Sky Rover 60GPA f/6 ED APO Doublet Refractor Telescope

Sky Rover 60GPA: Big Performance, Backpack-Friendly Size!

The Sky Rover 60GPA is a compact apochromatic refractor built for astronomers and imagers who want premium performance without hauling around heavy gear. Weighing in at under 2 kgs (4.4 lbs), this lightweight 60 mm astrograph is incredibly easy to travel with, making it perfect for grab-and-go observing sessions, portable imaging rigs, and dark-sky adventures!

Its precision-crafted air-spaced ED doublet optical design, featuring Super ED glass, delivers sharp stars, impressive contrast, and excellent color correction across the field. Designed with astrophotographers in mind, the 60GPA includes a smooth dual-speed focuser with a built-in CAA (Camera Angle Adjuster) for fast, easy framing adjustments during imaging sessions. The threaded field flattener connection helps maintain optical alignment, while the dedicated 60GPA 1x flattener (sold seperately) supports full-frame cameras with excellent edge-to-edge performance. Whether you're capturing wide nebulae or simply exploring the night sky, the 60GPA delivers premium refractor performance in a portable package.

Versatility at the Forefront!

From detailed lunar landscapes to breathtaking nebulae and sprawling Milky Way star fields, this telescope is built to handle a wide variety of astronomical targets. Its sharp optics and wide-field capabilities make it equally at home exploring the Moon, capturing deep-sky objects, surveying rich star fields, or imaging stunning nighttime landscapes. Pair it with the proper solar filter (sold seperately) for safe daytime observing and experience intricate solar surface detail, prominences, and dynamic solar activity. Whether you're observing visually or building a portable astrophotography setup, this versatile refractor is ready for nearly any adventure under the sky.

Theoretical Spot Diagram

The above diagrams are derived from key ray traces in the professional optical design (showing the maximum outer envelope of the spot and not representing spectral energy distribution). In practical imaging, the final star profile will also depend on factors such as sensor pixel size, pixel arrangement, and spectral energy concentration. As a result, the actual image performance is often better than the theoretical ray-trace outline. The spot diagrams and explanations above are provided for reference only and should not be regarded as the final standard for imaging performance.