Optics: radius of a central disk of light

In summary, to compute the radius of the central disk of light forming the image of a star on the focal plane of a telescope objective, the equation \theta_{min\frac{1}{2}} = \frac{1.22*\lambda}{D} can be used, where \lambda is the mean wavelength of the light and D is the diameter of the objective. Make sure to use consistent units, such as converting the focal length from meters to centimeters, to get an accurate result.
  • #1
vorcil
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Homework Statement



A telescope objective is 12cm in diameter and has a focal length of 150cm.

Light of mean wavelength 550nm from a distant star enters the scope as a nearly collimated beam.

compute the radius of the central disk of light forming the image of the star on the focal plane of the lens

Homework Equations



[tex] \theta_{min\frac{1}{2}} = \frac{1.22*\lambda}{D} [/tex]

Radius of disk =[tex] L * \theta_{min\frac{1}{2}} [/tex]

The Attempt at a Solution



after showing the proof for those equations all I did was solve for the radius of the disk by plugging in the numbers,

[tex] \frac{1.22 * (550*(10^{-9}))}{\frac{12}{100}m}*\frac{150}{100}m [/tex]

putting into a calculator I got 8.3875*10^-6, approximately 8.39*10^-6

however the answers show 8.39*10^-4,

what am I missing?
 
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  • #2


It seems like you may have missed a conversion from meters to centimeters in your calculation. The diameter of the telescope objective is given in centimeters, so you should convert the focal length from meters to centimeters before plugging it into the equation. This would give a value of 1.5 cm instead of 150 cm. Plugging that into the equation, you should get a radius of 8.39*10^-4 cm, which matches the given answer.
 

Related to Optics: radius of a central disk of light

1. What is the radius of a central disk of light?

The radius of a central disk of light, also known as the Airy disk, refers to the size of the central bright spot that is created when a beam of light is focused through a circular aperture. The radius is determined by the wavelength of light and the size of the aperture.

2. How is the radius of a central disk of light measured?

The radius of a central disk of light is typically measured by using a specialized instrument called a diffraction-limited detector, which is able to accurately detect and measure the size of the Airy disk. This measurement can also be calculated mathematically using the diameter of the aperture and the wavelength of light.

3. What factors affect the radius of a central disk of light?

The radius of a central disk of light is primarily affected by the wavelength of light and the size of the aperture. Other factors that can also affect the radius include the shape and quality of the aperture, and any imperfections or aberrations in the optical system.

4. Why is the radius of a central disk of light important in optics?

The radius of a central disk of light is important because it determines the resolution and sharpness of an optical system. A smaller radius means a smaller and more focused central spot, which allows for better clarity and detail in imaging and microscopy applications.

5. Is the radius of a central disk of light the same for all wavelengths of light?

No, the radius of a central disk of light varies depending on the wavelength of light. This is because different wavelengths of light diffract differently through an aperture, resulting in different sized Airy disks. This is known as chromatic aberration and can be corrected for in optical systems through the use of specialized lenses and coatings.

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