"The Most Fabulously Useful Formula In Astronomy"

By Tom Lougheed

Well, at least it is of some use when dealing with telescopes. :-)

1. Eye Relief And Eyepiece Aperture

 

 

 

2. Apparent and True Field of View

    This commonly used formula is only approximate.

   Is more exact

 

3. Apparent field of view, field stop, and eyepiece focal length.

 

This only works for "normal" eyepieces, like Kellners, Plossls, and Panoptics. It does not work for eyepieces that have a built-in Barlow, like Vixen Lanthinum, Nagler, and Meade Ultrawide.

Note that "s" is what one measures using the star drift test. So it is not possible by that test alone to measure both the eyepiece focal length and the apparent field of view: either you need another thest (like the size of a focused image of the sun, made using only the eyepiece) or you must assume the manufacturer's value of alpha or "l" is correct (it never is exact).

 

4. Maximum true field of view in a focusing tube.

This only gives the upper limit on the true field of view -- what you would get from longest focal length/widest field eyepiece usable in that scope. Usually the eyepiece will impose the limit on the field of view. This also does not consider whether vignetting from baffles or from a secondary mirror will prevent the full field of view from being completely illuminated.

The picture is for a refractor, but the formula also works for Netonians and Catadioptrics.

 

5. Maximum field of view with a dew shield or telescope tube.

This formula is only approximate for catadioptrics, where the corrector lens spreads out the light path. It's exact for Newtonians and Refractors.

Note: Formulas 2, 4, and 5 give three different answers for the (maximum) true field of view. What you get is the smallest number -- usually from the eyepiece, hence formula 2.

Notice that this is the same formula as 3 -- the telescope's pupil is the objective diameter, and its outermost aperture is like the eyepiece eye-lens diameter.

ASCC Lectures