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Lunt LS60MT H-Alpha Solar Telescope - Premium PLUS Kit

UGC LSS-LS60MT-Premium
Prix d'origine CA$4,193.00 - Prix d'origine CA$4,193.00
Prix d'origine
CA$4,193.00
CA$4,193.00 - CA$4,193.00
Prix actuel CA$4,193.00
Égalisation de prix!
  • Aperture: 60mm
  • Focal Length: 420mm (F/7)
  • Bandpass (Double-Stack): <0.28Å
  • Tuning: Internal Pressure-Tuned Etalon (Doppler True Tuning)
  • Blocking Filter: B1200 in 2" Diagonal
  • Focuser: 2" Rack & Pinion
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • Observe the Sun's Chromosphere in High-Contrast Detail

    The Lunt LS60MT H-Alpha Solar Telescope - Premium PLUS Kit is a complete, modular system designed for the highest-resolution views of the Sun's dynamic chromosphere. By combining a high-quality 60mm ED doublet refractor with two precision-matched etalons, this package delivers a sub-0.28Å bandpass, transforming the solar disk from a flat, bright circle into a three-dimensional landscape of filaments, prominences, and active regions. It is the definitive choice for the observer who wants to resolve the finest surface structures the Sun has to offer in a portable, versatile instrument.

    The 60mm F/7 ED Doublet Optical Tube

    At the heart of the LS60MT is an F/7 ED doublet objective lens. The 60mm aperture provides a significant increase in resolving power over smaller 40mm and 50mm solar telescopes, rendering finer detail in solar granulation and the wispy texture of prominences. The use of Extra-low Dispersion (ED) glass minimizes chromatic aberration, which is critical not only for its nighttime performance but for ensuring the highest possible contrast at the focused H-alpha wavelength.

    This aperture is a carefully considered choice. It is large enough to resolve fine chromospheric detail yet small enough to remain largely immune to the effects of daytime atmospheric seeing. This results in more frequent opportunities for high-magnification observing compared to larger solar telescopes, which are often limited by local atmospheric turbulence.

    Internal Pressure-Tuned Etalon for Uniformity

    The primary filtering is performed by an internal, unobstructed etalon. Unlike front-mounted filters, this internal placement protects the most critical optical component from the elements. Lunt's Doppler True Tuning system uses air pressure to adjust the etalon's bandpass, a method that avoids the mechanical stress and potential tilting inaccuracies of other tuning systems. This ensures a uniform, on-band image across the entire field of view, free from hot spots or gradients.

    The observer's benefit is direct and immediate. As you adjust the pressure, you can shift the filter's bandpass slightly off the central H-alpha line. This allows you to track the Doppler-shifted motion of plasma in solar flares and active regions, adding a dynamic, real-time dimension to your observation that a static filter cannot provide.

    Double-Stack Etalon for Maximum Surface Contrast

    This Premium PLUS kit includes the matching LS50FHa front-mounted etalon, which works in series with the internal filter. This "double-stacking" dramatically narrows the final bandpass from a standard ≤0.45Å down to a very narrow <0.28Å. This reduction is the key to unlocking the highest-contrast views of the solar chromosphere.

    The visual effect is a significant darkening of the solar disk, which causes surface features like plage and filaments to stand out with pronounced definition. While a single-stacked view is excellent for prominences at the solar limb, the double-stacked view reveals the intricate, web-like structure of the chromosphere itself. For the dedicated solar observer, this enhanced contrast is not a luxury, it is the primary goal.

    The B1200 Blocking Filter Advantage

    The blocking filter is the final, essential stage in any dedicated solar telescope. This kit includes the upgraded B1200, which offers a 12mm aperture. This larger filter provides a wider, fully illuminated field of view compared to the standard B600, making it a better match for imaging with cameras that use larger sensors.

    Even for visual observers, the B1200 provides more generous eye placement and a more comfortable view when using wide-field, low-power eyepieces. It ensures that the edges of the field are not dimmed or vignetted, preserving the quality of the view from the center to the edge of the field stop.

    Robust 2" Rack & Pinion Focuser

    The LS60MT is equipped with a 2-inch rack and pinion focuser. This design is more robust than a helical focuser, providing the rigidity needed to support heavier eyepieces, Barlow lenses, or imaging cameras without slipping or flexing. The coarse and fine focus knobs allow for quick initial focusing followed by the precise adjustments needed to resolve delicate solar features.

    This choice of focuser is a practical one. It simplifies the process of switching between visual observation and imaging, and its non-rotating design means your camera orientation stays fixed as you focus, eliminating the need to re-frame your target after each adjustment.

    Modular Design for Day and Night Versatility

    The "MT" designation stands for Modular Telescope, a key feature of this system. The H-alpha module containing the etalon can be easily removed, and with an optional set of conversion accessories, the 60mm ED refractor can be used as a conventional telescope for nighttime astronomy or daytime terrestrial viewing. This dual-purpose capability represents a significant value.

    This is the system for an observer who wants one high-quality, portable refractor to do it all. You can spend the day observing the Sun in high-resolution H-alpha, and then, in minutes, convert the scope to view the Moon, planets, or star clusters at night. It is a true grab-and-go instrument for any time of day.

    The Double-Stacked Solar Experience

    With the zoom eyepiece included in this kit, center a large, arching prominence on the limb of the Sun at low power. Now increase the magnification. With the double-stack engaged, the prominence resolves into fine, feathery strands of plasma against a truly black sky. Now move your view onto the solar disk itself and focus on a long, dark filament snaking across the surface. The <0.28Å bandpass makes the filament appear almost three-dimensional, a dark river of cooler hydrogen suspended over the brighter, churning chromosphere below. This is the view that dedicated solar telescopes are built to deliver, and it is a sight that never gets old.

  • What's the main difference between the LS60MT and LS50THa?

    The LS60MT has a larger 60mm aperture for higher resolution and is a modular system that can be converted for nighttime use. The LS50THa is a dedicated 50mm solar telescope. The LS60MT also uses an internal pressure-tuned etalon, while the LS50THa uses a front tilt-tuned etalon.

    Do I really need a double-stack filter?

    For the highest-contrast views of solar surface detail, yes. A single-stack system is excellent for prominences on the Sun's edge, but a double-stack dramatically enhances the visibility of filaments, plage, and granulation on the disk itself by narrowing the bandpass.

    Why choose the B1200 blocking filter over the B600?

    The B1200 provides a larger, fully illuminated field of view. This is important for imagers using cameras with larger sensors to avoid vignetting, and it provides a more comfortable visual experience with low-power, wide-field eyepieces.

    What kind of mount do I need for the Lunt LS60MT?

    A lightweight, stable alt-azimuth mount like the Sky-Watcher AZ-GTe or a small equatorial mount is sufficient. The telescope is relatively light, but a solid platform is crucial for the fine focusing and tracking needed for solar observation.

    Can I use my regular nighttime eyepieces with this telescope?

    Yes, standard 1.25" and 2" astronomy eyepieces work perfectly with the LS60MT for both solar and nighttime viewing. The included zoom eyepiece is a versatile starting point, but high-quality planetary or wide-field eyepieces can enhance the view further.

    Is pressure tuning better than tilt tuning?

    Pressure tuning provides a more uniform view across the entire field because it doesn't tilt the etalon. This avoids creating an off-band gradient from one side of the image to the other. It is generally considered a more advanced and consistent tuning method.

  • Telescope Type Modular H-alpha Solar & Nighttime Refractor
    Aperture 60mm
    Objective ED Doublet, Air-Spaced
    Focal Length 420mm
    Focal Ratio F/7
    Primary Etalon Internal Pressure-Tuned, ≤0.45Å
    Secondary Etalon LS50FHa Front-Mounted, Tilt-Tuned
    System Bandpass <0.28Å
    Blocking Filter B1200 in 2" Star Diagonal
    Focuser 2" Rack & Pinion
    Tube Length 15.25" (387mm)
    Weight 6.6 lbs (3 kg)
    • LS60MT 60mm Modular Telescope

      × 1

    • LS50FHa Double-Stack Etalon Filter

      × 1

    • B1200 Blocking Filter in 2" Diagonal

      × 1

    • 2" Rack & Pinion Focuser

      × 1

    • SunLock Red Dot Sun Finder

      × 1

    • Lunt Zoom Eyepiece

      × 1

    • 4" Dovetail Rail (Vixen-style)

      × 1

    • Custom Hard Case

      × 1

  • Lunt Solar Systems 5-Year Warranty