Lunt LS80MT H-Alpha Solar Telescope - Enhanced Kit
- Aperture: 80mm Doublet
- Focal Length: 560mm
- Focal Ratio: f/7
- Bandpass: <0.4 Å (Single-Stack)
- Blocking Filter: B1800 (18mm)
- Focuser: Dual-Speed Rack & Pinion
Measure how tall a prominence stands and how long a filament runs on your own solar images.
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See exactly how your targets fit with the Lunt LS80MT H-Alpha Solar Telescope - Enhanced Kit, on real sky survey data.
Launch Imaging AssistantThe Lunt LS80MT H-Alpha Solar Telescope - Enhanced Kit is a multi-purpose instrument designed for the serious solar observer who demands both high-resolution views and the flexibility for imaging. Its 80mm aperture and internal pressure-tuned etalon deliver exceptionally detailed, high-contrast images of the Sun's chromosphere, resolving fine filaments, plage, and the intricate structure of solar prominences. This Enhanced Kit is built around the larger B1800 blocking filter, providing a fully illuminated field for larger camera sensors.
At the heart of the LS80MT is a precision 80mm f/7 doublet objective that focuses light to a sharp, high-contrast point. This optical purity is critical in a solar telescope, as it provides a clean, artifact-free image to the etalon, resulting in a darker background sky and more vibrant surface detail.
For the observer, this means the ability to push magnification on days of good seeing to resolve the fine, thread-like structure within sunspot umbras and the delicate, feathery texture of hedgerow prominences. The 560mm focal length provides a versatile image scale, suitable for full-disc views with longer focal length eyepieces and detailed close-ups with shorter ones, without requiring a Barlow lens.
Lunt's signature pressure-tuning system provides superior control over the etalon's bandpass. Unlike mechanical tilt-tuning which can introduce uneven illumination, pressure tuning adjusts the refractive index of the air between the etalon plates. This maintains a perfectly even, on-band image from edge to edge, which is crucial for uniform brightness in both visual observation and imaging.
This system allows you to precisely shift the filter's bandpass to track features moving at high velocity, such as solar flares or coronal mass ejections. By slightly increasing or decreasing the pressure, you can "Doppler shift" the view to highlight material moving towards or away from you, revealing dynamic details that would otherwise be invisible. The factory-verified bandpass of <0.4Å provides an ideal balance between surface detail and prominence brightness.
The Enhanced Kit includes the B1800 blocking filter, featuring a large 18mm aperture. This is a significant upgrade from the standard B1200, as it provides a much larger fully-illuminated field of view. For imagers using cameras with APS-C or larger sensors, this eliminates vignetting, ensuring the entire frame is evenly lit.
Visually, the kit's four flat-field eyepieces (8, 12, 16 and 19mm, all 1.25" barrels with 60° apparent fields) cover 29x to 70x, from full-disk views and limb surveys to tight crops on active regions. It transforms the telescope into a capable instrument for full-disc solar mosaics and general wide-field observation.
To handle the demands of modern imaging equipment, the LS80MT is equipped with a heavy-duty dual-speed rack and pinion focuser. This design offers a significant advantage over Crayford-style focusers by providing zero slippage, even when supporting a heavy camera, filter wheel, and Barlow lens. The coarse focus knob gets you into the general vicinity quickly, while the 10:1 fine-focus knob allows for the critical, minute adjustments needed to snap spicules into sharp relief.
The "MT" in LS80MT stands for Modular Telescope. The hydrogen-alpha module, containing the etalon, can be easily removed. With the optional Lunt Backing Plate and Focuser for nighttime mode, the 80mm f/7 objective can be used as a nighttime refractor for observing the moon, planets, and deep-sky objects. This versatility makes the LS80MT a complete observing system, saving you the expense and storage space of a separate nighttime refractor.
The included solar handle with built-in red dot finder is a safe and intuitive way to align the telescope with the Sun. The finder is built into the tube ring assembly and stays permanently aligned.
With the LS80MT and a medium-power eyepiece, the solar limb is no longer a simple, sharp edge. It resolves into a field of countless fiery spicules, tiny jets of plasma that give the chromosphere a "furry" appearance. Following a dark filament as it rotates to the edge of the disk, you can watch it transform into a magnificent prominence, a curtain of glowing hydrogen gas suspended in the blackness of space. The pressure tuner allows you to subtly adjust the view, making the prominence glow with maximum contrast against the background, revealing knots and streamers within its structure.
The primary trade-off for this versatility and aperture is portability. While manageable for one person, the LS80MT is a more substantial instrument than a 50mm or 60mm scope and requires a stable mount like an EQ5 or HEQ5-class equatorial mount for optimal performance, especially for imaging. It is the right choice for the observer who has a dedicated space or is willing to transport a larger setup for a significant increase in resolution and flexibility.
The B1800 blocking filter has an 18mm aperture, which provides a larger fully illuminated field of view compared to the standard B1200 (12mm). This is essential for imaging with larger camera sensors to avoid vignetting (darkened corners).
No, the included dual-speed rack and pinion focuser is designed for imaging. It is very robust and can handle the weight of most camera setups without slipping, and the 10:1 fine focus control is critical for achieving sharp solar images.
The single-stack <0.4Å bandpass provides an excellent balance for viewing both. It is narrow enough to show high-contrast surface detail like filaments and plage, while being wide enough to show bright prominences on the limb. For even higher surface contrast, it can be upgraded with a double-stack filter.
Due to its weight and length, the LS80MT requires a stable mount. A mid-sized equatorial mount like a Sky-Watcher HEQ5 or Celestron AVX is recommended for visual use, while a larger class mount is suggested for serious imaging to ensure stability.
Pressure tuning adjusts the air pressure around the internal etalon, changing its refractive index to shift the bandpass. This keeps the etalon perfectly parallel to the light path for a more uniform view across the entire field. Tilt tuning physically tilts the etalon, which can cause banding or uneven illumination, especially for imaging.
Yes. The LS80MT is fully compatible with Lunt's internal double-stack module (DSII-SFPT). Adding this module will narrow the bandpass to <0.28Å, which significantly increases the contrast and visibility of fine surface details on the sun's chromosphere.
| Telescope Type | Modular Solar Telescope |
| Aperture | 80mm |
| Objective | f/7 Doublet |
| Focal Length | 560mm |
| Focal Ratio | f/7 |
| Bandpass | <0.4 Angstrom |
| Tuning | Internal Pressure Tune (Doppler True Tuning) |
| Blocking Filter | B1800 (18mm clear aperture) |
| Focuser | 2" Dual Speed Rack & Pinion |
| Mounting | Solar Handle Tube Ring with 5.5" Vixen-style Dovetail |
| Storage | Hard Case with Custom-cut Foam |
| Focuser travel | 55-60 mm |
| Focuser load capacity | 2.5-3 kg |
| Mount included | No |
| Matching flattener / reducer | Lunt CAA 0.8x Reducer/Field Flattener (night imaging) |
LS80MT DBL OTA (internal pressure-tuned etalon)
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B1800 Blocking Filter
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2" R&P Focuser (10:1)
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Solar Handle w/ Red Dot Finder (integrated tube ring assembly)
× 1
5.5" Vixen Dovetail
× 1
Hard Case
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Eyepiece Set (8, 12, 16, 19mm)
× 1