This telescope has been constructed with key features like
- Portability – they are movable and easy to assemble, a smaller looking telescope with easy to carry components.
- Stability – highly stable with the German Equatorial mounts placed over the tripod. Adjustable to a height of 50″.
- Balance – the CGEM equatorial mounts easily balances in both axes even with the added accessories of the telescope.
- Clearance – the CGEM mount supports the tubes at a single point of contact without disturbing its movement. This is useful for photography solutions.
Celestron CGEM 800 Computerized Schmidt-Cassegrain Telescope comes with the optical design of Schmidt-Cassegrain which uses both the mirror and lens technology. The aperture of this telescope is 8″ which provides a greater light gathering capacity and together with its magnification power of 81x clearer and brighter images of the far off objects can be obtained. Coming with a longer focal length of 2032mm for viewing Saturn’s rings, surface of moon, Mars and the far off planets like Neptune and Pluto.
- Celestron CGEM 800 Computerized starbright optical coating Telescope with a 6×30 finderscope.
- The computerized equatorial mount makes a difference for both celestial and terrestrial viewing and long exposure photography.
- Has an aluminum optical tube which is the best optical tube for outdoors.
- The three legged carbon steel tripod enhances its stability and also has adjustable height and angle.
- Designed with starbright optical coating which is a unique multi layer mirror coating, anti-reflective and high transmission white glass makes this telescope popular.
- Updated database of 40,000+ objects, 400 user defined programmable objects with information about over 200 objects for instant access and study. It includes deep sky objects, solar system, asterisms and variable stars.
- Easy operation with Double line, 16-character Liquid Crystal Display with Hand Control and backlit LED buttons.



magnitude +0.8 with an angular size of ~18.8 arc seconds and these fall to +0.9 and 18.1 as the month progresses. Saturn is significantly less bright this year than it sometimes is: the rings are very close to edge on (as shown in the Hubble image of Saturn) and thus there is less apparent reflecting area. During May they are at an angle of ~4 degrees from the line of sight. The rings will be seen (or rather – not seen) edge-on later this year and it will not be until 2016 that they will be at their widest again. A small telescope will easily show its largest moon, Titan, and show some bands around the surface.











