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Celestron C11 SCT XLT AVX Optical Tube Assembly

Celestron C11 SCT XLT AVX Optical Tube Assembly

There are other ways to design a catadioptric system at f/10 using the full aperture Schmidt type correcting plate, by generating a different aspheric curve on the secondary. However, for production purposes, the difficulty lies in producing a diffraction limited instrument using a different aspheric curve on the secondary, on a consistent basis. Regardless of theoretical advances that other designs may promise, the key lies in the consistent diffraction limited performance that is actually realised when a catadioptric telescope is factory produced. Celestron’s original tried and tested method has worked and worked very well over the decades, one of the main reasons astronomers continue to trust Celestron's optical designs. Many competing catadioptric telescopes have found it difficult to match the optical consistency of Celestron.

The Celestron Schmidt Cassegrain design is also beneficial for planetary imagers over other catadioptric designs such as the Maksutov Cassegrain (both the standard Gregory type and the separate secondary configuration), due to the cooling times of the thick meniscus lens on Maksutovs. Maksutovs often show correction errors for long periods of time whilst cooling. On the larger instruments (greater than about 180mm) this can be quite protracted. The problem is often due to the differential cooling periods of both the primary mirror and the meniscus. For planetary imagers, this can sometimes mean an unproductive night waiting for spherical aberration to reach a minimum. The Celestron Schmidt Cassegrains cool at a much faster rate, which means a much longer period of observation with the telescope at optimum correction.

Celestron’s Schmidt Cassegrains offer the amateur astronomer or the optical enthusiast the complete “owning a telescope” experience. The apertures range from five inches to fourteen inches and focal lengths between 1250mm and 4000mm. They are the scope of choice for planetary imagers, and deep-sky imagers because of the range of image scales. They represent the ideal observing instrument with medium to large apertures, medium to longer focal lengths for the comfortable use of higher magnifications, a large diffraction limited field free of aberrations, and rear eyepiece positioning for relaxed long periods of observing. The closed tube design keeps the important optical surfaces clean and prevents image-destroying tube currents seen in some Newtonians. The primary mirror focusing system permits close focusing with minimum spherical aberration, whilst enabling the observer to vary image scale, and all of this potential and performance in a closed compact easy to handle optical tube assembly.

11" Schmidt-Cassegrain Optical Tube Assembly
Aluminum Optical Tube
Celestron's premium StarBright XLT coatings
2800mm focal length (f/10)
40mm eyepiece included (70x)
Visual back allows for use with 1.25" accessories
9x50 finderscope to help accurately find objects
Star diagonal provides more comfortable viewing position when observing objects that are high in the sky
Includes dovetail rail compatible AVX / Synta saddles

OPTICAL DESIGN: Schmidt-Cassegrain
APERTURE: 279.4 mm
EYEPIECE 1: 40 mm
OPTICAL TUBE WEIGHT: 27.5 lb (12.47 kg)

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Celestron C11 SCT XLT AVX Optical Tube Assembly

MPN: 91067XLT

Price: 2,054.00

Celestron's C11 is an extremely popular larger Schmidt Cassegrain that is both a large aperture telescope, and yet easily manageable by one person, hence portable. The same Starbright XLT coated optics as all other SCTs in Celestron's range means very bright, contrasty and well resolved DSOs, as well as planetary colour contrast that is immediately obvious. The natural progression for a C8 owner, at the eyepiece the C11 demonstrates a very worthwhile upgrade, with more resolved detail, higher contrast on extended nebulous objects, and galaxies show structure more easily. A superb optical tube for those wanting true laege aperture performance.

There has been much said and written regarding the optics in the SCT. Essentially, the combination of a spherical primary, an aspherized secondary and a Schmidt plate (a thin glass plate, plano (flat) on one side, and with the Schmidt curves on the other), creates a wavefront that is free from Lower Order Spherical aberration (LSA), free from Higher Order Spherical aberration (HSA or zones), a diffraction limited field free of coma and astigmatism, and the field free of Chromatic aberration (CA).

The design has much greater freedom from off-axis coma than the equivalent focal ratio Dall-Kirkham

Much greater freedom from off-axis coma than the focal ratios usually found in Newtonians

Does not suffer from the tube currents common in open tube Cassegrain focus designs, such as the Dall-Kirkham, the Klevsov, the sub-aperture meniscus Maksutov and the standard Cassegrain, nor does it require regular cleaning of the primary optics because the closed tube keeps dust and debris out

It has a smaller secondary than the photographic Ritchey-Chrétien

It has none of the chromatic aberration associated with achromatic refractors.

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