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IMPORTANT: Our store is located in Canada. All orders that include products manufactured outside of Canada or USA will be subject to tariffs and duties, regardless of the order value. US customers are responsible for all applicable duties and tariffs, and those will be billed by the carrier, except for the Lacerta upgrade kit, for which we collect them at checkout.

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Celestron 36 cm RASA OTA - CGE Dovetail

SKU CEL-91078
Original price $14,999.00 - Original price $14,999.00
Original price
$14,999.00
$14,999.00 - $14,999.00
Current price $14,999.00
Price Match Policy!
  • 355.6mm (14") Rowe-Ackermann Schmidt Astrograph
  • Ultra-fast f/2.2 focal ratio with 790mm focal length
  • Covers a 60.1mm image circle, with a usable field up to 70mm
  • New Ultra-Stable Focus System (USFS) eliminates image shift
  • Extended wavelength range from 400 nm to 900 nm
  • Weighs 75 lbs (34.02 kg)
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • Celestron 36 cm Rowe-Ackermann Schmidt Astrograph (RASA 36) V2

    The Celestron RASA 36 V2 combines a massive 355.6mm (14") aperture with an incredibly fast f/2.2 optical system, delivering an unmatched combination of light-gathering power, speed, and field of view for professional and scientific applications. Its 790mm focal length produces a huge 60.1mm image circle, delivering spot sizes smaller than 6.3 μm RMS across the entire field of view. The optical design is optimized for an extended spectral range of 400-900 nm, capturing more signal than typical visual systems and boosting the light-gathering power, which already stands at 2581 times that of the human eye.

    An f/2.2 System with a 70mm Usable Field

    The RASA design is engineered for one purpose: wide-field imaging at unprecedented speed. At f/2.2, you can achieve exposure times that are fractions of what's required on slower systems, enabling the capture of faint details in nebulae and galaxies or tracking fast-moving satellites. The Rowe-Ackermann Schmidt optical layout produces a completely flat focal plane, free from coma, astigmatism, and field curvature, eliminating the need for additional correctors.

    With an optimized image circle of 60.1mm and a usable field of 70mm, the RASA 36 fully illuminates the largest professional CMOS and CCD sensors available. This vast, corrected field allows you to capture enormous targets like the entire Veil Nebula complex or the Andromeda Galaxy (M31) in a single frame with stunning resolution from edge to edge.

    The Ultra-Stable Focus System (USFS) for Zero Image Shift

    A key upgrade in the V2 is the Ultra-Stable Focus System (USFS). This system uses a precision linear ball bearing to support and guide the primary mirror during focusing. This robust design virtually eliminates focus shift and mirror flop—unwanted lateral movement of the mirror that can ruin an exposure, especially during automated focusing routines or when slewing across the sky.

    The result is a rock-solid focusing mechanism that holds collimation and maintains a perfectly centered image, which is critical for scientific photometry, astrometry, and deep-sky imaging. The USFS is also compatible with the optional Celestron Focus Motor for complete remote operation.

    A 75 lb OTA with Integrated Cooling and Support

    The RASA 36 is a professional instrument, and its mechanical systems are built to match. The 75 lb aluminum optical tube is supported by dual CGE/Losmandy-style dovetail bars, providing secure mounting and ample surface area for attaching guide scopes and other accessories. Integrated carrying handles make transport and mounting more manageable.

    To ensure peak optical performance, an integrated 12V DC MagLev fan accelerates cooldown to ambient temperature, minimizing tube currents that can degrade image sharpness. The fan pulls air through micromesh-filtered vents, preventing dust from settling on the primary mirror and corrector plate.

    Imaging with 77.5mm of Back Focus for Large Format Sensors

    The RASA 36 is designed for seamless integration with modern imaging systems. It provides a generous 77.5mm of back focus from the top of the threaded collar, accommodating a wide range of large-format cameras, filter wheels, and other accessories. With the included M48 camera adapter, the back focus is set to a standard 55mm, making it easy to connect many popular cameras out of the box. This flexibility ensures you can achieve the correct spacing for optimal performance across the entire 70mm usable field.

    RASA 36 vs. Smaller Models: The 355.6mm Aperture Advantage

    As the largest RASA Celestron manufactures, the RASA 36 offers a significant step up in capability. Its 355.6mm aperture provides a major boost in both light-gathering power and resolution compared to smaller models like the RASA 11. This increase in aperture allows you to resolve finer details, with a Dawes' limit of just 0.36 arc seconds, and capture fainter objects in the same amount of time.

    This power comes with the trade-off of size and weight; at 75 lbs, the RASA 36 requires a high-capacity, observatory-class mount. For space surveillance, scientific research, or advanced imagers who need the ultimate in speed and resolution, the RASA 36 is in a class of its own.

  • What kind of mount is required for the RASA 36 V2?

    The RASA 36 V2 optical tube weighs 75 lbs (34.02 kg). You will need a robust, observatory-class equatorial mount with a payload capacity of at least 100 lbs to handle the OTA and a full imaging train. Precise tracking and guiding are essential to take advantage of the instrument's high resolution.

    What is the Ultra-Stable Focus System (USFS) on the RASA 36?

    The USFS is a mechanical upgrade that supports the primary mirror on a precision linear ball bearing. This system prevents the mirror from tilting or shifting during focusing (focus shift) or when the telescope points to different parts of the sky (mirror flop). It ensures your target stays perfectly centered and in focus, which is critical for automated imaging.

    Can I use my DSLR or mirrorless camera with the RASA 36 V2?

    While physically possible with the correct adapters, DSLR and mirrorless camera bodies are often too large and will obstruct a significant portion of the telescope's 355.6mm aperture. The RASA 36 is designed for use with cylindrical, low-profile dedicated astronomy cameras to minimize this central obstruction, which is already 158mm wide.

    How does the RASA 36's f/2.2 speed affect imaging the Andromeda Galaxy (M31)?

    The RASA 36's f/2.2 speed and 790mm focal length allow you to capture the entire Andromeda Galaxy (M31) in a single frame with a large sensor. You can acquire deep, high-signal data in a fraction of the time needed for a typical f/7 or f/10 system. A single 5-minute exposure on the RASA 36 can reveal details that might take over 30 minutes to capture on a slower telescope.

    What is the benefit of the extended 400-900 nm wavelength range for the RASA 36?

    Most telescopes are corrected for visible light (400-700 nm). The RASA 36's optics are designed to focus light well into the near-infrared (up to 900 nm). Modern CMOS and CCD sensors are sensitive to this light, so the extended range allows the telescope to gather a brighter signal, effectively increasing its sensitivity and further reducing exposure times.

    I have a large format camera. How do I attach it to the RASA 36 V2 to use the full 70mm field?

    To utilize the full 70mm usable field, you will likely need a custom camera adapter. The RASA 36 has a native back focus of 77.5mm from the threaded collar. You'll need to calculate the distance required by your specific camera, filter wheel, and any other accessories to have an adapter machined that places your sensor at this focal plane.

  • Optical Tube Info
    Optical Design Rowe-Ackermann Schmidt Astrograph
    Aperture 355.6mm (14")
    Focal Length 790mm (31.1")
    Focal Ratio f/2.2
    Image Circle 60.1mm (2.36") Ø, 4.4°
    Useable Field 70mm (2.75") Ø, 5.1°
    Central Obstruction Diameter 158mm (6.22") (44% of aperture diameter)
    Light Gathering Power 2581x (Compared to human eye)
    Resolution (Rayleigh) 0.39 arc seconds
    Resolution (Dawes) 0.36 arc seconds
    Spot Size < 6.3 μm RMS across FOV
    Wavelength Range 400 – 900 nm
    Optical Coatings Enhanced aluminum, XLT Multi-Coated throughout
    Off-axis Illumination 83% at 30mm (1.18") off-axis
    Optical Window 104mm (4.09") Ø
    Back Focus (from collar) 77.5mm (3.05")
    Back Focus (with adapter) 55mm (2.16")
    Focuser Ultra-Stable Focus System (USFS)
    Mechanical Info
    Optical Tube Aluminum
    Optical Tube Length 1079.5mm (42.5")
    Optical Tube Diameter 406.4mm (16")
    Optical Tube Weight 75 lbs (34.02 kg)
    Other Features Ventilation fan, dual dovetail mounting bars
    • RASA 36 V2 Optical Tube Assembly

      × 1

    • M48 Camera Adapter

      × 1

    • Fan Battery Pack

      × 1

  • Celestron 2-Year Telescope Warranty