A 279 mm f/10 aplanatic Schmidt-Cassegrain with a flat, corrected field — 2 800 mm of focal length aimed squarely at small galaxies, planetary nebulae and high-resolution planetary work.
Short verdict
A superb long-focal-length instrument that will expose every weakness in your mount, your seeing and your guiding before it shows you what it can do.
Sold as an optical tube only. No mount, tripod or head is included. For imaging in particular, the mount is usually the larger part of the total cost.
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Best for
Small-galaxy and planetary-nebula imaging from a permanent or semi-permanent setup
High-resolution planetary imaging
Experienced observers who want maximum resolution in a transportable tube
Not ideal for
Wide-field nebula imaging, even with the reducer
A first imaging telescope
Anyone whose mount is rated below about 20 kg
Purpose scores
The same four purposes are scored for every telescope on this site, using the same weights. A telescope that is excellent for one is often poor for another — that is the point.
Scores are relative to every telescope on this site, not absolute quality marks. A 6.5 for galaxy imaging and a 6.5 for visual observing do not mean the same thing. How scoring works.
Optical design
The EdgeHD adds a field-flattening lens group inside the baffle tube of an otherwise conventional
Schmidt-Cassegrain. The result is an aplanatic system: coma-free and, crucially for imaging, flat
across a 42 mm image circle. A standard SCT of the same aperture produces visibly elongated stars
in the corners of an APS-C frame; this does not.
Celestron also added mirror locks and tube vents. The locks stop the primary shifting when you
change orientation — the single most irritating property of a moving-mirror focus system for
imagers — and the vents shorten what would otherwise be a very long cooldown for a 279 mm mirror.
Visual observing
Very good, and rarely the reason anyone buys one. 279 mm shows globular clusters resolved across
the core, structure in bright galaxies, and planetary detail limited by the atmosphere rather than
the optics. The field is narrow, as it must be at 2 800 mm, and the practical obstacle is that you
need a substantial mount before you can look through it at all.
Nebula imaging
Not the tool. At 2 800 mm, or 1 960 mm with the reducer, only the smallest planetary nebulae fit
the frame, and f/10 or f/7 is slow for extended nebulosity. A small refractor will produce a better
nebula image in a tenth of the time.
Galaxy imaging
This is the EdgeHD’s purpose. 2 800 mm gives roughly 0.28 arcseconds per pixel with a 3.76 µm
sensor — over-sampled for typical seeing, well matched on the best nights, and the flat field means
the whole frame is usable rather than just the centre.
Be honest about the demands. Guiding must hold well under an arcsecond RMS, the mount must be rated
far above the tube’s 12.7 kg, and flexure anywhere in the train shows immediately. Most owners run
the 0.7× reducer at 1 960 mm and f/7, which is more forgiving and still delivers real image scale.
Planetary imaging
Excellent. 279 mm resolves to about 0.42 arcseconds, and the native 2 800 mm needs only modest
amplification for a well-sampled planetary capture. On nights when seeing allows the full aperture
to be used, this is among the best planetary instruments available in a transportable form.
Portability, setup, collimation and thermals
12.7 kg of tube, 610 mm long and 310 mm across, on a mount that will itself weigh 20 to 30 kg. This
is a set-up-and-leave instrument for most owners. Collimation is a secondary-screw adjustment done
occasionally. Even with the vents, allow a good hour of cooling before high-resolution work, and
fit a dew shield — a 279 mm corrector plate is a large surface to lose to dew.
Full specifications
Optics
Optics specifications for Celestron EdgeHD 11 (OTA)
Aperture
279.4 mm (11")
Focal length
2800 mm (110.2")
Focal ratio
f/10
Optical design
Aplanatic Schmidt-Cassegrain with integral field flattener
Type
Schmidt-Cassegrain
Glass / mirror
Schmidt corrector with StarBright XLT coatings; field-flattening lens group in the baffle tube
Central obstruction
32%
Resolving power
0.42"Calculated from aperture (Dawes limit), not a manufacturer figure.
Limiting magnitude
≈ 14.2Estimated from aperture under dark skies. Real skies are usually worse.
Imaging compatibility
Imaging compatibility specifications for Celestron EdgeHD 11 (OTA)
Corrected image circle
42 mm
Backfocus
146 mm
Field correction built in
Yes
Usable visually
Yes
APS-C sensors
Supported
Full-frame sensors
Not fully covered
Reducer
Available (×0.7)
Corrector required
No
Autoguiding
Recommended
Mount and tracking
Mount and tracking specifications for Celestron EdgeHD 11 (OTA)
Mount included
No — optical tube only
Tracking
Depends on your mount
GoTo
Depends on your mount
Mounting interface
Losmandy-style dovetail
Size and weight
Size and weight specifications for Celestron EdgeHD 11 (OTA)
OTA weight
12.7 kg (28 lb)
Tube length
610 mm (24")
Tube diameter
310 mm
Longest transport dimension
700 mm (27.6")
Product
Product specifications for Celestron EdgeHD 11 (OTA)
Brand
Celestron
Model
EdgeHD 11 Schmidt-Cassegrain
Status
Current
Price band
FlagshipWe publish bands, not prices. Check the retailer for the current price.
Skill level
advanced
Editorial notes
Backfocus for the EdgeHD series is specified from the rear cell and differs between native and reduced configurations. Confirm the figure for your exact accessory stack before ordering adapters.
Strengths and limitations
Strengths
+Genuinely flat, corrected field across an APS-C sensor — an ordinary SCT needs a corrector to approach this and still does not match it.
+279 mm of aperture resolving to about 0.42 arcseconds, which is beyond what most nights of seeing will let you use.
+Mirror locks and vented tube address the two classic SCT complaints: focus shift and slow cooldown.
Limitations
−2 800 mm is unforgiving. Guiding errors, seeing and flexure all show up at roughly 0.28 arcseconds per pixel.
−12.7 kg of tube demands a mount that costs more than the telescope does.
−The 146 mm backfocus requirement is a strict constraint that dictates your whole imaging train.
Accessories
In the box
Losmandy-style dovetail bar
Mirror-locking rear cell
Required, sold separately
A heavy equatorial mount — realistically rated at 20 kg or more for imaging
An off-axis guider or guide scope
A camera and the correct 146 mm backfocus spacing
Worth adding
0.7× reducer for a faster, wider configuration
Dew shield and heater
Cooling fan accessory
We list an accessory as included only when the product record says so explicitly. If a mount, eyepiece, camera, flattener, reducer, corrector, guider or adapter is not listed above, assume it is not in the box.
Ideal targets
Small and medium galaxies
Planetary nebulae
Globular clusters
Jupiter, Saturn and Mars at high resolution
Alternatives to consider
Rowe-Ackermann Schmidt AstrographCamera onlyOTA only