetry.[12] For a fixed apex angle , the minimum deviation is unique and directly depends on the refractive index of the prism material, making this condition a key indicator of the medium's optical properties.[14]Derivation of Refractive Index Formula
The angle of deviation for a light ray traversing a prism with apex angle is expressed as , where is the angle of incidence at the first face and is the angle of emergence at the second face.[10] This relation arises from the geometry of the ray path, considering the sum of the external angles and relative to the internal traversal across angle .[15] Under the condition of minimum deviation , the ray path through the prism exhibits symmetry, such that and the angles of refraction at the two faces are equal, .[10] From the prism's internal geometry, the sum of the refraction angles equals the apex angle, so , which simplifies to under this symmetry.[2] Applying Snell's law at the first face of the prism, where the ray transitions from air (refractive index approximately 1) to the prism material with refractive index , yields .[15] Substituting gives .[10] By symmetry, Snell's law at the second face confirms the same relation, as and , ensuring consistency: .[2] To relate to the minimum deviation angle, consider the overall ray geometry. The total deviation bends the ray by at the first face and at the second, but with symmetry, this combines such that .[15] Substituting this into the Snell's law equation produces .[10] Rearranging for the refractive index gives the standard formula: This equation allows direct computation of from measured values of and .[2] This derivation assumes monochromatic light to define a single refractive index , avoiding complications from wavelength-dependent dispersion, and holds for general prism apex angles without invoking small-angle approximations.[15]Experimental Methods
Setup and Procedure
The standard laboratory setup for measuring the angle of minimum deviation in a prism utilizes a spectrometer, which includes a collimator to produce parallel light rays, a rotatable prism table to hold the sample, a telescope for observing the deviated beam, and an angular scale with verniers for precise measurements.[16][17] A monochromatic light source, such as a mercury vapor lamp providing discrete spectral lines (e.g., yellow at 579 nm), illuminates a narrow adjustable slit in the collimator to ensure sharp imaging.[18][19] The prism, typically made of glass or another transparent material, is placed on the table for rotation. The procedure involves several key steps to ensure accurate alignment and measurement:- Level the spectrometer base and prism table using built-in screws and a spirit level to align all optical axes vertically.[19][18]
- Adjust the telescope eyepiece for clear crosshairs and focus on a distant object to set it for infinity (parallel rays); then, illuminate the collimator slit and fine-tune the collimator lens until the slit image is sharp and vertical in the telescope field.[16][17]
- Place the prism on the table with its refracting edge parallel to the slit and apex toward the collimator; rotate the table to observe reflections from the two prism faces through the telescope, recording vernier positions to calculate the prism angle A as half the difference between these positions.[18][19]
- Reposition the prism so light enters one face and exits the other; without the prism, note the "direct" telescope position for the collimated beam, then insert the prism and rotate the table while viewing a specific spectral line (e.g., the yellow mercury line) until the image appears stationary, indicating minimum deviation—clamp the table and record the telescope position to find δ_m as the angular difference from the direct position.[16][17]
- For greater precision, vary the angle of incidence i by rotating the prism table in increments around the minimum, measure the corresponding deviation angles δ using the telescope, and plot δ versus i to identify the minimum δ_m at the curve's lowest point; repeat for multiple spectral lines if needed, always reading both verniers and clamping components during observations.[20][19]

