1.Basic Description: In addition to our revolutionary Penta Mirror Technology, Bushnell is proud to present yet another pioneering feature with this
2.
EYEPIECE WITH THE ERECTING LENS OR BARLOW IN ANY POSSIBLE CONFIGURATION
Selecting an Eyepiece:
1.You should always start viewing with the lowest power eyepiece, which in this case is the 15 mm lens. Note: the base power of each eyepiece is determined by the focal length of the telescope objective lens, which for this model is 750 mm. A formula can be used to determine the power of
each eyepiece: telescope OBJECTIVE lens focal length EYEPIECE focal length =
MAGNIFICATION (e.g. Using the 15 mm lens, the calculation would look like this: 750 mm ÷ 15mm = 50x or 50 power.)
2.Included with this telescope is a Barlow lens. Barlow lenses are used to double or triple the power of your telescope. Place your Barlow between the focusing tube and the penta mirror. Note: The
Penta Mirror Assembly when used in conjunction with the Barlow Lens and Eyepiece as shown in the Intended Configuration Diagram will yield an effective doubling power of the
magnification already acheived with the Barlow and Eyepiece configuration alone. The magnification calculation would look like this: 750 mm ÷ 20mm = 38 power. 38 power x 3=114 power. 38 x 3 x 2=228 power. (See Intended Configuration Diagram).
Focusing Telescope:
1.After selecting the desired eyepiece, aim main telescope tube at a
Pinion Focusing Mechanism (13).
2.While looking through selected eyepiece (in this case the 20 mm), slowly retract focusing tube by turning Rack and Pinion Focusing Mechanism until object comes into focus.
Aligning Finderscope:
Look through main telescope tube at low power and establish a
Now, objects located first with the Finderscope (16) will be centered in the field of view of the main telescope.
Never Look Directly At The Sun With Your Telescope
Permanent Damage To Your Eyes May Occur