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SharpStar SCA260 V2 260mm f/5 Super Cassegrain Astrograph

SKU SSO-SCA260V2
Original price CA$6,461.00 - Original price CA$6,461.00
Original price
CA$6,461.00
CA$6,461.00 - CA$6,461.00
Current price CA$6,461.00
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  • 260mm (10.2") Aperture Aspherical Primary Mirror
  • 1300mm Focal Length at a fast f/5 Focal Ratio
  • Massive 80mm Corrected Image Circle for Large Format Sensors
  • Lightweight Carbon Fiber Tube Weighing 14.5kg
  • 3.35" Focuser with 360° Rotator and 70mm Back Focus
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See exactly how your targets fit with the SharpStar SCA260 V2 260mm f/5 Super Cassegrain Astrograph, on real sky survey data.

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Check which filter and adapter sizes clear the sensor with the SharpStar SCA260 V2 260mm f/5 Super Cassegrain Astrograph, and how much light the corners lose.

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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • SharpStar SCA260 V2 260mm f/5 Super Cassegrain Astrograph

    The SharpStar SCA260 V2 is an imaging instrument designed for large-format sensors, combining a 260mm aspherical primary mirror and a fast f/5 optical system to produce a massive 80mm corrected image circle. With a native focal length of 1300mm, it achieves a theoretical resolution of 0.46 arc-seconds, capable of capturing fine detail in distant galaxies and faint nebulae. The entire optical tube assembly weighs only 14.5kg thanks to its carbon fiber construction, making it manageable for a wide range of equatorial mounts.

    260mm Aspherical Primary and 3-Element Corrector System

    At the heart of the SCA260 V2 is a 260mm aspherical primary mirror, a design that demands a far more sophisticated manufacturing and testing process than a simple spherical mirror. This advanced optical surface provides superior correction across the field. The primary is made from PZ33, a Pyrex-like glass that is more stable than the mirror materials traditionally used, which helps the optics stay consistent as temperatures change overnight.

    • Enhanced Aluminum Coatings: Both the primary mirror and the 120mm spherical secondary mirror feature high-reflectivity coatings that deliver more than 95% reflectivity, resulting in brighter images and shorter exposure times.
    • Three-Element Corrector: A 3-inch, three-element air-spaced corrector sits in the optical path. SharpStar uses it so the whole system can better achieve full-frame imaging and keep vignetting under control.
    • Aspherical Advantage: By correcting optical aberrations at the primary mirror itself, the design achieves a higher level of sharpness and contrast, which is critical for resolving fine details across the enormous imaging field.

    A Massive 80mm Corrected Image Circle

    The SCA260 V2 has an 80mm image circle. The 3-inch three-element corrector is there so the f/5 system can better achieve full-frame imaging and control vignetting, which makes the astrograph a strong match for large-sensor CMOS and CCD cameras.

    This enormous field of view allows you to capture vast nebulae complexes and galaxy clusters in a single frame, or create ultra-high-resolution mosaics with fewer panels. A full-frame sensor (43mm diagonal) and a medium-format chip such as the IMX461 (55mm diagonal) both fit well inside the 80mm circle.

    The Imaging Advantages of a 1300mm f/5 System

    The combination of a 260mm aperture and a 1300mm focal length strikes a powerful balance between image scale and light-gathering power. The f/5 focal ratio is much faster than slower f/8 or f/10 systems, allowing you to collect data on faint deep-sky objects much more quickly. This speed reduces individual sub-exposure times, minimizing the impact of tracking errors and changing atmospheric conditions.

    With a theoretical resolution of 0.46 arc-seconds, the SCA260 V2 has the resolving power to capture intricate details in spiral arms of galaxies like the Whirlpool Galaxy (M51) and resolve individual stars in dense clusters like the Hercules Cluster (M13). The 1300mm focal length provides the ideal image scale for many popular deep-sky targets when paired with modern CMOS sensors.

    14.5kg Carbon Fiber Tube and Thermal Stability

    The optical tube is constructed from a lightweight yet rigid carbon fiber material. This offers two key advantages for astrophotography: a high stiffness-to-weight ratio and minimal thermal expansion. The total OTA weight of 14.5kg places it within the payload capacity of many popular mid-to-high-end equatorial mounts.

    Carbon fiber's near-zero coefficient of thermal expansion means that the distance between the primary and secondary mirrors remains constant as the temperature drops. This keeps the focal point stable throughout a long imaging session, preventing focus drift that can ruin hours of data. As with any large reflector, give the telescope time outdoors to reach ambient temperature before imaging.

    3.35" Focuser, 360° Rotator, and 70mm Back Focus

    The SCA260 V2 is equipped with a dedicated 3.35" focuser whose load capacity SharpStar has upgraded, so it carries imaging accessories with no slippage and smooth operation. SharpStar also extended its travel to 50mm for greater practicability. The rear of the focuser incorporates several features essential for a modern imaging setup.

    • 360° Rotator: A 360° rotator at the rear of the focuser lets you frame your target without loosening the camera, which helps when composing mosaics or finding a guide star. SharpStar placed it behind the focusing unit so an EAF cable does not get tangled as you rotate.
    • 70mm Back Focus: A generous 70mm of back focus is available from the M48x0.75 thread, providing ample room for accessories like filter wheels, and off-axis guiders.
    • Versatile Connections: The focuser includes a system of adapter rings for M68x1, M54x0.75, and M48x0.75 threads, making it easy to connect to most imaging cameras and accessories on the market. A built-in 2-inch filter thread is also included for added flexibility.

    Mounting Points and Simplified Optical Alignment

    The SCA260 V2 is designed for practical field use. It includes a CNC-machined handle bar that not only makes transport easier but also serves as a mounting platform for guide scopes or other accessories.

    SharpStar has also simplified the optical axis mechanics: to adjust the secondary mirror, you only need to work its pull rod. Like any reflecting telescope, the SCA260 V2 benefits from a collimation check from time to time, and keeping it aligned is how you get the most out of its 0.46 arc-second resolution.

  • What imaging sensors can the SharpStar SCA260 V2's 80mm image circle cover?

    The 80mm image circle is large enough to fully illuminate professional-grade sensors with minimal vignetting. This includes full-frame sensors (e.g., IMX455, 43mm diagonal) and medium-format sensors (e.g., IMX461, 55mm diagonal), making it an ideal choice for creating large-scale mosaics and imaging wide fields of view.

    How does the f/5 focal ratio of the SCA260 V2 benefit deep-sky imaging?

    An f/5 focal ratio is considered fast for an astrograph of this aperture. It allows you to collect a significant amount of light in a shorter period compared to slower f/8 or f/10 systems. This reduces individual sub-exposure times, which can lessen the impact of tracking errors and changing atmospheric conditions.

    What is the advantage of the PZ33 primary mirror material in the SCA260 V2?

    PZ33 is a borosilicate glass with a very low coefficient of thermal expansion, similar to Pyrex. This means the mirror's shape remains stable as the temperature drops throughout the night, preventing the focal point from shifting. This thermal stability is critical for maintaining sharp focus during long-exposure astrophotography.

    How do I collimate the SharpStar SCA260 V2?

    SharpStar simplified the optical axis mechanics of the SCA260 V2: the secondary mirror is adjusted with its pull rod. Check alignment with a star test from time to time and adjust only when the star shows it is needed. The collimation manual in the Downloads tab was written for the SCA260F5, so some of its steps may not apply to the V2.

    Can I image the entire Veil Nebula (NGC 6960) with the SCA260 V2 and a full-frame camera?

    Yes. The Veil Nebula complex spans approximately 3 degrees of the sky. With the SCA260 V2's 1300mm focal length and a full-frame sensor (like a ZWO ASI6200), you can capture large sections of the nebula in a single frame and create a high-resolution mosaic of the entire complex in just a few panes.

    What class of mount is required for the 14.5kg tube weight of the SCA260 V2?

    Given the 14.5kg tube weight, plus the additional weight of a large camera, guide scope, and other accessories, a mount with an imaging payload capacity of at least 25-30kg (55-66 lbs) is recommended for stable, long-exposure astrophotography. Mounts in the Sky-Watcher EQ8, iOptron CEM70/CEM120, or equivalent class are appropriate.

    Is the 1300mm focal length of the SCA260 V2 good for planetary imaging?

    The SCA260 V2 is built as a deep-sky astrograph, and no planetary figures are published for it. Its 260mm aperture has a theoretical resolution of 0.46 arc-seconds, but at 1300mm the image scale is small for planets, and the large 120mm secondary mirror lowers contrast on fine planetary detail. It is at its best on galaxies, nebulae and star clusters.

    How does the carbon fiber tube help with focus stability on the SCA260 V2?

    Carbon fiber has a near-zero coefficient of thermal expansion. This means that as temperatures drop during an imaging session, the tube does not shrink like an aluminum or steel tube would. This keeps the critical spacing between the primary and secondary mirrors constant, preventing the focal point from shifting and ensuring your images remain sharp all night.

    What do the M68, M54, and M48 threads on the SCA260 V2 let me do?

    This system of included adapter rings provides maximum flexibility for connecting your imaging equipment. The larger M68 and M54 threads are ideal for connecting large format cameras and accessories directly to prevent vignetting, while the M48x0.75 adapter is the standard for connecting most full-frame cameras, filter wheels, and off-axis guiders.

    Can I use the SharpStar SCA260 V2 for visual observing?

    The SCA260 V2 is an astrograph, designed and corrected for photographic use. Its limiting visual magnitude is 13.8, but no eyepiece setup is described, and the large 120mm secondary mirror will result in a significant central obstruction, which reduces contrast on planetary and lunar details compared to a telescope designed for visual use.

  • Aperture 260mm
    Focal Length 1300mm
    Focal Ratio f/5
    Corrected Image Circle 80mm
    Primary Mirror Type Aspherical Reflector
    Primary Mirror Material PZ33 (Pyrex-like)
    Secondary Mirror Type Spherical Reflector
    Secondary Mirror Minor Axis 120mm
    Corrector Three-element air-spaced lens structure
    Focuser 3.35"
    Back Focus (from M48 thread) 70mm
    Tube Material Carbon Fiber
    Tube Diameter 304mm
    Tube Weight 14.5kg
    Resolution 0.46 arc-seconds
    Limiting Visual Magnitude 13.8
    Focuser Travel 50mm
    Rear / Camera-Side Connection M68x1 / M54x0.75 / M48x0.75 adapter rings
    Optical Design Super Cassegrain astrograph
    Mount No
    • SharpStar SCA260 V2 OTA

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  • SharpStar/Askar 1-Year Warranty