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view), it’s like trying to find a needle in a haystack! Once
you’ve centered the object in the eyepiece, you can switch to
higher magnification (shorter focal length eyepiece), if you
wish.

The best rule of thumb with eyepiece selection is to start
with a low power, wide-field eyepiece, and then work your
way up in magnification. If the object looks better, try an even
higher magnification. If the object looks worse, then back off
the magnification a little by using a lower-power eyepiece.

What to Expect

So what will you see with your telescope? You should be
able to see bands on Jupiter, the rings of Saturn, craters on
the Moon, the waxing and waning of Venus, and many bright
deep-sky objects. Do not expect to see color as you do in
NASA photos, since those are taken with long-exposure
cameras and have “false color” added. Our eyes are not sen-
sitive enough to see color in deep-sky objects except in a
few of the brightest ones.

Remember that you are seeing these objects using your own
telescope with your own eyes! The object you see in your
eyepiece is in real-time, and not some conveniently provided
image from an expensive space probe. Each session with
your telescope will be a learning experience. Each time you
work with your telescope it will get easier to use, and stellar
objects will become easier to find. Take it from us, there is
big difference between looking at a well-made full-color
NASA image of a deep-sky object in a lit room during the
daytime, and seeing that same object in your telescope at
night. One can merely be a pretty image someone gave to
you. The other is an experience you will never forget!

Objects to Observe

Now that you are all set up and ready to go, one critical deci-
sion must be made: what to look at?

A. The Moon

With its rocky surface, the Moon is one of the easiest and
most interesting targets to view with your telescope. Lunar
craters, marias, and even mountain ranges can all be clearly
seen from a distance of 238,000 miles away! With its ever-
changing phases, you’ll get a new view of the Moon every
night. The best time to observe our one and only natural
satellite is during a partial phase, that is, when the Moon is
NOT full. During partial phases, shadows are cast on the
surface, which reveal more detail, especially right along the
border between the dark and light portions of the disk (called
the “terminator”). A full Moon is too bright and devoid of sur-
face shadows to yield a pleasing view. Make sure to observe
the Moon when it is well above the horizon to get the
sharpest images.

Use an optional Moon filter to dim the Moon when it is very
bright. It simply threads onto the bottom of the eyepieces
(you must first remove the eyepiece from the focuser to
attach a filter). You’ll find that the Moon filter improves view-
ing comfort, and also helps to bring out subtle features on
the lunar surface.

B. The Sun

You can change your nighttime telescope into a daytime Sun
viewer by installing an optional full-aperture solar filter over
the front opening of the ShortTube 4.5 EQ. The primary
attraction is sunspots, which change shape, appearance,
and location daily. Sunspots are directly related to magnetic
activity in the Sun. Many observers like to make drawings of
sunspots to monitor how the Sun is changing from day to
day.

Important Note: Do not look at the Sun with any optical
instrument without a professionally made solar filter, or
permanent eye damage could result.

C. The Planets

The planets don’t stay put like the stars, so to find them you
should refer to Sky Calendar at our website (telescope.com),
or to char ts published monthly in Astronomy, Sky &
Telescope,  
or other astronomy magazines. Venus, Mars,
Jupiter, and Saturn are the brightest objects in the sky after
the Sun and the Moon. Your ShortTube 4.5 EQ is capable of
showing you these planets in some detail. Other planets may
be visible but will likely appear star-like. Because planets are
quite small in apparent size, optional higher-power eyepieces
are recommended and often needed for detailed observa-
tions. Not all the planets are generally visible at any one time.

JUPITER: The largest planet, Jupiter, is a great subject for
observation. You can see the disk of the giant planet and
watch the ever-changing positions of its four largest
moons—Io, Callisto, Europa, and Ganymede.

SATURN: The ringed planet is a breathtaking sight when it is
well positioned. The tilt angle of the rings varies over a peri-
od of many years; sometimes they are seen edge-on, while
at other times they are broadside and look like giant “ears”
on each side of Saturn’s disk. A steady atmosphere (good
seeing) is necessary for a good view. You will probably see a
bright “star” close by, which is Saturn’s brightest moon, Titan.

VENUS: At its brightest, Venus is the most luminous object
in the sky, excluding the Sun and the Moon. It is so bright
that sometimes it is visible to the naked eye during full day-
light! Ironically, Venus appears as a thin crescent, not a full
disk, when at its peak brightness. Because it is so close to
the Sun, it never wanders too far from the morning or
evening horizon. No surface markings can be seen on
Venus, which is always shrouded in dense clouds.

MARS: The Red Planet makes its closest approach to Earth
every two years. During close approaches you’ll see a red
disk, and may be able to see the polar ice cap.

D. The Stars

Stars will appear like twinkling points of light. Even powerful
telescopes cannot magnify stars to appear as more than a
point of light. You can, however, enjoy the different colors of
the stars and locate many pretty double and multiple stars.
The famous “Double-Double” in the constellation Lyra and
the gorgeous two-color double star Albireo in Cygnus are
favorites. Defocusing a star slightly can help bring out its
color.

Содержание ShortTube 4.5 EQ 9849

Страница 1: ...l Consumer Optical Products Since 1975 Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831 763 7000 P O Box 1815 Santa Cruz CA 95061 INSTRUCTION MANUAL Orion ShortTube 4 5 EQ 9849 Equatorial Reflecting Telescope ...

Страница 2: ...g circle Right ascension slow motion control cable Latitude adjustment T bolt Tripod leg Leg lock knob Declination slow motion control cable Declination lock knob Declination setting circle Counterweight shaft Counterweight Counterweight lock knob Latitude lock T bolt not shown Azimuth lock knob Accessory tray bracket Accessory tray Tripod leg ...

Страница 3: ...ews should be tightened securely to eliminate flexing and wobbling but be careful not to over tighten or the threads may strip Refer to Figures 1 and 2 during the assembly process During assembly and anytime for that matter Do not touch the surfaces of the telescope mirrors or the lenses of the EZ Finder II or eyepieces with your fingers The optical surfaces have delicate coatings on them that can...

Страница 4: ...d the counterweight shaft into the equatorial mount at the base of the declination axis until tight 7 Remove the screw and washer on the bottom of the counterweight shaft and slide the counterweight onto the shaft Make sure the counterweight lock knob is ade quately loosened to allow the counterweight shaft to pass through the hole Position the counterweight about halfway up the shaft and tighten ...

Страница 5: ...s first tighten the R A lock knob with the counterweight shaft still in the horizontal position 5 With one hand on the telescope optical tube loosen the Dec lock knob The telescope should now be able to rotate freely about the Dec axis Loosen the tube ring clamps a few turns until you can slide the telescope tube forward and back inside the rings this can be aided by using a slight twisting motion...

Страница 6: ...your finger It s a non magnifying aiming device that superimposes a tiny red dot on the sky showing exactly where the telescope is pointed The EZ Finder II works by projecting a tiny red dot it s not a laser beam onto a lens mounted in the front of the unit When you look through the EZ Finder II the red dot will appear to float in space helping you locate even the faintest of deep space objects Th...

Страница 7: ...aligned with the Earth s rotational polar axis a process called polar alignment Polar Alignment For Northern Hemisphere observers approximate polar alignment is achieved by pointing the mount s R A axis at the North Star or Polaris It lies within 1 of the north celes tial pole NCP which is an extension of the Earth s rotation al axis out into space Stars in the Northern Hemisphere appear to revolv...

Страница 8: ...d just turn the R A slow motion control cable clockwise The Dec slow motion control cable is not needed for tracking Objects will appear to move faster at higher magnifications because the field of view is narrower Optional Electronic Drives for Automatic Tracking An optional DC electronic drive can be mounted on the R A axis of the equatorial mount to provide hands free tracking Objects will then...

Страница 9: ...telescope on the R A axis until the counter weight shaft is horizontal parallel to the ground Then loosen the Dec lock knob and rotate the telescope until it is pointing straight overhead The counterweight shaft is still horizontal Then retighten both lock knobs Similarly to point the telescope directly south the counter weight shaft should again be horizontal Then you simply rotate the scope on t...

Страница 10: ...en the three small alignment setscrews in the cen ter hub of the 3 vaned spider several turns Now hold the mir ror holder stationary be careful not to touch the surface of the mirrors while turning the center screw with a Phillips head screw driver Figure 9 Turning the screw clockwise will move the secondary mirror toward the front opening of the optical tube while turning the screw counter clockw...

Страница 11: ...e very center of the out of focus circle like the hole in a donut If the hole appears off center the telescope is out of collimation If you try the star test and the bright star you have selected is not accurately centered in the eyepiece the optics will always appear out of collimation even though they may be perfectly aligned It is critical to keep the star centered so over time you will need to...

Страница 12: ... dark adapted sensitivity As your eyes become dark adapted more stars will glimmer into view and you ll be able to see fainter details in objects you view in your telescope To see what you re doing in the darkness use a red filtered flashlight rather than a white light Red light does not spoil your eyes dark adaptation like white light does A flashlight with a red LED light is ideal or you can cov...

Страница 13: ...omfort and also helps to bring out subtle features on the lunar surface B The Sun You can change your nighttime telescope into a daytime Sun viewer by installing an optional full aperture solar filter over the front opening of the ShortTube 4 5 EQ The primary attraction is sunspots which change shape appearance and location daily Sunspots are directly related to magnetic activity in the Sun Many o...

Страница 14: ...f paint have virtually no effect on the visual performance of the telescope The large primary mirror and the elliptical secondary mirror of your telescope are front surface aluminized and over coated with hard silicon dioxide which prevents the aluminum from oxidizing These coatings normally last through many years of use before requiring re coating which is easily done To clean the secondary mirr...

Страница 15: ...15 ...

Страница 16: ...warranted instrument that proves to be defective provided it is returned postage paid to Orion Warranty Repair 89 Hangar Way Watsonville CA 95076 If the product is not registered proof of purchase such as a copy of the original invoice is required This warranty does not apply if in Orion s judgment the instrument has been abused mishan dled or modified nor does it apply to normal wear and tear Thi...

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