SharpStar 150mm f/2.8 HNT Hyperbolic Newtonian Astrograph
- Aperture: 150mm
- Focal Ratio: f/2.8
- Image Circle: 44mm
- Gross Weight: 6 kg
- Back-Focus: 55mm
Simulate the exact field of view of the SharpStar 150mm f/2.8 HNT Hyperbolic Newtonian Astrograph with your specific telescope.
Launch Visual Assistant
Simulate the exact field of view of the SharpStar 150mm f/2.8 HNT Hyperbolic Newtonian Astrograph with your specific telescope.
Launch Imaging AssistantThe 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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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 |