EXPLORER-200PDS (EQ5 PRO)

200mm (8") f/5 Parabolic Dual-Speed Go-To Newtonian Reflector

EXPLORER-200PDS (EQ5 PRO)
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SRP: £1,308.00

Product Code:  10220-20981
Brand:  Sky-Watcher



Sky-Watcher


  • Sir Patrick Moore CBE FRS"I have used a great number of telescopes; some are good, some mediocre and some bad. To me the Sky-Watcher range of instruments are very good indeed, and suited to amateurs of all kinds – and they are not priced out of the market! Excellent value.
    Use them and enjoy them."
    Sir Patrick Moore CBE FRS (1923 to 2012)

The new Sky-Watcher EXPLORER-200PDS Newtonian Reflector incorporates the same superb mirror-set as the Explorer-200P Black Diamond Series, but with two significant advantages. A Dual-Speed 10:1 ratio focuser is now included for excellent focusing precision. Also the tube length has been slightly shortened to optimise performance for prime-focus photography.

Even better performance for astro-photography and visual use can be achieved when used in combination with Sky-Watcher’s Newtonian coma corrector (Prod.Code 20233)

*Note: the Explorer-200PDS has a larger 58mm secondary mirror, for enhanced field illumination, compared to the Explorer-200P which has a 52mm secondary.

 

Standard Specification:

 

  • Magnification (with eyepiece supplied) x36
  • Highest Practical Power (Potential) x400
  • Diameter of Primary Mirror 200mm
  • Telescope Focal Length 1000mm (f/5)
  • Eyepiece Supplied 28mm LET (2"/50.8mm)
  • 9x50 Finderscope
  • Parabolic primary mirror & secondary mirror with Radiant™ Aluminum Quartz (RAQ™) coating providing up to 94% reflectivity with optimal durability and long term performance
  • 2" (50.8mm) Dual-Speed 10:1 Crayford Focuser
  • 0.5mm Ultra-Thin Secondary Mirror Supports
  • EQ5 PRO Go-To Equatorial Mount with 1.75" Stainless Steel Tripod
  • 42,900+ Object SynScan Computer Database
  • 77% more Light-Gathering than 150mm

PARABOLIC PRIMARY MIRRORS
Features High Quality Parabolic Primary Mirrors to eliminate spherical aberrations inherent in 'fast' focal lengh reflectors with spherical primary mirrors. The mirrors are parabolized to bring all the light rays to the same focal point to give sharp, constrasty images, which are full of detail.
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