Refractor Telescope Bresser Optics CLASSIC 60/900 EQ

The BRESSER Classic 60/900 EQ refractor telescope is a beginner-friendly optical instrument with a 60 mm objective lens and 900 mm focal length, supplied on an equatorial EQ-SKY mount and aluminium tripod. The metal optical tube, included eyepieces and smartphone adapter allow visual observation and basic astrophotography of the Moon, planets and bright deep-sky objects. The set contains astronomy software for starting observations and a mounting system designed to make celestial tracking and vertical adjustment straightforward.

Advantages

The telescope combines a classical achromatic lens design and a lightweight metal tube to deliver sharp images while remaining portable. The equatorial mount permits manual tracking of celestial objects as they move across the sky and the stable aluminium tripod reduces vibration. Included accessories such as eyepieces and a smartphone camera holder expand usability without requiring immediate additional purchases.

Suitable for

• Beginner astronomers and students
• Visual observation of the Moon and planets (e.g., Saturn, Jupiter)
• Basic astrophotography with a smartphone
• Educational use and introductory astronomy lessons

Key specifications

• Objective diameter: 60 mm
• Focal length: 900 mm
• Mount: Equatorial EQ-SKY
• Tripod: Aluminium
• Tube: Metal optical tube
• Approximate total weight: 6.5 kg
• MPN: 4660910, EAN: 4007922039787

How to use

Set up the aluminium tripod on a stable, level surface and attach the equatorial mount according to the included instructions. Secure the metal optical tube, fit a low-power eyepiece to locate targets, then switch to higher magnification eyepieces as required. Use the equatorial mount's adjustment controls to align the axis with the celestial pole for easier tracking; once polar alignment is completed, follow objects by turning the mount's slow-motion controls. The smartphone camera holder can be attached to the eyepiece for simple image capture.

Usage recommendations

For the best results observe from a dark location away from bright street lighting, allow the telescope to reach thermal equilibrium with outdoor temperatures, and perform a careful polar alignment on the equatorial mount before extended tracking or photography.