Quick check on telescope optics calculations please

In summary, we calculated the magnification, light gathering power, and angular field of a Cassegrain telescope with a 500mm diameter, 5000mm focal length, and 80mm central obstruction. We also calculated the angular and linear resolution for 550 nm light, with the correct conversion to linear resolution being 0.133 μm or 133 nm.
  • #1
skydivephil
474
9

Homework Statement


A Cassegrain telescope has a 500mm diameter , a focal length of 5000mm and a central obstruction of 80mm diameter.
Calculate:
1) the magnification with a 25mm eye piece
2) the light gathering power compared to aye of 5mm in diameter
3) the angular field in the sky if the apparent angular field is 50 degrees
4) the angular and linear resolution for 550 nm light in arc seconds and micro metersMost of this is easy but i just wanted to check I have to the conversion from angular resolution to linear resolution correct.

The Attempt at a Solution


1) mag= focal length scope/ eye piece length = 5000/25= 200
2) light gathering = (apeture of scope/apeture of eye)^2 =(500/5)^2 = 10,000
we have to subtract the central obstruction which is
(80/5)^2 = 256
so the answer is 10,000- 256 = 9744
3) angular field = apparent field /mag = 50/200 = .25
4) theta = 2.5 * 10^5 * lambda/diameter
= 2.5.10^5 * 550*10^-9*500810^-3
=2.5*10^5*1.1*10^-6
= 2.75 seconds of arc
To convert this into linear resolution in micro meters
apeture in um /206265
=500*10^3/206265 = 2.42
hence 2.42*2.75 = 6.66 um.
 
Last edited:
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  • #2


Your calculations for parts 1-3 appear to be correct. However, for part 4, the conversion from angular resolution to linear resolution is not quite accurate. The formula for angular resolution is θ = λ/d, where λ is the wavelength of light and d is the diameter of the telescope's aperture. To convert this into linear resolution, you need to multiply by a factor of 206265 (the number of arcseconds in a radian) and then divide by the focal length of the telescope. So the correct calculation would be:

θ = λ/d = 550*10^-9/500*10^-3 = 1.1*10^-6
Linear resolution = θ * 206265 / focal length = 1.1*10^-6 * 206265 / 500 = 0.453 μm

Alternatively, you could also use the formula for linear resolution, which is d = 1.22 * λ/f, where f is the focal length of the telescope. Plugging in the values, we get:

Linear resolution = 1.22 * 550*10^-9 / 5000*10^-3 = 0.133 μm

Both methods should give you the same result. So the final answer for part 4 would be:

Angular resolution = 2.75 seconds of arc
Linear resolution = 0.133 μm or 133 nm
 

1. What are the essential components of a telescope?

The essential components of a telescope are the objective lens or mirror, the eyepiece, and a mount or tripod.

2. How do I calculate the magnification of a telescope?

To calculate the magnification of a telescope, divide the focal length of the objective by the focal length of the eyepiece. For example, if the focal length of the objective is 1000mm and the focal length of the eyepiece is 20mm, the magnification would be 50x (1000/20 = 50).

3. What is the difference between refracting and reflecting telescopes?

A refracting telescope uses lenses to bend and focus light, while a reflecting telescope uses mirrors. Reflecting telescopes tend to be more compact and have a wider field of view, while refracting telescopes can produce sharper images.

4. How does the aperture affect a telescope's performance?

The aperture, or the diameter of the objective lens or mirror, affects a telescope's performance by determining its light-gathering ability. A larger aperture allows for more light to enter the telescope, resulting in brighter and clearer images.

5. What is chromatic aberration and how does it impact a telescope's optics?

Chromatic aberration is the distortion of colors in an image due to the different wavelengths of light being refracted at slightly different angles. This can impact a telescope's optics by causing color fringing and reducing image clarity. This can be minimized through the use of special lens coatings or by using a larger aperture.

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