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SharpStar 150mm f/2.8 HNT Hyperbolic Newtonian Astrograph

SKU SSO-15028HNT-AL
Original price CA$2,765.00 - Original price CA$2,765.00
Original price
CA$2,765.00
CA$2,765.00 - CA$2,765.00
Current price CA$2,765.00
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  • Aperture: 150mm
  • Focal Ratio: f/2.8
  • Image Circle: 44mm
  • Gross Weight: 6 kg
  • Back-Focus: 55mm
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  • Description
  • FAQ
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  • SharpStar 150mm f/2.8 HNT Hyperbolic Newtonian Astrograph

    The SharpStar 150mm f/2.8 HNT Hyperbolic Newtonian Astrograph is an imaging instrument engineered for speed, delivering a 420mm focal length at an exceptionally fast f/2.8 focal ratio. Its 150mm hyperbolic primary mirror and integrated corrector produce a flat, fully illuminated 44mm image circle, covering full-frame sensors with a vast 6-degree field of view. The entire system, including the tube ring and dovetail plate, weighs just 6kg, making it a portable solution for wide-field deep-sky astrophotography.

    150mm f/2.8 Hyperbolic Optics: A 44mm Flat-Field System

    The optical core of the 150HNT is its 150mm hyperbolic primary mirror, which achieves a native f/2.8 focal ratio. Unlike a standard parabolic mirror, a hyperbolic figure is designed to work as part of a system with a dedicated corrector, enabling superior off-axis correction across a large 44mm image circle. The primary mirror is made from PZ33, a low-expansion Pyrex-type glass that ensures thermal stability as ambient temperatures change.

    Both the primary and 70mm secondary mirrors feature enhanced aluminum coatings, guaranteeing light reflectivity of over 96%. This high throughput, combined with the fast focal ratio, allows you to capture faint details with significantly shorter exposure times, maximizing the data collected during clear nights.

    Integrated 3-Element Corrector for a 6° Field of View

    To deliver its expansive 6-degree field of view, the 150HNT incorporates a three-element, air-spaced corrector directly into the focuser assembly. This design, which includes one ED (Extra-low Dispersion) glass element, is optimized specifically for the hyperbolic primary, eliminating coma and ensuring pinpoint stars to the edge of a full-frame sensor. By integrating the corrector, the system removes the complexity of matching a third-party coma corrector and guarantees the specified 55mm back-focus distance.

    Rigid 2-Speed Focuser for Precise Control

    An astrograph's focuser must be rigid enough to carry a modern imaging train without flexure. The 150HNT is equipped with a dual-speed rack-and-pinion focuser capable of supporting a 3kg payload. The focuser includes a built-in camera rotator for effortless framing and is compatible with most electronic auto-focusers.

    Mechanical stability is reinforced throughout the optical tube. The CNC-machined secondary mirror support is a single, rigid piece designed to prevent misalignment and produce clean, sharp diffraction spikes. The primary mirror cell features three sets of adjustment screws for precise and stable collimation.

    Astrograph-Ready Build: 6 kg Total Weight with Rings & Plate

    Designed for portability and rapid deployment, the SharpStar 150HNT has a total weight of just 6kg, including its tube rings and a 200mm Losmandy-style dovetail plate. The compact 443mm tube length makes it easy to balance on a wide range of equatorial mounts. The package also includes a 200mm handle bar that adds rigidity and provides a convenient mounting point for guide scopes or other accessories via its integrated finder base.

    SharpStar 15028HNT vs. Standard 6" f/4 Newtonians: Speed and Correction

    While a standard 6" f/4 Newtonian is a capable imaging instrument, the SharpStar 150HNT is purpose-built for a higher tier of astrophotography. The primary differences lie in optical speed and field correction.

    • Exposure Time: At f/2.8, the 150HNT gathers light approximately twice as fast as an f/4 system. This means a 5-minute exposure on the 150HNT collects the same signal as a 10-minute exposure on an f/4 scope, effectively doubling your imaging efficiency.
    • Integrated Correction: The 150HNT's hyperbolic mirror and built-in corrector are designed as a single optical system to produce a flat 44mm field. A standard f/4 Newtonian requires a separate, often generic, coma corrector that may not fully correct the field or illuminate a full-frame sensor without vignetting.
    • Optical Design: The hyperbolic design allows for sharper stars at the edge of the field compared to what a standard parabolic mirror and separate corrector can typically achieve, especially on large sensors.
  • What kind of mount is required for the SharpStar 150mm HNT?

    With a gross weight of 6kg (including rings and dovetail), the SharpStar 150HNT is well-suited for mid-range equatorial mounts. For optimal tracking and guiding, a mount in the payload class of a Sky-Watcher HEQ5, iOptron CEM26, or larger is recommended, especially once a camera and guide scope are added.

    What is the advantage of a hyperbolic primary mirror in the 150mm HNT?

    A hyperbolic mirror is part of a more advanced optical design than the parabolic mirrors found in standard Newtonians. It is specifically figured to work in tandem with the built-in three-element corrector to achieve a wider, flatter, and better-corrected field of view across its 44mm image circle than a parabolic mirror with a separate, general-purpose coma corrector.

    How do I set the correct 55mm back-focus for my camera with the SharpStar 150mm HNT?

    The standard 55mm back-focus is measured from the base of the M48x0.75 male thread on the focuser's camera rotator. To achieve this distance, you will use a combination of extension tubes and adapters, such as an M48 T-ring for your DSLR or a set of spacers for a dedicated astronomy camera, to place your camera's sensor at the correct distance.

    How will the SharpStar 150mm HNT frame large targets like the North American Nebula (NGC 7000)?

    The SharpStar 150HNT is ideal for such targets. With its 420mm focal length and 6-degree field of view on a full-frame sensor, it can easily capture the entirety of the North American Nebula (NGC 7000) and the neighboring Pelican Nebula (IC 5070) in a single, richly detailed frame.

    Is the SharpStar 150mm HNT suitable for imaging small galaxies like the Whirlpool Galaxy (M51)?

    While the 150HNT can certainly image the Whirlpool Galaxy (M51), its wide 420mm focal length is optimized for large nebulae and star fields. M51 will appear relatively small in the frame. The astrograph's strength is capturing such galaxies within the context of their surrounding galactic cirrus and stellar environment, rather than for high-magnification detail.

    Can I use an electronic autofocuser (EAF) with the SharpStar 150mm HNT?

    Yes. The dual-speed rack-and-pinion focuser on the 150HNT is designed to be compatible with most common electronic auto-focusers (EAFs). This allows for precise, automated focusing which is critical for a fast f/2.8 system where the critical focus zone is very narrow.

  • Aperture Size 150mm
    Focal Length 420mm
    Focal Ratio f/2.8
    Image Circle 44mm
    Field of View 6 degrees
    Back-Focus 55mm
    Primary Mirror Type Hyperbolic reflective mirror
    Primary Mirror Material PZ33 (Pyrex-type glass)
    Corrector Three-element air-spaced (inc. one ED element)
    Secondary Mirror Minor Axis 70mm
    Resolution 0.77 arc seconds
    Limiting Visual Magnitude 12.7
    OTA Weight 4.8kg
    Gross Weight 6kg (including tube ring and dovetail plate)
    Main Tube Material Aluminum
    Main Tube Outer Diameter 193mm
    Main Tube Length 443mm
  • Askar 1-Year Warranty