Calculating Limiting Magnitude for 12-Inch Telescope: Tips and Advice

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In summary, the limiting magnitude of a 16-inch telescope is about 14.8 and a 12-inch telescope is about 14.3. However, the limiting magnitude for digital photography with a CCD camera and 25 images per second can only be determined by comparing images to a star catalogue. There are calculators available to estimate the limiting magnitude, but it also depends on various factors such as telescope type and viewing conditions.
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big man
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I was just wondering if any of you guys knew how to calculate the limiting magnitude of a 12-inch telescope given that you know the limiting magnitude of a 16-inch telescope.

I'm using the same exposure time obviously and I'm using an SBIG ST-4 CCD camera so these factors are constant. I just don't know how to scale it down for a 12-inch and it would be nice to know.

Thanks for any advice
 
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A 16-inch telescope generally has a limiting magnitude of about 14.8, while a 12-inch telescope generally has a limiting magnitude of about 14.3.

- Warren
 
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Thanks, that is useful to know.

I found the limiting magnitude of the 16-inch to be about 12.4 or so from comparing my images to star catalogues and finding the faintest star on the image. But I'm taking about 25 images per second.

So I'm wanting to know how I can find the limiting magnitude of the 12-inch from this.
 
  • #4
big man said:
Thanks, that is useful to know.

I found the limiting magnitude of the 16-inch to be about 12.4 or so from comparing my images to star catalogues and finding the faintest star on the image. But I'm taking about 25 images per second.

So I'm wanting to know how I can find the limiting magnitude of the 12-inch from this.
I don't think you can from just that information. There are several things to consider in telescope resolution (R) and limiting magnitude (M). Usually, most of what is in the "common" definitions for both R and M are referring to visual limits, not photography.

For Visual, the standards are that:
R=(4.56/D), where D is the scope's aperture in inches.
and:
M=10+(5(log(D)*0.4342945))

But, actual visual M depends on seeing conditions, type of telescope, power of eyepiece, angle from zenith, etc., etc. There are calculators for this at:

http://www.go.ednet.ns.ca/~larry/astro/maglimit.html and:
http://www.geocities.com/catskills_astronomy_club/calculator.htm
Which appear to be the same and even try (not accurately) to factor in your age.

The "standard" formulae first shown above show that:
For a 16" scope: M=16.02 and R=0.28 arcseconds.
For a 12" scope: M=15.40 and R=0.38 arcseconds.

But, you're doing digital photography (CCD) with 25 images per second (and stacking??). So, the only way to figure your M limit in the photos is as you do in your post quoted above and compare faintest stars to a catalog. Then jiggle several of the inputs in one of the web calculators to match what your 16" can see as a limit and then just change the aperture only to 12" leaving all the other parameters alone to see what you could expect for the 12" scope in the same conditions.

Of course you could change exposure time and stack fewer or more images or move to a darker sky location and all of that would change. With the CCD and exposure/stacking/location variables, the answers would near infinite.
 
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1. What is the formula for calculating limiting magnitude for a 12-inch telescope?

The formula for calculating limiting magnitude is: m = 2 + 5log(D) + 5log(t) where m is the limiting magnitude, D is the diameter of the telescope in inches, and t is the exposure time in seconds.

2. How does the diameter of a telescope affect the limiting magnitude?

The diameter of a telescope is a key factor in determining the limiting magnitude. A larger telescope diameter allows for more light-gathering power, which increases the overall sensitivity and therefore the limiting magnitude.

3. What is the role of exposure time in calculating limiting magnitude?

Exposure time is also an important factor in calculating limiting magnitude. The longer the exposure time, the more light will be gathered by the telescope, leading to a lower limiting magnitude.

4. Are there other factors besides telescope diameter and exposure time that affect limiting magnitude?

Yes, there are other factors that can affect limiting magnitude, such as atmospheric conditions, light pollution, and the quality of the telescope optics. These factors can impact the overall sensitivity and clarity of the telescope, and therefore affect the calculated limiting magnitude.

5. Can limiting magnitude be used to determine the overall performance of a telescope?

Limiting magnitude is just one measure of a telescope's performance and sensitivity. Other factors such as resolution, contrast, and image quality should also be taken into consideration when evaluating the overall performance of a telescope.

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