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

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SUMMARY

The limiting magnitude for a 12-inch telescope is approximately 14.3, while a 16-inch telescope has a limiting magnitude of about 14.8. To calculate the limiting magnitude for the 12-inch telescope based on the performance of a 16-inch telescope, one must consider factors such as telescope resolution (R) and limiting magnitude (M), which are influenced by aperture size, seeing conditions, and photographic techniques. The standard formulas for calculating these values are R=(4.56/D) and M=10+(5(log(D)*0.4342945)). For precise measurements, comparing images to star catalogs is essential, especially when using a CCD camera like the SBIG ST-4.

PREREQUISITES
  • Understanding of telescope aperture and its impact on limiting magnitude
  • Familiarity with CCD imaging techniques and exposure settings
  • Knowledge of astronomical star catalogs for comparison
  • Basic grasp of mathematical formulas for calculating telescope resolution and limiting magnitude
NEXT STEPS
  • Research the use of CCD cameras in astrophotography, focusing on the SBIG ST-4 model
  • Learn how to use online calculators for determining limiting magnitude based on telescope specifications
  • Explore techniques for stacking images to enhance faint star visibility
  • Investigate the effects of different sky conditions on telescope performance and limiting magnitude
USEFUL FOR

Astronomy enthusiasts, astrophotographers, and anyone interested in optimizing telescope performance and understanding limiting magnitude calculations.

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
 
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.
 
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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