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Getting started, Choosing an eyepiece, Observing by moving the telescope manually – Meade Instruments LX80 User Manual

Page 21

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at least 200 yards away. If the distant object is not

in focus, turn the focus lock ring counterclockwise

to loosen the viewfi nder front cell (Page 8, Fig 1,

3). Twist the front cell until focus is achieved and

retighten the focus lock ring.

4. Unlock the RA lock (Page 8, Fig 1, 29) and the

DEC lock (Page 8, Fig 1, 30) so that the telescope

turns freely on both axes. Then point the main

telescope at a tall, well-defi ned and stationary

land object (e.g., the top of a telephone pole) at

least 200 yards distant and center the object in the

telescope’s eyepiece. Focus the image by turning

the optical tube focus knobs (Page 8, Fig 1, 11).

Retighten the RA and DEC locks and verify the

object is still centered in the eyepiece.

5. Look through the viewfi nder and loosen or tighten,

as appropriate, one or more of the viewfi nder

collimation thumbscrews (Page 8, Fig 1, 2) until

the viewfi nder’s crosshairs are precisely centered

on the object you previously centered in the main

telescope’s eyepiece.

NEVER point the telescope or viewfi nder directly
at or near the Sun at any time! Observing the Sun,
even for the smallest fraction of a second, will
result in instant and irreversible eye damage, as
well as physical damage to the telescope itself.

Check this alignment on a celestial object, such as

a bright star or the Moon, and make any necessary

refi nements, using the method outlined above in steps

4 & 5.

With this alignment performed, objects fi rst located

in the wide-fi eld viewfi nder will also appear in the

telescope’s eyepiece.

Choosing an Eyepiece

A telescope’s eyepiece magnifi es the image formed by

the telescope’s main optics. Each eyepiece has a focal

length, expressed in millimeters, or “mm.” The smaller

the focal length, the higher the magnifi cation. For

example, an eyepiece with a focal length of 9mm has

a higher magnifi cation than an eyepiece with a focal

length of 26mm when used with the same OTA.

Your telescope comes supplied with an eyepiece which

gives a wide, comfortable fi eld of view with high image

resolution.

Low-power eyepieces offer a wide fi

eld of view,

bright, high-contrast images, and eye relief during

long observing sessions. To fi nd an object with a

telescope, always start with a lower power eyepiece

such as the 26mm. When the object is located and

centered in the eyepiece, you may wish to switch

to a higher power eyepiece to enlarge the image as

much as practical for prevailing seeing conditions.

For information about optional eyepieces for the LX80

Series models, see OPTIONAL ACCESSORIES,

Page 52.

The power, or magnifi

cation of a telescope is

determined by the focal length of the telescope and the

focal length of the eyepiece being used. To calculate

eyepiece power, divide the telescope’s focal length

by the eyepiece’s focal length. For example, a 26mm

eyepiece is supplied with the LX80 Series. The focal

length of the 8” LX80 Series SC model is 2034mm (see

Specifi cations, Page 60).

Telescope Focal Length ÷ Eyepiece Focal Length

= Magnifi cation (Power)

Telescope Focal Length

= 2034mm

Eyepiece Focal Length

= 26mm

2034 ÷ 26

= 78

The eyepiece power, or magnifi cation is therefore 78X

(approximately).

Observing by Moving the Telescope
Manually

After the telescope is assembled and balanced as

described previously, you are ready to begin manual

observations. View easy-to-fi nd terrestrial objects such

as street signs or traffi c lights to become accustomed

to the functions and operations of the telescope.

For the best results during observations, follow the

suggestions below:

When you wish to locate an object to observe, fi rst

loosen the telescope’s RA lock (Page 8, Fig 1, 29)

and DEC lock (Page 8, Fig 1, 30). The telescope

can now turn freely on its axes. Unlock each axis

separately and practice moving your telescope.

Then practice with two unlocked axes at the same

time. It is especially important to practice this

step to understand how your telescope moves in

equatorial confi guration, as the movement of an

equatorial mount are not intuitive.

Use the aligned viewfi nder to sight-in on the object

you wish to observe. When the object is centered

in the viewfi nder’s crosshairs, re-tighten the RA

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Getting Started