More detail than any other smart telescope.

12.5 megapixels on a 7.0 × 7.0 mm square sensor with 2 μm pixels. The square 1:1 format fills every pixel on round optics with useful data, while the fine pixel pitch resolves structure in nebulae and galaxies that larger-pixel sensors simply smear over. Limiting magnitude 16 opens targets no competitor can reach.

megapixel mosaics via CovalENS automated mode — the Vespera Pro 2 plans, captures, and assembles panels automatically, scaling to a 4.18° × 2.45° field of view across multiple nights.

Automated when you want it. Open when you don’t.

Adjust exposure time, gain, and framing manually. Capture calibration frames. Export 16-bit RAW FITS files ready for PixInsight, Siril, or any processing workflow. Beginners get a fully automated result; experienced imagers get full access to the imaging chain.

No dew heater. No ruined session.

An integrated humidity and temperature sensor activates the anti-fog system before condensation reaches the optics. No dew heater cables to route or remember — critical for humid Australian coastal and bush nights.

225 GB. Multi-night. Onboard.

225 GB of internal storage stores 30 multi-night imaging slots simultaneously. FITS frames, TIFF pre-stacks, and JPEG previews. A 30 MB/s USB-C connection transfers a night’s work to a laptop in minutes when you’re ready to process.

Resume where you left off. Automatically.

The Vespera Pro 2 automatically continues a mosaic project across multiple nights, restoring framing and settings between sessions without any manual intervention. Large-scale targets — the Vela Supernova Remnant, the Magellanic Clouds — become achievable from a dark paddock, not just a permanent observatory.

Deeper contrast from any backyard.

Internal precision optical baffles block stray-light paths that wash out contrast in light-polluted skies. The result is a higher effective dynamic range and deeper limiting magnitude than unshielded designs — a meaningful advantage from suburban Sydney, Melbourne, or Brisbane.