background image

One of the most fascinating sights of Jupiter
are its moons. The four largest moons are
called the Galilean moons, after the
astronomer Galileo, who observed them for
the first time. If you’ve never watched the
Galilean moons in your telescope before,
you’re missing a real treat! Each night, the
moons appear in different positions around
the Jovian sky. This is sometimes called the
Galilean dance. On any given night, you
might be able to see the shadow of a moon
on the face of Jupiter, see one moon eclipse
another or even see a moon emerge from
behind Jupiter’s giant disk. Drawing the
positions of the moons each night is an
excellent exercise for novice astronomers.

Any small telescope can see the four
Galilean moons of Jupiter (Fig. 8), plus a few
others, but how many moons does Jupiter
actually have? No one knows for sure! Nor
are we sure how many Saturn has either. At
last count, Jupiter had over 60 moons, and
held a small lead over Saturn. Most of these
moons are very small and can only be seen
with very large telescopes.

Probably the most memorable sight you will
see in your telescope is Saturn. Although you

may not see many features on the surface of
Saturn, its ring structure will steal your
breath away. You will probably be able to see
a black opening in the rings, known as the
Cassini band.

Saturn is not the only planet that has rings,
but it is the only set of rings that can be
seen with a small telescope. Jupiter’s rings
cannot be seen from Earth at all—the
Voyager spacecraft discovered the ring after
it passed Jupiter and looked back at it. It
turns out, only with the sunlight shining
through them, can the rings be seen. Uranus
and Neptune also have faint rings.

Optional color filters help bring out detail
and contrast of the planets. Meade offers a
line of inexpensive color filters.

What’s Next?  Beyond the Solar System

:

Once you have observed our own system of
planets, it’s time to really travel far from
home and look at stars and other objects.

You can observe thousands of stars with
your telescope. At first, you may think stars
are just pinpoints of light and aren’t very
interesting. But look again. There is much
information that is revealed in stars.

ASTRONOMY RESOURCES

The Meade 4M Community
6001 Oak Canyon, Irvine, CA 92618

Astronomical League
Executive Secretary
5675 Real del Norte, Las Cruces, NM 88012

The Astronomical Society of the Pacific
390 Ashton Ave., San Francisco, CA 94112

The Planetary Society
65 North Catalina Ave, Pasadena, CA 91106

International Dark-Sky Association, Inc.
3225 N. First Avenue, Tucson, AZ 85719-2103

The first thing you will notice is that not
all stars are the same colors. See if you
can find blue, orange, yellow, white and
red stars. The color of stars sometimes
can tell you about the age of a star and the
temperature that they burn at.

Other stars to look for are multiple stars.
Very often, you can find double (or binary)
stars, stars that are very close together.
These stars orbit each other. What do you
notice about these stars? Are they 
different colors? Does one seem brighter
than the other?

Almost all the stars you can see in the sky
are part of our galaxy. A galaxy is a large

11

Looking at or near the 

Sun

will cause 

irreversible

damage to your eye. Do not point this telescope at or near the Sun. Do not look through the telescope as it is moving.

Meade114EQASTR  3/28/07  9:33 AM  Page 13

Summary of Contents for 114EQ-ASTR

Page 1: ...MEADE INSTRUCTION MANUAL 114mm 4 5 Equatorial Reflecting Telescope 114EQ ASTR www meade com Meade114EQASTR 3 28 07 9 33 AM Page 1 ...

Page 2: ...ur eye Eye damage is often painless so there is no warning to the observer that damage has occurred until it is too late Do not point the telescope at or near the Sun Do not look through the telescope or SmartFinder as it is moving Children should always have adult supervision while observing Meade114EQASTR 3 28 07 9 33 AM Page 2 ...

Page 3: ...ive lens has a diameter of 114mm The lens diameter is one of the most important pieces of information about the telescope The size of the objective lens determines how much detail you will be able to see in your telescope The focal length information will help later on to calculate magnification Setting up your telescope involves these simple steps Assemble your tripod Attach the accessory tray At...

Page 4: ...mbscrew 17 Eyepiece 18 Red dot viewfinder bracket see Inset B 19 Declination axis see Fig 5 20 Right Ascension lock see Fig 5 21 Declination lock see Fig 5 22 Red dot viewfinder 23 Telescope front dust cover not shown 24 Leg brace see Inset A 25 Right Ascension setting circle 26 Declination setting circle see Fig 5 27 Latitude dial see Fig 5 28 Sliding leg extension see Inset C 29 Focus knobs 30 A...

Page 5: ...r mounting bolt to a firm feel ATTACH THE RED DOT VIEWFINDER An eyepiece 17 has a narrow field of view A viewfinder 22 makes it easier to locate objects The red dot viewfinder has a red dot 3 b Slide the inner portion of the leg 39 in or out to the desired length Repeat for the other two legs c Rotate and tighten the leg lock thumbscrew to relock the leg lock d Repeat for the other two legs ATTACH...

Page 6: ... in ng g ATTACH THE OPTICAL TUBE TO THE MOUNT 1 Insert the two bolts on the bottom of the optical tube 4 into the bolt holes on the saddle plate 13 2 Tighten the attachment wingnuts 42 to a firm feel PREPARE MOUNT 1 Attach the flexible cables 3 and 4 See Fig 6 These cables are secured in place with a firm tightening of the thumbscrews located at the attachment ends of each cable 2 Tilt the polar a...

Page 7: ...d turn the focuser knob 29 until the image is sharply focused Center the object precisely in the eyepiece s field of view 2 Look through the red dot viewfinder Turn one or more of the viewfinder s alignment screws 32 Inset B until the red dot is precisely over the same object as you centered in the eyepiece 3 Check this alignment at night on a celestial object such as the Moon or a bright star and...

Page 8: ...n be located by its latitude and longitude celestial objects may also be located using Right Ascension and Declination For example You can locate 6 Fig 6 14 15 16 17 18 19 20 21 22 23 0 1 12 11 10 9 8 7 5 6 4 3 2 13 Rotation of the Earth 0 Dec South Celestial Pole Right Ascension Star Celestial Equator 90 Dec 90 Déc D e c l i n a t i o n North Celestial Pole Vicinity of Polaris Jupiter s four brig...

Page 9: ... aligned with the pole very little use of the telescope s Declination flexible cable control is necessary Virtually all of the required telescope tracking will be in Right Ascension For the purposes of casual visual telescopic observations lining up the telescope s polar axis to within a degree or two of the pole is more than sufficient with this level of pointing accuracy the telescope can track ...

Page 10: ...everything that there is to know about a telescope or what all the 8 Saturn s rings of ice dust and gas are huge and small at the same time The main rings are so large they could almost reach from the earth to the moon But they are only about a half of a mile just a few city blocks wide sights in the universe are but that s OK Just point and observe at first You will enjoy your telescope even more...

Page 11: ...ent No shadows are seen during a full Moon making it appear flat and uninteresting Look for different features on the Moon The most obvious features are craters In fact you can see craters within craters Some craters have bright lines about them These are called rays and are the result of material thrown out of the crater when it was struck by a colliding object The dark areas on the Moon are call...

Page 12: ...e dawn or after sunset because it is close to the Sun You can observe Venus going through crescent phases But you cannot see any surface detail on Venus because it has a very thick atmosphere of gas 10 STAR CHARTS Star charts and planispheres are useful for a variety of reasons In particular they are a great aid in planning a night of celestial viewing A wide variety of star charts are available i...

Page 13: ...only with the sunlight shining through them can the rings be seen Uranus and Neptune also have faint rings Optional color filters help bring out detail and contrast of the planets Meade offers a line of inexpensive color filters What s Next Beyond the Solar System Once you have observed our own system of planets it s time to really travel far from home and look at stars and other objects You can o...

Page 14: ...ts are formed red shift the big bang what are the different kinds of nebula what are comets asteroids and meteors and what is a black hole The more you learn about astronomy the more Fig 9 eyepiece barlow You will also be able to see some nebulas with your scope Nebula means cloud Most nebulas are clouds of gas The two easiest to see in the Northern Hemisphere are the Orion nebula during the winte...

Page 15: ...copes coarse and fine adjustment controls At higher powers astronomical objects will seem to move through the field of view of the eyepiece more rapidly Place the object to be viewed at the edge of the field and without touching the telescope watch it drift through the field to the other side before repositioning the telescope so that the object to be viewed is again placed at the edge of the fiel...

Page 16: ...iewing obstructions such as tall trees street lights headlights and so forth The best locations are dark locations the darker the better Deep space objects are easiest to see under dark skies But it is still possible to observe even in a city Surf the Web and visit your local library The internet contains a huge amount of astronomical information both for children and adults Check out astronomy bo...

Page 17: ...er increase the power of an eyepiece To find out how much your magnification is when you use a Barlow multiply your eyepiece s magnification by two Your 25mm low power eyepiece magnifies an object 28 times Multiply 28 by 2 and you get 56 times magnification with a Barlow Eyepiece s magnification x 2 Magnification with a 2X Barlow lens It s worth repeating Keep in mind that a bright clear but small...

Page 18: ...lignment procedure is simple and requires only a few minutes the very first time the telescope is used Take the time to familiarize yourself with the following collimation procedure so That you will recognize a properly collimated instrument and can adjust the collimation yourself if necessary A CORRECT COLLIMATION The properly collimated aligned mirror system in the Polaris 114 EQ AR assures the ...

Page 19: ...e entire primary mirror can be seen centered within the diagonal mirror reflecting When the diagonal mirror is correctly aligned it will look like Fig 13 Note The primary mirror is shown out of alignment C PRIMARY MIRROR ADJUSTMENTS If the diagonal mirror 1 Fig 15 and the reflection of the primary mirror 2 Fig 15 Fig 12 3 2 Primary Mirror Cell 4 5 3 2 2 1 3 1 2 2 1 3 4 A B C Collimation Primary Mi...

Page 20: ...enter within the out of focus star disk this is the shadow of the secondary mirror as shown in Fig 16C An improperly aligned telescope will reveal elongated circles Fig 16A with an off center dark shadow If the out of focus star disk appears elongated Fig 16A you will need to adjust the primary mirror Phillips head tilt screws of the primary mirror cell 3 Fig 12 To adjust the primary mirror tilt s...

Page 21: ...iety of sizes provide a high level of image resolution and color correction at an economical price Contact your Meade Dealer or see the Meade catalog for more information Visit us on the web at www meade com 19 Looking at or near the Sun will cause irreversible damage to your eye Do not point this telescope at or near the Sun Do not look through the telescope as it is moving Meade114EQASTR 3 28 07...

Page 22: ...purchased outside North America are not included in this warranty but are covered under separate warranties issued by Meade international distributors RGA Number Required Prior to the return of any product or part a Return Goods Authorization RGA number m mu us st t be obtained from Meade by writing or by calling 800 626 3233 Each returned part or product must include a written statement detailing...

Page 23: ...OBSERVER OBJECT NAME DATE TIME OBSERVED CONSTELLATION EYEPIECE SIZE SEEING CONDITIONS EXCELLENT GOOD POOR NOTES DRAWING OF IMAGE OBSERVATION LOG Meade114EQASTR 3 28 07 9 33 AM Page 23 ...

Page 24: ...OBSERVER OBJECT NAME DATE TIME OBSERVED CONSTELLATION EYEPIECE SIZE SEEING CONDITIONS EXCELLENT GOOD POOR NOTES DRAWING OF IMAGE OBSERVATION LOG Meade114EQASTR 3 28 07 9 33 AM Page 24 ...

Page 25: ...OBSERVER OBJECT NAME DATE TIME OBSERVED CONSTELLATION EYEPIECE SIZE SEEING CONDITIONS EXCELLENT GOOD POOR NOTES DRAWING OF IMAGE OBSERVATION LOG Meade114EQASTR 3 28 07 9 33 AM Page 25 ...

Page 26: ...OBSERVER OBJECT NAME DATE TIME OBSERVED CONSTELLATION EYEPIECE SIZE SEEING CONDITIONS EXCELLENT GOOD POOR NOTES DRAWING OF IMAGE OBSERVATION LOG Meade114EQASTR 3 28 07 9 33 AM Page 26 ...

Page 27: ...Meade114EQASTR 3 28 07 9 33 AM Page 27 ...

Page 28: ...www meade com Meade Instruments Corporation 6001 Oak Canyon Irvine California 92618 1 800 626 3233 Meade114EQASTR 3 28 07 9 33 AM Page 28 ...

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