What is the Index of Refraction in a Crystal Sphere Focusing Light?

In summary: The upper left angle is the angle which is formed by drawing a line from the point of incidence to the north pole and the intersection of that line with the radius drawn to the north pole. So sin(angle of incidence)=sin(angle of refraction), and since sin(45)=1, n'=1.414.
  • #1
Aelo
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0

Homework Statement


Consider a special crystal sphere, where light from a distant object is focused by the front surface of the sphere exactly onto the opposite side of the sphere. What is the index of refraction of the sphere? Assume the sphere is in air.


Homework Equations



(n'/l') - (n/l) = (1/R)*(n' - n)
f' = n'/K = n'F

The Attempt at a Solution



I know that n is taken to be 1 since the sphere is in air. Since the object is described to be distant, I'm guessing that perhaps l could be infinity. I've thought about trying to relate different angles to each other or looking at the sag, but it looks like the question is asking for a numerical value, and I don't know how to get there with what was given. Because it's focusing at the side of the sphere, we may be able to relate the radius to the focal point?
 
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  • #2
Since the light is focused on the opposite face you know that the focal length is 2R; you also know that the radius of curvature is R. There is a great deal of symmetry.

You should be able to trace a single ray and then solve for n.
 
  • #3
Since f = -nF, I know that F = -2R. Similarly, f' = n'F. How do I find f'? Or am I over-simplifying it?
 
  • #4
You don't need any of the lens equations; you already know where all of the rays terminate ... because your light is from a "distant source" the incoming rays are parallel, so assume that they illuminate one full hemisphere.

You can imagine the sphere as a globe, with the light illuminating the southern hemisphere - then the longest ray (and the only straight ray) travels from the south pole to the north pole, a distance of 2R, and the angle of incidence with the normal is 0. The rays hitting at the equator (just barely!) are at 90 degrees ... but these may not make the transit ... so pick a latitude close to the south pole (latitude theta-1), determine the angle of incidence all around this latitude circle, and the internal angle required to send each of these rays to the north pole (angle theta-2).

Now apply Snell's law to these two angles ... the geometric conditions will provide enough constraints to determine the index of refraction - and also the greatest circle of latitude which contributes to the light at the north pole!
 
  • #5
Why wouldn't the ray hitting at 90 degrees be usable? If I'm understanding you correctly, what I need to do is consider just the ray hitting at (or around) 90 degrees, find the angle of refraction once that ray has entered into the sphere, and say that n*sin(90 or almost 90) = n'*sin(angle of refraction).
 
  • #6
If the equatorial ray makes it to the north pole then what is the angle of refraction?

Plug these angles into Snell's law and you will have a value for n' of the glass. But sin (90)=1, and n for air is 1, so n' would have to be 1/sin (45)=sqrt (2). So unless n'=1.414 the equatorial ray will not reach the pole. This does seem to match the problem statement.
 
  • #7
I thought this sphere was special in that every ray hitting it was focused to the sphere's opposite side. Wouldn't that mean that the equatorial ray would have to make it?
 
  • #8
Just test another latitude, 45 degrees would work and see if n' is the same.
 
  • #9
What trig relationship should I use to find the value of the refracted ray?
 
  • #10
The incident ray comes in parallel to the polar axis; the angle of incidence is thus the angle between the polar axis and the normal to the surface where the ray strikes ... if it strikes at latitude 45 the angle is 45. If it strikes at latitude 30 it is 60 ... draw a diagram of a circle to test this.

Then connect the ray from the point of incidence to the north pole ... the interior triangle made from the point of incidence and the two poles (draw it!) obeys a simple theorem from plane geometry. This will give the angle of refraction.
 
  • #11
I've had a drawing since the start, I've just been too lazy to post it. :rolleyes:

Here it is:

Scan0008_1.jpg


Knowing only one angle of the three sides, I don't know how to find theta 2. Geometry was never a strength, unfortunately. It's not a right triangle, so I can't say that the sum of the 3 angles is 180.
 
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  • #13
Looking at that and this: http://www.regentsprep.org/Regents/math/geometry/GP15/CircleAngles.htm

Wouldn't that indicate the upper left corner angle is 90 degrees, so that theta 2 = 180 - 90 - 45?
 

Related to What is the Index of Refraction in a Crystal Sphere Focusing Light?

What is the index of refraction?

The index of refraction is a measure of how much a material bends light as it passes through. It is defined as the ratio of the speed of light in a vacuum to the speed of light in the material.

How is the index of refraction measured?

The index of refraction can be measured using a variety of methods, such as the Snell's Law experiment or the critical angle method. These experiments involve measuring the angle of refraction as light passes through the material and using mathematical equations to calculate the index of refraction.

What factors affect the index of refraction?

The index of refraction is affected by the density and composition of the material, as well as the wavelength of light passing through it. It also varies with temperature and pressure.

Why is the index of refraction important?

The index of refraction is important in understanding how light behaves as it passes through different materials. It is also crucial in the design and development of lenses and other optical devices.

How does the index of refraction relate to the speed of light?

The index of refraction is inversely proportional to the speed of light in a material. This means that as the index of refraction increases, the speed of light decreases. This is why light appears to slow down and bend when passing through materials with high indices of refraction, such as water or glass.

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