EXPLORER-150P (EQ3-2)

150MM (6") F/750 Parabolic Newtonian Reflector Telescope

EXPLORER-150P (EQ3-2)
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  • 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)

"Good for advanced observing"....."Saturn was a stunning sight"
BBC Sky At Night Magazine

The Sky-Watcher EXPLORER-150P is a fantastic choice for intermediate astronomers and also the serious beginner. With a large 150mm of light gathering aperture combined with superb parabolic optics, this telescope is a highly capable all-rounder with excellent performance for the observation of the Moon, planets, nebulae, galaxies and star clusters. Supplied with the EQ3-2 equatorial mount, which when polar aligned, will allow you to easily track objects as they move across the night sky via its slow motion control cables.
  • Magnifications (with eyepieces supplied): x30, x60, x75, x150
  • Highest Practical Power (potential):x300
  • Diameter of Primary Mirror: 150mm
  • Telescope Focal Length: 750mm (f/5)
  • Tube assembly available separately
  • Supplied complete with 10mm & 25mm eyepieces
  • 6x30 finderscope
  • x2 Barlow lens 1.25" (with camera adaptor)
  • Parabolic primary mirror & secondary mirrors 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
  • Direct SLR Camera Connection
  • EQ3-2 Deluxe Equatorial Mount
  • Built in Polar Alignment Scope Holder
  • Aluminium Tripod with Accessory Tray
  • 33% more Light Gathering than 130mm
  • Tube rings and dovetail mounting bar

Highly commended

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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