SharpStar 130mm f/2.8 HNT Hyperbolic Newtonian Astrograph
- 130mm Hyperbolic Newtonian Optics
- 364mm Focal Length
- f/2.8 Focal Ratio
- 44mm Full-Frame Image Circle
- Total Assembled Weight: 4.8kg
Simulate the exact field of view of the SharpStar 130mm f/2.8 HNT Hyperbolic Newtonian Astrograph with your specific telescope.
Launch Visual Assistant
Simulate the exact field of view of the SharpStar 130mm f/2.8 HNT Hyperbolic Newtonian Astrograph with your specific telescope.
Launch Imaging AssistantThe SharpStar 130mm f/2.8 HNT Astrograph combines a 130mm hyperbolic primary mirror with a 364mm focal length to achieve its native f/2.8 optical speed. It illuminates a full 44mm image circle, covering modern full-frame sensors with a vast 6.9-degree field of view and resolving details down to 0.89 arc seconds. Weighing just 4.8kg with its rings and plate, this astrograph provides this wide-field imaging capability in a compact 400mm tube length.
At the core of the 130HNT is a fast, light-gathering optical system designed for one purpose: deep-sky imaging. The 130mm hyperbolic primary mirror, made from low-expansion PZ33 glass, works in tandem with a two-element corrector to deliver sharp stars across the field. This f/2.8 focal ratio allows you to capture faint details in nebulae and galaxies with significantly shorter exposure times compared to slower f/5 or f/7 systems.
The 130HNT is engineered to fully illuminate a 44mm image circle, making it an ideal match for full-frame DSLR, mirrorless, and dedicated astronomy cameras. A 65mm secondary mirror ensures there is no vignetting across these large sensors. This expansive 6.9-degree field of view lets you frame enormous targets like the Andromeda Galaxy (M31) or the entire North American Nebula (NGC 7000) in a single shot.
An astrograph's mechanical stability is just as critical as its optical design. The SharpStar 130HNT is built from all-metal components, featuring a rigid aluminum main tube and CNC-machined parts for the focuser, secondary bracket, and mirror cell. This construction ensures precise, repeatable collimation and minimizes mechanical flexure, even with a heavy imaging payload.
The imaging train is managed by a heavy-duty, dual-speed rack-and-pinion focuser designed to carry a payload of up to 3kg. This robust focuser can easily support a full-frame camera, filter wheel, and off-axis guider without slipping or tilting. An integrated 360° camera rotator allows you to frame your target perfectly without loosening any other components, while the standard 55mm back focus simplifies the process of connecting your camera and accessories using standard M48 spacers.
While a 130mm apochromatic refractor offers a maintenance-free, sealed optical tube, the SharpStar 130HNT provides a decisive advantage in speed. A typical 130mm APO has a focal ratio around f/7, whereas the 130HNT operates at f/2.8.
An f/2.8 focal ratio dramatically reduces the exposure time needed to capture faint deep-sky objects. Compared to a more common f/5.6 instrument, it gathers light four times faster. This means you can capture more data in a single night, improve your signal-to-noise ratio, and place less demand on your tracking mount.
The 44mm image circle is designed for full-frame sensors. Combined with the 364mm focal length, this provides a massive 6.9-degree field of view. This is wide enough to capture the entire Andromeda Galaxy (M31) and its satellite galaxies, M32 and M110, with plenty of surrounding space, making it ideal for large-scale mosaics and framing the biggest nebulae.
Yes, as a Newtonian reflector, the SharpStar 130HNT requires collimation to ensure the mirrors are perfectly aligned for sharp images. The primary mirror features three sets of user-friendly adjustment screws. While it requires a laser collimator or cheshire eyepiece, the process is straightforward and essential for achieving the telescope's specified 0.89 arc second resolution.
Absolutely. The 3kg payload capacity of the dual-speed rack-and-pinion focuser is specifically designed for modern imaging setups. A typical full-frame cooled CMOS camera, 7-position filter wheel, and an off-axis guider will fall well within this limit, preventing focuser sag or tilt during long exposures.
The 55mm back focus is the standardized distance required between the focuser's M48 thread and your camera's sensor for the optical corrector to work properly. This standard is used by most DSLRs (with a T-ring) and dedicated astronomy cameras, making it easy to achieve the correct spacing without complex calculations or custom adapters.
PZ33 is a borosilicate glass similar to Pyrex, with a very low coefficient of thermal expansion. This means as the temperature drops overnight, the mirror's shape remains stable, preventing the focus from shifting. This is a critical feature for maintaining sharp stars over a long imaging session.
| Aperture Size | 130mm |
| Focal Length | 364mm |
| Focal Ratio | f/2.8 |
| Image Circle | 44mm |
| Field of View | 6.9° |
| Resolution | 0.89 arc second |
| Limiting Visual Magnitude | 12.3 |
| Primary Mirror Type | Hyperbolic reflective mirror |
| Primary Mirror Material | PZ33 (similar to Pyrex glass) |
| Secondary Mirror Minor Axis | 65mm |
| Corrector | Two-element air-spaced refractive lenses (one ED glass) |
| Back Focus | 55mm |
| Main Tube Material | Aluminum |
| Main Tube Outer Diameter | 174mm |
| Main Tube Length | 400mm |
| OTA Weight | 3.8kg |
| Total Weight (with Rings & Plate) | 4.8kg |