Meade LNT Instruction Manual Page 16

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16
OBSERVING
Observing By Moving the Telescope Manually
If you wish to observe a distant land object, such as a mountain top or a bird, you can observe
by merely pointing the telescope and looking through the eyepiece.
1. Loosen the telescope’s R.A. lock (
9, Fig. 1) and Dec lock (6, Fig. 1).
2. Move your telescope to observe distant street signs, mountains, trees, and other
structures. Use SmartFinder and/or the viewfinder to to help site-in on an object.
3. Center the object with SmartFinder’s red dot and then in the telescope eyepiece. When the
object is
centered in your eyepiece, remember to re-tighten the R.A. and Dec locks.
4. Practice focusing objects with the focus knob (
8, Fig. 1).
5. Once you get a feel for how your telescope moves and focuses, try to view something more
challenging, like a bird or a distant moving train.
NOTE: Viewing conditions vary widely from night-to-night and site-to-site.
Turbulence in the air, even on an apparently clear night, can distort images. Low-
power eyepieces, such as the Super Plössl 26mm supplied with your telescope, are
better suited to resolving images in poor viewing conditions.
You can also observe stars and objects in the night sky using this method, but note that objects
begin to slowly drift across the eyepiece field. This motion is caused by the rotation of the Earth.
As you become familiar with the AutoStar handbox operation, you can counteract the drift using
the automatic tracking feature in the AutoStar Setup menu (see "TO TRACK AN OBJECT
AUTOMATICALLY," page 18), or by using AutoStar's GO TO capabilities (see "GO TO
SATURN," page 20).
Terrestrial Observing
The LX90 ia an excellent high-resolution, terrestrial (land) telescopes. Viewing terrestrial
objects requires looking along the Earth's surface through heat waves. These heat waves often
cause degradation of image quality. Lower power eyepieces, like the Super Plössl 26mm
eyepiece, magnify these heat waves less than higher power eyepieces. Therefore, lower power
eyepieces provide a steadier, higher quality image. If the image is fuzzy or ill-defined, reduce
to a lower power eyepiece, where the heat waves do not have such an effect on image quality.
Observing in early morning hours, before the ground has built up internal heat, produces
better viewing conditions than during late afternoon hours.
Observing Using AutoStar's Arrow Keys
You may observe land and astronomical objects using AutoStar's Arrow keys to move the
telescope.
1.
Tighten the Dec and R.A.
loc
ks (
6 and 9,
Fig.
1
).
IMPORTANT NOTE:
Objects appear
upside-down and
reversed left-for-right
when observed in the
eyepiece when insert-
ed directly into the
(straight-through) eye-
piece holder – with the
diagonal prism in
place, images will be
right-side-up, but
reversed left-for-right.
This image inversion is
of no consequence
when observing
astronomical objects
and, in fact, all astro-
nomical telescopes
yield inverted images.
During terrestrial
observing, where a
fully-correctly-oriented
image (right-side-up
and correct left-for-
right) is desirable, an
optional #928 45°
Erecting Prism is
available. See
“OPTIONAL
ACCESSORIES,” page
41.
Too Much Power?
Can you ever have too much power? If the type of power you’re referring to is
eyepiece magnification, yes, you can! The most common mistake of the
beginning observer is to “overpower” a telescope by using high magnifications
which the telescope and atmospher
ic conditions cannot reasonably support.
Keep in mind that a smaller, but bright and well-resolved image is far superior to
one that is larger, but dim and poorly resolved (see Figs. 8a and 8b). Powers
abo
v
e 400X should be emplo
y
ed only under the steadiest atmospheric
conditions
.
AutoStar can calculate the best eyepiece for you to use. Try out the “Eyepiece
Calc” feature in the Utilities menu.
Most observers should have three or four additional eyepieces to achieve the full
range of reasonable magnifications possible with the
LX90 telescopes. See
OPTIONAL A
CCESSORIES
, page 41.
LX90 TIPS
Fig. 8a & 8b: Jupiter:
Examples of the right
amount of magnification and
too much magnification.
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