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.