Observatory Series
A complete observatory-class telescope system that combines massive 40" aperture with integrated Smart Finder observing assistance. Featuring plate-solving Smart Finder technology, 27-point flotation mirror cell, and observatory-grade all-metal construction. Built for serious observatory programs, advanced observing, and large-aperture imaging workflows.
Real-time sky guidance helps plan efficient observing sessions.
f/3.3: $69,000 USD
Ready to commission your observatory?
50% deposit required ($34,500 USD)
Consult with an Observatory SpecialistAt 40 inches of aperture with a fast f/3.3 optical system, the UL40SO delivers extreme light-gathering power in a practical observatory installation. This is not just about seeing more. It makes professional observatory-class apertures achievable for educational institutions, research programs, and serious amateurs who previously had to settle for far less. The UL40SO is built for permanent and semi-permanent observatories, with portable deployment possible when needed. It is well suited for research and education programs, public outreach, advanced visual observing, large-aperture EAA, and astrophotography.
Aperture
1016mm (40")
Focal Ratio
f/3.3
Resolution
0.11 arcsec
Light Gathering
21,000x
System Weight
~365 kg
Purpose-built for permanent and semi-permanent observatory installations, with portable deployment possible when needed.
Ideal for educational institutions and research programs seeking uncompromised aperture with intelligent pointing and observing assistance for students and researchers.
Smart Finder "Star Show" programs and intelligent routing support public outreach events, reducing setup time and maximizing observing time.
With 21,000x the light-gathering power of the human eye, the UL40SO supports advanced visual observing, large-aperture EAA, and astrophotography.
The integrated SkyHub Pro Smart Finder adds intelligent pointing and observing assistance to the UL40SO. Featuring a dedicated high-speed imaging module, the Smart Finder enables one-button automated alignment with integrated plate solving, reducing the need for manual star centering.
Dynamically generated "Star Shows" create observing sessions based on your location, date, and current sky conditions. Examples include Messier Marathon, Galaxy Evolution, and Tonight's Best. Each session is intelligently optimized to maximize observing time and minimize unnecessary slewing. Every observing session is uniquely generated, so no two nights are ever the same.
Advanced real-time image processing with sigma-clipping, HDR stretching, and progressive stacking reveals faint deep-sky objects within seconds. Planetary imaging includes multi-layer wavelet sharpening for high-resolution detail extraction.
The system supports dual-camera operation, FITS export, a 10,000+ object database, and real-time visibility calculations. The Smart Finder system helps coordinate the observing workflow and handles technical complexity so you can focus on exploring the universe.
The lightweight sandwich mirror design reaches thermal equilibrium dramatically faster than a solid mirror of the same aperture, minimizing the thermal gradients that cause image distortion. The structure itself is passive, so it never introduces vibration into the optical path.
One of the primary limitations in large-aperture telescopes is "mirror seeing," the turbulence caused by temperature differences between the mirror and the surrounding air. A thick solid mirror may never fully reach equilibrium in changing conditions, preventing it from achieving its full optical performance. For smaller apertures, the sandwich design typically requires no active cooling. At 40 inches, the scale of the system makes ambient shifts more significant, particularly where temperatures change rapidly between day and night. Active pre-conditioning brings the mirror close to ambient before observation, and the lightweight structure then maintains stable performance passively during the session. In practice, diffraction patterns stabilize within tens of minutes rather than requiring hours of cooling.
Fully engineered flotation mirror cell with sling lateral support and 90-degree pivoting edge supports. Ensures uniform mirror support, eliminates stress-induced deformation, and prevents "potato chip" astigmatism. The mirror cell is completely independent from the collimation system.
96% enhanced reflective coatings on both primary and secondary mirrors with precision dielectric overcoats. Maximum light throughput, improved contrast and brightness, with excellent durability and environmental protection.
CNC-machined components with FEA-optimized structural design. 6063-T6 aluminum truss system, steel mirror cell, aluminum alloy OTA and mount, and stainless steel rocker. Extremely rigid, mechanically stable, and built for long-term observatory use.
State-of-the-art OnStep or SiTech controller with WiFi, Bluetooth, INDI/ASCOM support. Compatible with SkySafari, Stellarium, and more. Includes dedicated smart hand controller with ~30,000 objects, sidereal/lunar/solar tracking, and park/unpark functions.
| Optical Design | Newtonian Reflector |
| Optical Diameter | 1016mm (40") |
| Focal Length | ~3352mm |
| Focal Ratio | f/3.3 |
| Eyepiece Height at Zenith | ~2570mm (~101") |
| Optical Quality | Diffraction Limited (Strehl ≥ 0.95 typical, 1/10 lambda PV secondary) |
| GoTo Controller | OnStep / SiTech with WiFi & Bluetooth |
| Focuser | 2" dual-speed linear bearing Crayford |
| Secondary Obstruction | 310mm / 30% by diameter / 9% by area |
| Mirror Coatings | 96% Enhanced on both primary and secondary |
| Tube Material | 6063-T6 Aluminum Alloy truss, aluminum alloy OTA/mount, structural steel mirror cell, stainless steel rocker |
| Tube Length | ~3000mm |
| Weight (OTA) | ~275 kg |
| Weight (Mount & Rocker) | ~90 kg |
| Weight (Assembled) | ~365 kg |
| Power Supply | Control: 12 VDC 2A, 5.5-2.1/2.5mm; Motor: 24 VDC 5A, 5.5-2.5mm |
| Rayleigh Limit | 0.11 arcsec |
| Dawes Limit | 0.114 arcsec |
| Limiting Magnitude | 16.8 |
| Max Magnification | 2000x |
| Light Gathering Power | ~21,000× (compared to the human eye) |
| Accessories | 9x50 Finder, Shroud (optional) |
| Other Features | 8-point whiffletree lateral support, push-pull brass knob collimation |
Add these when ordering, or contact us at info@hubble-optics.com
We provide white-glove shipping service globally. Contact our observatory specialists for a custom shipping quote based on your location and installation requirements.