Skyliner-250P FlexTube™

254mm (10") F/1200 Parabolic Truss-Tube Dobsonian Telescope

SRP: £795.00

Product Code:  10157
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)
Dobsonian telescopes offer an incredible aperture-to-price ratio. The Dobsonian mount, popularized by John Dobson in the 1970.s, is a simple and efficient method of mounting a Newtonian reflector, based on the Alt-Azimuth principal. Fast and easy to set up, the Dobsonian mount consists of a box-type mounting which allows the telescope to pivot in altitude, while the box itself is rotated on a base in azimuth. The secret of the design is to correctly balance the optical tube and use frictional materials which allow it to be moved easily when nudged but to stay in position when not. The mount is designed to be driven by hand as opposed to slow motion controls. Sky-Watcher Dobsonians provide excellent all round performance for the observation the Moon and Planets and Deep Sky Objects such as Galaxies and Nebulae.
  • Magnifications (with Eyepieces supplied): x48 & x120
  • Highest Practical Power (Potential): x500
  • Diameter of Primary Mirror: 254mm
  • Telescope Focal Length: 1200mm (f/5)
  • Eyepieces Supplied (1.25"): 10mm & 25mm
  • Dual-Fit 1.25"/2" Crayford Focuser
  • Parabolic primary & secondary mirror with Radiant™ Aluminum Quartz (RAQ™) coating providing up to 94% reflectivity with optimal durability and long term performance
  • 0.5mm Ultra-Thin Secondary Mirror Supports
  • 9x50 Finderscope (straight)
  • Direct SLR Camera Connection
  • 3-Point tube locking system
  • Wooden Alt-Azimuth Mount with Accessory Tray
  • 56% more Light Gathering than 200mm

 
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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