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There are many options to consider when choosing a CCD camera, but usually there are a couple majors factors which can make the decision easier. Admittedly cost is one of the most important factors, but there can be a variety of cameras available within your price range. Matching a CCD camera to a particular telescope can be a factor as well. The following section gives you some ideas how to select the right camera for you. If you have any questions concerning the choice of an appropriate CCD camera, please feel free to contact us.

Types of CCD Cameras

Just as there are various types of telescopes, there are also many different types of CCD cameras. The basic difference between models is the CCD sensor itself, just like the mirror or lens is the basic difference between telescope models. And like telescopes, there are other features available which may make a certain camera more desirable.

CCD Sensor Size

A bigger CCD sensor will, all other things being equal, image a bigger part of the sky. However, all things are not necessarily equal, and a short focal length telescope with a smaller CCD may have a wider field of view than a long-focal-length scope with a larger CCD. Depending on what you want to image, a small-format CCD may suffice, but it is usually desirable to have as large a CCD sensor as possible. Back to the telescope analogy, figure that everyone wants a bigger telescope, just like everyone wants a bigger CCD, but the real limitations are budget and practicality.

The image above shows common CCD sesnors to scale. The actual sizes are about half what they appear on screen. The table below lists specifications for the sensors above.

Sensor Number of Pixels Pixel Size Width x Height Example Camera Models
KAF-16803 16 million 9 microns 36.8 x 36.8 mm Apogee U16M, SBIG STX-16803
KAI-11000 11 million 9 microns 36 x 24.7 mm SBIG STL-11000
APS-C Format 6-18 million 4.3-7.8 microns 23.4 x 15.6 mm Canon EOS 7D, Starlight Xpress M26C
KAF-8300 8.3 million 5.4 microns 18 x 13.5 mm Atik 383, SBIG ST-8300, Starlight Xpress H18
KAI-4000 4 million 7.4 microns 15 x 15 mm Atik 4000, SBIG ST-4000
ICX694 6 million 4.54 microns 12.5 x 10 mm Starlight Xpress H694
KAI-2000 2 million 7.4 microns 11.8 x 8.9 mm SBIG ST-2000
ICX674 2.8 million 4.54 microns 8.8 x 6.6 mm Atik 428EX, Starlight Xpress H674
KAF-0400 400,000 9 microns 6.9 x 4.6 mm SBIG ST-7, SBIG ST-402

The size of the CCD chip is one of the most important factors in imaging. The size of the chip largely determines the field of view, and thus which objects you can take pictures of. Different telescopes can change the field of view as well, but since most people own just one telescope, choosing a CCD with a sufficient field for that telescope is a good idea.

CCD Pixel Size

Here's a touchy subject. One school of thought is that there is an ideal match between CCD pixel size and telescope focal length. If your goal is the highest resolution images possible, especially for scientific applications, then this idea is valid. However, if pretty pictures are your goal, then the second school of thought is probably more appropriate: pixel size doesn't matter.

On a given telescope, smaller pixels give higher resolution. Larger pixels tend to be more sensitive. There is always a trade-off. Figure the number of pixels, and the size of the chip itself, are more important than pixel size for most purposes.

Select a CCD camera and telescope from the menus below. The pixel resolution and field of view will be displayed below. You may also change the binning to see the effect this has on pixel resolution.
CCD Camera
  or Enter User Defined Focal Length (mm)
Pixel Binning

Pixel Size:

Field of View



Above: Standard CCD theory holds that a resolution of about 1-2 arcseconds/pixel is ideal. Above is an image taken with a resolution of 3.7 arcseconds/pixel. Pixel size is really no big deal for most imaging.

Number of Pixels

Again, more is better...usually. The only potential drawback to a greater number of pixels is a slower download time from the camera and longer processing times while manipulating the image later. Most CCD cameras now have high-speed USB 2.0 connections, and computers are always getting faster, so these disadvantages are becoming less and less important. The advantages to more pixels include larger images on a computer monitor, the ability to make larger prints, and the images tend to be more aesthetically pleasing, even when reduced significantly to be viewed on the web.

One-Shot Color vs. Tri-Color Imaging

A major advance in CCD technology in recent years has been the advent of one-shot color cameras. Many CCD chips are inherently black and white. These CCDs require colored filters (red, green, and blue), and a minimum of 3 exposures (one through each color filter) to capture a color image. Many new CCDs incorporate one-shot color chips. These chips divide the chip into separate red, green, and blue sensitive pixels. There is no need for individual color filters, so a single exposure can capture a color image. While these chips are sometimes less sensitive than their non-color counterparts, they require only a single exposure instead of three, so the total exposure times tend to be similar or even less. Also, newer one-shot color cameras tend to be much more sensitive than their predecessors.

Black and white CCDs tend to have more versatility than one-shot color cameras. They are better suited to narrowband imaging and scientific applications such as asteroid searches or photometric studies. However, for taking pretty pictures, one-shot color cameras work very well and offer a very easy learning curve for beginners.

The Reality of the Situation

In an ideal world, every CCD imager would have the biggest, most sensitive CCD camera available; just like every amateur astronomer would have the biggest telescope! But like telescopes, price is always a factor, and almost any quality CCD camera will work fine with any capable telescope. Technique is a big part of it, and great images have been taken with small telescopes and relatively inexpensive CCD cameras from suburban backyards, many of which are even better than some images taken with high-end, sophisticated telescopes, monster CCDs, and permanent observatories at dark sites.

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