INTRODUCTION
This manual details the set up, operation, specifications, and optional accessories of the Telestar
STANDARD EQUIPMENT (Refer to Fig. 1)
•Complete optical tube (objective lens diameter = 40mm; focal length = 600mm)
•25mm (25X), 6mm (100X) eyepieces (.965" O.D. “Outside Diameter”)
•Diagonal mirror (.965" O.D.)
•2X viewfinder with bracket
•
INSTALLATION:
1.Unfold the tripod (6, Fig. 1) and place the optical tube (1, Fig. 1) on top of the tripod. Then adjust the attachment screw (10, Fig. 1) to tighten (to a firm feel) the optical tube to the tripod.
2.Attach the viewfinder bracket (13, Fig. 1) to the optical tube (1, Fig. 1) with the eyepiece cup (14, Fig.1) pointing to the back, toward the telescope eyepiece (see diagram). Adjust the viewfinder as you are tightening the bracket so that it points in the same direction the optical tube is pointing.
3.Slide the diagonal mirror (3, Fig. 1) into the tube and tighten the thumbscrews to a firm feel to hold in place.
4.Place an eyepiece (7, Fig. 1) into the diagonal and tighten the thumbscrews to a firm feel to hold in place.
TO ACHIEVE A CLEAR AND SHARP FOCUS:
1.Place the telescope on a stable desk or platform.
2.Do not focus through window glass; this will result in an unclear image. View an object that is at least 50 meters or more distant.
3.Make use of the altitude control handle (5, Fig. 1) and the viewfinder (2, Fig. 1) to help locate an object to view.
4.Look through the eyepiece (7, Fig. 1) and rotate the focus knob (4, Fig. 1). Turn the knob with a slow and gentle motion.
5.Take your time and enjoy.
USING THE TELESCOPE
With the telescope assembled as described above, you are ready to begin observations.
1.First decide on an
2.To center an object in the main telescope, first use the viewfinder to
The 25mm eyepiece included as standard equipment is the best eyepiece to use for the initial finding and centering of an object. The low power 25mm eyepiece presents a bright, wide field of view, ideal for terrestrial and general astronomical observing of star fields, clusters of stars, nebulae, and galaxies. For lunar and planetary viewing, switch to a higher power eyepiece such as the
3.If you are observing an astronomical object (the Moon, a planet, star, etc.), you will immediately notice that the object is in a rather slow but continuous motion through the telescopic field of view. This motion is caused by the rotation of the Earth on its axis which results in an apparent motion of the object in the telescope’s field of view; i.e. although the Moon, planets and stars are, for practical purposes, fixed in