Instruction Manual
LT ACF and LT SC Series Telescopes
with AutoStar #497 Hand Controller
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CONTENTS
Introduction
Object Menu . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .24
#497 AutoStar Menu Tree. . . . . . . . . . . . . . . . . . . .25
Event Menu. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .26
Glossary Menu . . . . . . . . . . . . . . . . . . . . . . . . . . . .27
Utilities Menu. . . . . . . . . . . . . . . . . . . . . . . . . . . . . .27
Setup Menu. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .28
A solid telescope built for a lifetime of service. . . . . .4
Getting Started
Assembling the and Using the LT Telescope
Assembling the Tripod. . . . . . . . . . . . . . . . . . . . . . . .5
Mounting the Tripod . . . . . . . . . . . . . . . . . . . . . . . . .6
Installing the Batteries. . . . . . . . . . . . . . . . . . . . . . . .6
Using an AC Adapter or DC Power Cord . . . . . . . . .6
Attaching Accessories. . . . . . . . . . . . . . . . . . . . . . . .7
Telescope is now Fully Assembled . . . . . . . . . . . . . .7
Using the Red Dot Finder . . . . . . . . . . . . . . . . . . . . .8
Adjusting the Red Dot Finder . . . . . . . . . . . . . . . . . .8
Aligning the LT Series . . . . . . . . . . . . . . . . . . . . . . . .9
The LT Series Home Position . . . . . . . . . . . . . . . . . .9
Magnetic North Home Position . . . . . . . . . . . . . . . . .9
True North Home Position. . . . . . . . . . . . . . . . . . . . .9
Moving Through AutoStar’s Menus. . . . . . . . . . . . .10
Initializing AutoStar . . . . . . . . . . . . . . . . . . . . . . . . .10
Easy (Two-Star) Align . . . . . . . . . . . . . . . . . . . . . . . 11
How to Perform the Easy Align Procedure . . . . . . . 11
Go To Saturn. . . . . . . . . . . . . . . . . . . . . . . . . . . . . .12
Using the Guided Tour . . . . . . . . . . . . . . . . . . . . . .12
Advanced AutoStar Features
Adding Observing Sites. . . . . . . . . . . . . . . . . . . . . .31
Finding Objects Not In the Database . . . . . . . . . . .32
GoTo a User-entered Object. . . . . . . . . . . . . . . . . .32
Observing Satellites . . . . . . . . . . . . . . . . . . . . . . . .32
How to Create Your Own Guided Tour . . . . . . . . . .33
Writing a Tour . . . . . . . . . . . . . . . . . . . . . . . . . . . . .34
Landmarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .37
Identify . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .38
Two-Star Alt/Az Alignment. . . . . . . . . . . . . . . . . . . .38
Browse . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .40
Maintenance
Basic Maintenance . . . . . . . . . . . . . . . . . . . . . . . . .41
Collimation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .41
Inspecting the Optics. . . . . . . . . . . . . . . . . . . . . . . .43
Gauging the Movement of the Telescope . . . . . . . .43
Updating Your LT Series Firmware . . . . . . . . . . . . .43
LT Series Key Features
Meade Customer Service
Telescope
How to get in contact. . . . . . . . . . . . . . . . . . . . . . . .43
Key Features Identified on the Telescope. . . . . . . .13
Key Features Explained . . . . . . . . . . . . . . . . . . . . .15
Appendix A:
Optional MEADE® Accessories
Training the Drive . . . . . . . . . . . . . . . . . . . . . . . . . .44
Choosing Eyepieces . . . . . . . . . . . . . . . . . . . . . . . .16
Meade Series 4000 Super Plössl Eyepieces . . . . .16
Meade Series 5000 Premium Eyepieces . . . . . . . .15
Power Supplies. . . . . . . . . . . . . . . . . . . . . . . . . . . .18
Imagers and related Accessories . . . . . . . . . . . . . .18
Appendix B:
Basic Astronomy . . . . . . . . . . . . . . . . . . . . . . . . . . .45
Appendix C:
Specifications . . . . . . . . . . . . . . . . . . . . . . . . . . . . .47
AutoStar #497 Handbox – Basic Usage
Buttons, Display and their functions . . . . . . . . . . . .19
Observing Using AutoStars’ Keys . . . . . . . . . . . . . .21
Observe the Moon. . . . . . . . . . . . . . . . . . . . . . . . . .22
Terrestrial Observing. . . . . . . . . . . . . . . . . . . . . . . .22
LT Series Tips . . . . . . . . . . . . . . . . . . . . . . . . . . . . .22
Appendix D:
Optical Systems . . . . . . . . . . . . . . . . . . . . . . . . . . .49
Appendix E:
Meade DoC. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .50
AutoStar Operation
AutoStar Navigation Exercise . . . . . . . . . . . . . . . . .23
Entering Data into AutoStar. . . . . . . . . . . . . . . . . . .24
Guided Tour Menu. . . . . . . . . . . . . . . . . . . . . . . . . .24
Meade Warranty
One Year Limited Warranty. . . . . . . . . . . Back Cover
® The name “Meade,” “AutoStar” and the Meade logo are trade-
marks registered with the U.S. Patent and Trademark Office and
in principal countries throughout the world. “Deep Sky Imager”, “LT
Series”, and “Tonight’s Best” are trademarks of Meade Instruments
Corp.
Patents:
US 7,277,223, US 7,079,317, US 7,092,156
US 6,304,376, US 6,369,942, US 6,392,799
© 2009 Meade Instruments Corp.
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INTRODUCTION
The LT Series ACF and LT Series SC Telescope
A solid telescope built for a lifetime of service
Congratulations on receiving your new LT Series telescope. You’ll find that this telescope system has all you need
to explore the Universe we live in. Meade’s concept was to create a telescope that would be simple enough for
anyone to use, yet capable enough for the experienced amateur to stretch their knowledge and skills. With the LTs’
advanced set of features, you will have plenty of room to learn and expand your interest in astronomy and not out
grow your telescope. Here are a few of the features that set the Meade LT Series telescope system apart from all
others.
Optics:
Your choice of optical systems to meet your needs. Meade’s Schmidt-Cassegrain (SC) optics
give you high performance for the best possible price. Water-white glass, Ultra-High Transmission
Coatings (UHTC) and oversized, thermally-stable Pyrex® primary mirrors provide spectacular
viewing experience not available on comparable competitors’ telescopes. Advanced Coma-Free
takes all of the features of our SC models and then ups the ante. ACF gives a flatter, coma-free
field of view with pinpoint images all the way to the edge of the field, equaling Ritchey-Crétien
performance. ACF is the perfect solution for the serious astroimager or visual astronomer looking
for observatory-class optics.
Mechanics: Strong and stable aluminum castings with large precision worm-gear drives in both axes for smooth
tracking with low periodic error.
Computer: AutoStar #497 handbox gives you complete control of your LT Series system from the palm of your
hand. With a database of over 30,000 objects, you will never run out of things to explore.
If you are like us, you can’t wait to get outside under a dark sky to try out your new LT Series telescope. We have
provided a Getting Started Guide that will get you up and running in the shortest amount of time possible. After
your first experience, please sit down with this manual and read about all the advanced features that are available
to you with this telescope system. We are confident that the LT Series will keep you fascinated with the Universe
and entertained for many years to come.
Clear Skies,
The people at Meade
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GETTING STARTED
You may want to perform the LT telescope assembly indoors in the light so that you become familiar with the
parts and operation before moving the telescope outside into the dark for observing. This Getting Started Guide
assumes you are too impatient to read the entire manual first and want to use your new telescope as quickly as
possible. Just follow the simple steps below and you will be up and running before you know it.
ᕡ
It is best to set up the telescope in twilight or before
sunset the first time you use it. Take the telescope and
tripod outside. Set the telescope in a large open area
where you can see lots of sky. Don’t setup right next
to a building or a wall. Make sure the ground is stable
and is approximately level. It is best to set up the scope
away from bright nighttime lighting. Bright lights will
spoil your night vision and impede your ability to see
the sky.
Lock-Knob
Assembling the Tripod
ᕣ
Thread in two lock-knobs on each leg (six total)
near the foot of each tripod leg. Use the lock-knobs
to vary the height of the inner, extendible tripod leg
sections. Tighten the locks to a firm feel only; do
not overtighten.
Spreader Shaft
End Nut
ᕢ
Remove the field tripod from the shipping carton.
Spreader Bar
Stand the tripod vertically with the tripod feet down
and with the tripod still fully collapsed. Grasp two of
the tripod legs and, with the full weight of the tripod
on the third leg, gently pull the legs apart to a fully
open position.
ᕤ
Remove the end nut from the spreader shaft
and slide the spreader in between the telescope
legs. Attach the end nut and hand tighten until the
telescope legs are held snuggly in the most spread
position. Position the tripod where you want the
telescope to be and check that the top of the tripod is
approximately level.
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Mounting the Telescope
Center Hub
Follow the battery
polarity (orientation)
as indicated by
molded icons
Thumb-Screw
CAUTION: Use care to install batteries as indicated by
thebatterycompartment. Followbatterymanufacturer’s
precautions. Do not install batteries backwards or mix
new and used batteries. Do not mix battery types. If
these precautions are not followed, batteries may
explode, catch fire, or leak. Improperly installed
batteries void your Meade warranty. Always remove
the batteries if they will not be used for a long period
of time.
ᕥ
Take the LT Series from its packaging and place
the entire telescope onto the top of the tripod head.
Rotate the telescope head slowly until you feel the
scope register on the center hub of the tripod head.
Carefully screw the three attachment thumb-screws
on the bottom of the plate to the base of the tripod.
Hand tighten the screws so the telescope cannot spin
or wobble on the tripod head.
Using an AC Adapter or
DC Power Cord
Installing the Batteries
Power
Port
ᕧ
Use only the optional Meade Universal AC Power
Adapter (part number 07584 for North America or
07584F for 220v foreign) with your LT Series telescope
when connecting toAC power. It is specifically selected
to provide the quality voltage and current required to
power and protect the electronics in the telescope.
Power adapters from other manufactures may cause
damage and void your warranty.
ᕦ
Remove the end cover from the battery
compartment exposing the battery tray. Carefully slide
the battery tray out until it reaches its end stop. Insert
8 (user supplied) Alkaline “C” batteries into the battery
compartment. Take care that the batteries + and - ends
are as indicated in the battery holder.
Slide the battery compartment back into the telescope
and re-attach the battery compartment cover.
Plug the AC plug into a AC household socket
and the DC plug into the 12v DC socket on the
telescope panel.
For external DC power use the optional #607 DC Power
Cord (part number 07043) to connect to an automotive
12v DC accessory socket.
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Attaching Accessories
Your Telescope is now Fully Assembled
µ
Now remove the dust cover from the front
of the telescope tube. Be careful not to touch the
glass lens.
ᕨ
Be sure the telescope master power switch is in
the off position. Remove the LT Series handbox and
the coiled interface cable from the packing materials.
Plug one end into the HBX port of the control panel
and plug the other end into the Handbox port on the
LT Series handbox.
¸
Flip the Power Switch on the computer control
panel to the ON position. The copyright message lights
on AutoStar’s LCD display.
Eyepiece Holder
Rear Cell Thread
Slew Speeds:
Speed 9: Fast
Arrow
Keys
.
.
.
Speed 5: Medium
.
.
.
Speed 1: Slow
Number
Keys
Dust Cap
Diagonal Prism
¹
“Press 0 to align or Mode for Menu” displays. You
ᕩ
Remove the dust cap from the rear cell of the
can use the Arrow keys to slew (move) the telescope
up, down, right, or left. To change the telescope’s slew
speed, press a Number key. “9” is the fastest speed
and “1” is the slowest speed. See page 20 for more
details. Or you can Press “0” to begin Easy Alignment.
See page 11 for more information.
telescope. Thread the 1.25" eyepiece holder onto
the rear cell thread. Slide the diagonal prism into
the eyepiece holder and lock in place by turning the
thumbscrew to a firm feel. Place the Super Plössl
26mm eyepiece into the diagonal prism and tighten the
diagonal prism thumbscrew to a firm feel only.
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Adjusting the Red Dot Finder
Using the Red Dot Finder
On/Off &
Brightness
Adjustment
Because your telescope has so much magnification,
its field of view is very small. This can make it
hard to know exactly where your telescope is
pointing by simply looking at it. To help you point
the telescope quickly and accurately, for terrestrial
targets or GO TO pointing, the LT Series has a 1X
Red Dot Viewfinder.
The Red Dot Finder has been aligned at the factory,
but you may need to touch-up the alignment from time
to time. To do this, look through the eyepiece of your
scope and using the hand controller center a distant
object. Now turn on the Red Dot Viewfinder and adjust
the brightness so you can see the red dot. Look through
the sight as pictured above.
The Red Dot Finder will aid you in pointing your
telescope easily. It works much like a fighter pilot’s
heads-up display. To turn on the Red Dot Finder,
carefully rotate the power switch until you feel it click
on. Turning further clockwise will increase the dot
brightness. Adjust the dot to the minimum brightness
where it can be easily seen. This will extend its
battery life and make it easier to see faint stars in the
background. Look through the finder’s glass window.
You will see a red dot superimposed on your view.
Using the direction keys on the handbox, move the
telescope until the red dot is on the target you want to
view in the eyepiece. As you get close to your target,
select a moderately low speed, like speed 5, and move
the scope to center your target as you look through the
eyepiece. This a great way to get used to finding the
movement keys without removing your eye from the
eyepiece.
Adjustment
Screws
Now, without moving the telescope, adjust the indicated
thumb screws until you have put the red dot on the
object at which you were looking. It’s that simple.
Now use the hand controller to put the laser dot on a
new target. Check to see that the desired target is in
the eyepiece and adjust the focus knob until the object
is in focus.
Focus Knob
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2. Now use the up/down arrow keys on the AutoStar
controller to level the optical tube using bubble level
feature to precisely level the optical tube.
Aligning the LT Series
As the Earth rotates beneath the night sky, the stars
appear to move from East to West. The speed at
which the stars move is called the sidereal rate. You
can setup your telescope to move at the sidereal
rate so that it automatically tracks the stars and
other objects in the night sky. If the telescope is not
tracking an astronomical object, the object will drift
out of the eyepiece field of view. The tracking function
automatically keeps an object more or less centered in
the telescope’s eyepiece.
3. The telescope is now in the Magnetic North Home
Position.
True North Home Position
1. Using the up/down arrow keys (pg. 19, Fig. 5, 5)
on the AutoStar controller, move the telescope so that
the optical tube is approximately level. Now use the
left/right arrow keys (pg. 19, Fig. 5, 5) to move the
telescope so the optical tube is pointing in the direction
of True North (the north star Polaris).
To automatically track and locate objects in the night
sky, the LT Series must first be aligned on the sky.
It is best to set up the telescope in twilight or before
sunset the first time you use the LT Series. Setup the
telescope in a large open area where you can see lots
of the night sky. Make sure the ground is stable and
approximately level. It is best to setup the scope away
from bright nighttime lighting. Bright lights will spoil your
night vision and impede you ability to see the sky.
2. Now use the up/down arrow keys on the AutoStar
controller to level the optical tube. The included bubble
level/compass can be place into the diagonal prism
and has a built in bubble level feature that will aide in
leveling the optical tube if needed.
3. The telescope is now in the True North Home
Position.
The LT Series Home Position
North
Once the LT Series is fully assembled, you will first
need to initialize AutoStar, set the telescope into the
home position, and perform the Easy Alignment in
order for the LT Series to successfully locate celestial
objects. The home position for the LT Series is with the
telescope optical tube level and pointed in the direction
of either True North or Magnetic North. See Figure 6.
Either North direction can be used and the LT Series
will prompt you to which North direction the optical
tube is pointing before beginning an alignment. Once
the telescope is fully assembled and outside under the
night sky, follow the steps below to correctly place the
telescope into the home position.
Telescope
Tube is level
Figure 6: Alt/Az Home Position
Compass
needle is
pointing to
Magnetic
North
Magnetic North Home Position
Bubble is
centered
1. Using the up/down arrow keys (pg. 19, Fig. 5, 5) on
the AutoStar controller, move the telescope so that the
optical tube is approximately level. Place the included
bubble level/compass into the diagonal prism and use
the AutoStar left/right arrow keys (pg. 19, Fig. 5, 5)
to move the telescope so the optical tube is lined up
with the compass needle. The telescope will then be
pointing in the direction of Magnetic North.
Figure 7: Bubble Level/Compass
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change this setting later on, use the Site menu.
See SITE, page 34 for more information.
Moving Through AutoStar’s Menus
The AutoStar database is organized in levels for quick
and easy navigation.
a. If you chose the zip code option, the left most
“0” is highlighted. Use the Number keys to enter
the digits. As you enter a digit, the next digit to
the right will be highlighted. Enter the next digit.
Repeat this process until all 5 digits of your zip
code are entered. Press ENTER.
• Press ENTER to go deeper into AutoStar’s
menu levels.
• Press MODE to move back toward the top
menu level.
• Press the Scroll keys to move up and down
through the options available for each level.
b. If you chose the location option, the next screen
asks for the country or state/province (listed
alphabetically) of the observing site.
• Press the Arrow keys to enter characters and
digits.
c. Use the Scroll keys to scroll through the list of
countries, states, and provinces. Press ENTER
when the correct location displays.
The Arrow keys are also used to move the telescope.
Initializing AutoStar
d. The next screen asks for the city (listed
alphabetically) closest to the observing site.
Use the Scroll keys to scroll through the list
of cities. Press ENTER when the correct city
appears on screen.
This section describes how to initialize AutoStar.
Perform this procedure the first time you use AutoStar
or after performing a RESET (see “RESET” page 30).
1. Verify that AutoStar is properly connected to
your telescope. See “Getting Started” page 5.
6. The next screen requests the status of Daylight
Savings Time. If Daylight Savings Time is
active, press the “1” key. If Daylight Savings
Time is not active, press the “2” key.
2. Turn the telescope power switch to the ON
position.
The AutoStar beeps and the display screen is
activated. Then AutoStar takes a few moments
to start up the system.
Note: Daylight Savings Time may be referred
to by a different name in various areas of the
world.
3. “Press 0 to Align or Mode for Menu” displays.
Press 0 to align your telescope using the “Easy
Align” method, see “Easy (Two-Star) Align” on
page 11. To skip the alignment process and
access the AutoStar menus, press the Mode
key.
7. AutoStar then asks for the Telescope Model.
Using the scroll keys (Pg. 19, Fig. 5, 7) on the
AutoStar locate the model of your telescope
and press enter.
8. Now enter the current date, then press
ENTER.
4. The telescope then tests the motor function of
the telescope by moving in the horizontal and
vertical directions.
9. Enter the current time. Select “AM,” “PM,” or
24-hour clock (blank). Then press ENTER.
5. Set Your Location or Zip Code: The Location
screen displays. This screen asks you if you
wish to choose either the zip code of your
observing location or the location (i.e., entering
the city and state or country of your observing
location). Press “1” to select the zip code option
or “2” to enter the city and state.
10. System initialization is now complete and
Autostar enters into the EasyAlignment routine.
The Autostar display now reads “North Method,
1=True 2= Compass”. See “Easy (Two-Star)
Alignment” for performing an alignment on
the night sky. If you do not wish to begin an
alignment on the night sky, press the MODE
key to exit to the main AutoStar menu.
Note:Thelocationsettings(country/state/province
and city, or zip code) are only asked for the first
time you turn on the control panel. If you wish to
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and be the brightest star in the area of the sky
where the telescope is pointing. While looking
through the red dot finder, use the Arrow Keys
to move the telescope to place the red dot
on the top of the star. Now look through the
eyepiece and use the Arrow Keys to move the
star to the center of the eyepiece field. Press
ENTER. If that area of the sky is obscured by
an object, you can prompt AutoStar to chose an
alternate star by pressing either one of the two
Scroll Keys. Repeat procedure for the second
alignment star.
Easy (Two-Star) Align
The fastest and easiest way to locate objects with
Autostar’s GO TO capabilities is to use Easy Align.
Autostar automatically picks two stars from its database
for the Easy Align procedure. During this procedure,
Autostar slews the telescope to a first alignment star.
The user is asked to verify that the telescope is pointed
at the chosen star and then prompted to center the star
in the eyepiece. The process is repeated with a second
star to complete the alignment.
Note: Before aligning the telescope, first verify
that “INITIALIZING AUTOSTAR”, page 10,
has been performed. See “Moving through
Autostar’s Menus”, page 10, for a description
of how Autostar’s keys operate.
When the procedure is performed correctly, “Alignment
Successful” displays. If Autostar does not display this
message, perform this procedure again.
Note: Autostar locates alignment stars based on the
date, time, and location entered. The alignment stars
may change from night to night. All that is required
is for the observer to center the selected stars in the
eyepiece when prompted.
How to perform the Easy Align
Procedure
If you have just powered on the telescope, follow the
procedures listed in “Initializing Autostar” on page
23. When completed, continue on to the steps below
to perform the Easy Alignment procedure. If the
telescope is already powered on and the correct site
location, date, time and telescope model have already
been entered, the Easy Alignment can be started by
selecting in the menu Setup: Align: Easy and following
the steps below.
NOTE: The GO TO key also allows you to perform
a “spiral search”. A spiral search is useful when the
telescope slews to an object, but that object is not
visible in the eyepiece after the telescope finishes its
search. (This sometimes occurs during an alignment
procedure.) Press GO TO when the slew is finished
and the telescope starts slewing in a spiral pattern at a
very slow speed around the search area. Look through
the eyepiece and when the object does become visible,
press MODE to stop the spiral search. Then use the
Arrow keys to center the object.
1. When the EasyAlignment procedure is selected
in the AutoStar’s setup menu, the display will
read “North Method: 1=True 2=Compass”.
AutoStar is asking which Home Position the
telescope will be placed in. See page 9, “The
LT Series Home Position” for a description on
placing the LT Series telescope into the home
position.
Which One’s the Alignment Star?
If you’re not familiar with objects in the night sky, how
can you be sure if the star in your eyepiece is really the
alignment star?
The rule of thumb is that an alignment star is usually
the brightest star in that area of the sky. If you perform a
GoTo to an alignment star and you’re not sure if you have
located the alignment star or it isn’t in the eyepiece, look
through your viewfinder. When you view an alignment
star in the viewfinder, it stands out dramatically from the
rest of the stars in that portion of the sky.
Note: The easiest way to set the telescope in
the home position is using the Magnetic North
method. Follow the steps on page 9 “Magnetic
North Home Position” and press the “2” key on
Autostar to select the “Compass” (Magnetic
North) method.
The viewfinder will help you locate a star more quickly
than the eyepiece. Using AutoStar, set the slew speed
to 6 (press Number key 6) or higher and use the Arrow
keys to center the alignment star in the viewfinder. If
your viewfinder has been aligned with the telescope,
the alignment star should now be in the eyepiece. Set
the slew speed to 4 or less and center the star in the
eyepiece. Also see the Spiral Search tip, page 11.
2. Star Alignment - The Autostar then chooses
two stars to align upon. When the telescope
slews to the first star for alignment, it may not
appear in the field of view in the eyepiece. The
alignment star should be easily recognized
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Go To Saturn
Using the Guided Tour
After performing the Easy Alignment procedure, the
motor drive begins operating and the telescope is
aligned for a night of viewing. Objects in the eyepiece
should maintain their position even though the Earth is
rotating beneath the stars.
This example demonstrates using “Tonight’s Best”
Guided Tour.
1. After observing Saturn, press mode twice so
that “Select Item: Object” displays again.
2. Press the Scroll Down key twice. “Select Item:
Guided Tour” displays.
Important Note: Once aligned, only use the GO TO
or Arrow keys to move the telescope. Do not move the
telescope manually, or alignment will be lost.
3. Press ENTER. “Guided Tour: Tonight’s Best”
displays. Press ENTER.
Once the telescope is aligned, you may choose and
“Go To” any object listed in AutoStar’s Object menu.
This exercise demonstrates how to select one such
celestial object, the planet Saturn, for viewing from the
Object menu.
If you wish to try out other Guided Tours, press
the Scroll Down key to scroll through other
tour choices. When the tour you wish to select
displays, press ENTER.
4. “Tonight’s Best: Searching...” displays. After
calculating, “Tonight’s Best: Jupiter” displays.
Note: Saturn is not visible the entire year and you
may need to choose another object from AutoStar’s
database; however, the procedure, as described below,
remains the same.
Note: Different objects may be displayed on a
tour list on any given night.
1 After the telescope is aligned, “Select Item:
Object” displays. Press ENTER.
Press ENTER to display information about the
object. Press GO TO to move the telescope to
the object.
2. “Object: Solar System” displays. Press
ENTER.
5. Press MODE to return to the Tour list. Press
the Scroll keys to scroll through the list. Press
ENTER when you find the next object you wish
to observe.
3. “Solar System: Mercury” displays. Keep
pressing the Scroll Down key until “Solar
System: Saturn” displays.
6. Press and hold down MODE for two seconds to
leave the Guided Tour menu.
4. Press ENTER. “Calculating” displays. Then
“Saturn” and a set of coordinates displays. Note
that Saturn’s (and other planets’) coordinates
change throughout the year.
5. Press GO TO. “Saturn: Slewing...” displays
and the telescope slews until it finds Saturn.
You may need to use the Arrow keys to center
Saturn precisely in the eyepiece. AutoStar
then automatically moves the telescope so
that it “tracks” Saturn (or whatever other object
you may have chosen); i.e., Saturn remains
centered in the eyepiece.
After you Go To Saturn, practice the Go To
feature with other objects in the Object menu
lists. For example, during Winter, choose M42,
the Orion nebula, from the Messier list. Or in
the summer, choose the Dumbbell nebula from
the Deep Sky, Named Objects list.
12
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Ƹ
ƹ
ᕥ
ᕨ
µ
ᕣ
ᕡ
ᕤ
ᕢ
ƺ
ƻ
ᕡ Diagonal Eyepiece Holder
ᕢ Diagonal Prism
µ Computer Control Panel
ᕣ 1.25” Eyepiece Holder
ᕤ Eyepiece Holder Thumb Screw
ᕥ Eyepiece
Ƹ Red Dot Finder
ƹ Red Dot Finder Alignment Screws
ƺ Handbox Storage Cradle
ᕨ Single Fork Arm Mount
ƻ AutoStar Suite Software Disc
Figure 1: LT Series Left Side
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ᕦ Diagonal Thumbscrew
ᕧ Optical Tube Assembly (OTA)
ᕩ Focus Knob
Ƹ
µ Computer Control Panel
A. Handbox (HBX) Port
B. LED
C. ON/OFF Switch
D. Auxiliary (AUX) Port
E. 12v Power Connector
¸ Dust Cover
¹ Battery Compartment
ᕧ
ᕦ
ᕩ
¹
Figure 2: LT Series Right Side
D. A. B. C. D. E.
µ
¸
Figure 4: LT Series Computer Control Panel
Figure 3: LT Series Front
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ᕡ Diagonal Holder: Holds the eyepiece in place.
¸ Dust Cover: Gently lift out the dust cover from
the front lens of the telescope. The dust cover
should be replaced after each observing session
and the power turned off to the telescope. Verify
that any dew that might have collected during
the observing session has evaporated prior to
replacing the dust cover.
ᕢ Diagonal Prism: provides a more comfortable
right angle viewing position. Slide the diagonal
prism directly into the eyepiece holder (Pg. 13,
Fig. 1, 3).
ᕣ 1.25" Eyepiece Holder
ᕤ Thumb Screw
¹ Battery Compartment: Insert eight ANSI 14A
(IEC LR14) Alkaline “C-Cell” (user-supplied)
batteries in compartment. Be sure batteries
are aligned correctly as shown in the battery
compartment.
ᕥ Eyepiece: Place the Super Plössl 26mm eyepiece
into the 90° diagonal prism (Pg. 13, Fig. 1, 2)
and tighten in place with the thumbscrews. The
eyepiece magnifies the image collected in the
optical tube.
Ƹ Red Dot Finder: Provides an easy way to sight
on objects and put them in the telescope’s
eyepiece.
ᕦ Diagonal Thumbscrew: Tightens the eyepiece
in place. Tighten to a firm feel only.
ƹ Red Dot Finder Alignment Screws: Adjust
these screws to align the Red Dot Finder with
the telescope’s main optics. See page 8 for
more information.
ᕧ Optical Tube Assembly (OTA): The main
optical component that gathers the light from
distant objects and brings this light to a focus for
examination through the eyepiece.
ƺ Handbox Storage Cradle: Holds the AutoStar
ᕨ Single Fork Arm Mount: Holds the optical tube
handbox in
a
convenient position on the
in place and moves it to find and track objects.
telescope.
ᕩ Focus Knob: Moves the telescope’s primary
mirror in a finely-controlled motion to achieve
precise image focus. The LT Series telescope
can be focused on objects from a distance of
about 25 ft. to infinity. Rotate the focus knob
counterclockwise to focus on distant objects, and
clockwise to focus on nearby objects.
ƻ AutoStar Suite Software: Contains the LT Series
Instruction Manual and a collection of useful
software including a planetarium program, the
AutoStar Updater for downloading and upgrading
the firmware in the telescope, software to control
the telescope from a computer and other programs
all designed to enhance your use of the LT Series
system.
µ Computer Control Panel
A. Handbox (HBX) Port: Plug the AutoStar coil
cord (Pg 19, Fig. 5, 10) into this port.
B. LED: The red power indicator light illuminates
when power is applied to the telescope.
C. ON/OFF Switch: Turns the Computer Control
Panel and AutoStar ON or OFF
D. Auxiliary (AUX) Port (2): Provides connection
for Meade accessories. See OPTIONAL
ACCESSORIES, page 16.
E. 12v Power Connector: Provides connection so
that the telescope assembly may be powered
from either a 12v DC auto cigarette light plug
or from a standard 115v AC home outlet.
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OPTIONAL ACCESSORIES
Meade makes a complete line of accessories to
enable you to get the most fun and performance from
your LT Series telescope. No matter what you want to
accomplish, we have the equipment to help you get
there.
26mm eyepiece, which gives a wide 53 ARC Minute
(just a little less than 1 degree) field of view with 59x
magnification. This is a very good all purpose eyepiece
for your telescope, but you should consider buying
additional eyepieces in longer and shorter focal lengths
to fully realize the potential of the excellent 6" optical
system in your LT Series telescope.
Choosing Eyepieces
A telescope’s eyepiece magnifies 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 magnification. For
example, an eyepiece with a focal length of 9mm has
a higher magnification than an eyepiece with a focal
length of 26mm. Experienced users know that higher
powers are, in general, not as useful as lower powers.
Many of the objects in the night sky are relatively large
and faint and look best at low magnifications.
Thepowerormagnificationofatelescopeisdetermined
by the focal length of the telescope and the focal length
of the eyepiece being used. To calculate magnification,
divide the telescope’s focal length by the eyepiece’s
focal length. For example, a 26mm eyepiece is supplied
with the LT Series. The focal length of the 6" LT Series
is 1524mm (see SPECIFICATIONS, page 47).
Telescope Focal Length 1524mm
Eyepiece Focal Length 26mm
1524 ÷ 26 = 58.6x
TheSeries4000SuperPlösslEyepiecesareexcellent
well corrected 4 element optics at popular prices. They
come in a wide range of focal lengths to give you the
right magnification for any type of celestial object you
are viewing. You can also use one of the Series 4000
Barlows to double or triple the magnification of a Super
Plössl eyepiece. These eyepieces have been the
standard for over 30 years.
The magnification is therefore 58.6x.
Low power eyepieces offer a wider field of view, bright,
high-contrast images, and long eye relief. To find an
object with a telescope, always start with a lower power
eyepiece such as the Super Plössl 26mm or longer
focal length. 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 or, for many
objects, the view is best with a high quality low-power
wide-field eyepiece.
Series 4000 Super Plössl Eyepieces
Focal
Length
Apparent
Field
Actual
Field
Type
Power
56.0mm
40.0mm
32.0mm
26.0mm
20.0mm
15.0mm
12.4mm
9.7mm
SP 2"
SP
SP
SP
SP
SP
SP
SP
SP
52º
44º
52º
52º
52º
52º
52º
52º
52º
27x
38x
1º 55'
1º 9'
1º 6'
53'
48x
NOTE: Seeing conditions vary widely from night-to-
night and site-to-site. Turbulence in the air, even on
an apparently clear night, can distort images. If an
image appears fuzzy and ill-defined, reduce to a lower
power eyepiece.
59x
76x
41'
102x
123x
157x
238x
31'
25'
20'
Your telescope comes supplied with a Super Plössl
6.4mm
13'
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The Series 5000 Premium Eyepieces represent
the highest level of eyepiece technology. Featuring
advanced lens designs with 5, 6 and 7 elements,
super fully multi-coated lenses and some of the
widest fields of view available, they provide the user
with the highest-contrast, pinpoint-sharp images and
spectacular wide field views of the heavens. They are
made to the same high quality standards as the primary
optics in your LT Series telescope and allow you to get
all the performance that the Advanced Coma-Free and
Schmidt-Cassegrain optical systems were designed
to deliver. Use a Series 5000 Telextender for 2, 3
or 5 times the magnification of the eyepiece alone.
There is even a 2x 2 inch Telextender for the large 2
inch eyepieces.
Series 5000 Ultra Wide Angle
NOTE: 2 inch eyepieces require the optional Series
5000 2” Enhanced Diagonal with 99% Reflectivity
(product number 07677) and the SC Thread to 2"
Accessory Adapter (product number 07085).
Series 5000 Plössl
Series 5000 Eyepieces
Focal
Length
Apparent
Field
Actual
Field
Type
Power
40.0mm 5 EP 2"
32.0mm 5 EP 2"
60º
60º
60º
60º
60º
60º
60º
38x
48x
1º 34'
1º 16'
1º 1'
47'
26.0mm
20.0mm
14.0mm
9.0mm
5 EP
5 EP
5 EP
5 EP
5 EP
59x
76x
109x
169x
277x
33'
21'
5.5mm
13'
Series 5000 Super Wide Angle
40.0mm SWA 2"
32.0mm SWA 2"
26.0mm SWA 2"
68º
68º
68º
68º
68º
68º
38x
45x
54x
64x
76x
95x
1º 47'
1º 31'
1º 15'
4'
20.0mm
15.0mm
12.4mm
SWA
SWA
SWA
54'
43'
30.0mm UWA 2"
24.0mm UWA 2"
82º
82º
82º
82º
82º
82º
82º
51x
64x
1º 37'
1º 17'
58'
18.0mm
14.0mm
8.8mm
6.7mm
4.7mm
UWA
UWA
UWA
UWA
UWA
85x
Series 5000 2” Enhanced Diagonal
109x
173x
227x
324x
45'
28'
22'
15'
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Imagers and Accessories
Power Supplies
While the LT Series will operate with 8 “C” cell batteries,
you should consider several other power options
that might work better for your situation and save
you money.
Deep Sky Imagers (DSI)
Universal AC Adapter (07584): This adapter supplies
a constant regulated 12 volt DC at up to 5 Amps from
either a standard 115 volt AC or 220 volt AC household
supply. It is the only tested and recommended AC
power supply for the LT Series system.
Camera Adapters
#607 DC Power Cord w/ Cigarette Lighter Adapter
(07043): This adapter allows you to plug into a standard
automobile 12v DC power socket. It comes with a 25
foot cord so you can setup far from the car.
#505 Connector Cable Set. For all AutoStar
#497 Telescopes. Allows you to connect your LT
Telescope to a PC serial port. Operate your computer
from your PC, download updates, create custom tours
and more.
Off Axis Guiders
Focal Reducers
USB to Serial Bridge Cable. Allows you to use
#505 or #506 cables above to connect to a USB port.
Driver software included. Windows 98, ME, 2000, and
XP compatible.
Accessories at Meade.com. Now you can order all
these and more accessories or any Meade products
it will be shipped right to your door.
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¹
ᕡ 2-Line LCD Display
ᕢ ENTER Key
ᕣ MODE Key
ᕤ “GO TO” Key
ᕥ Arrow Keys
ᕦ Number Keys
ᕧ Scroll Keys
ᕨ “? Key
ᕡ
¿
·
´
»
º
ᕩ Coil Cord Port
µ Coil Cord
²
¸ RS-232 Port
¹ Utility Light
¾
¶
µ
¸
Figure 5: The AutoStar #497 Handbox
Tour the Cosmos with Just the
Push of a Button
Control of the LT Series is through the operation of the
standard-equipment AutoStar. Nearly all functions of
the telescope are accomplished with just a few pushes
of AutoStar’s buttons. Some of the major features of
AutoStar are:
•
Control your LT Series with your PC using an
serial interface.
•
•
Access a glossary of astronomical terms.
Calculate which eyepiece to use for optimum
viewing of a celestial object.
•
Automatically move the telescope to any of
over 30,000 objects stored in the database or
manually enter the astronomical coordinates of
any celestial object.
•
Mount the telescope in the “Alt/Az” mode
(Altitude - Azimuth, or vertical - horizontal) for
fully automatic tracking of celestial objects.
•
•
Take a guided tour of the best celestial objects
to view on any given night of the year.
Download the latest satellite data and software
revisions directly from the Meade website (www.
meade.com) and share software with other
AutoStar enthusiasts.
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The AutoStar Computer Controller provides control
of virtually every telescope function within a compact
handbox. AutoStar has soft-touch keys designed to
have a positive feel. The LCD (Liquid Crystal Display)
is backlit with a red LED (Light Emitting Diode) for
easy viewing in the dark. The backlit display, key
arrangement, and sequential database make AutoStar
extremely user friendly.
•
•
•
•
•
Date
Site coordinates
Local Time and Local Sidereal Time (LST)
Timer and Alarm Status
Battery status
Press MODE again to return to the previous menu.
ᕡ
2-Line LCD Display: Provides an interface
between AutoStar and the telescope.
ᕤ
GO TO Key: Slews (moves) the telescope to the
coordinates of the currently selected object. While
the telescope is slewing, the operation may be
aborted at any time by pressing any key except
GO TO. Pressing GO TO again resumes the slew
to the object.
•
Top line: Lists the primary category or menu
item.
•
Bottom line: Contains a menu option or information
about an object or subject, depending on which
function is being performed.
ᕥ
Arrow Keys: Slew the telescope in a specific
direction (up, down, left, and right), at any one
of nine different speeds. Speed selection is
explained in “SLEW SPEEDS”, below. The
following functions are also available with the
Arrow keys:
ᕢ
ENTERKey:Accesses,inasequentialmanner,the
next menu or data level in the AutoStar database.
See MOVING THROUGHAUTOSTAR’S MENUS,
page 10.
NOTE: If ENTER is pressed for two seconds or
more and then released, AutoStar emits a beep
and “ENTER to Sync” is displayed. “ENTER to
Sync” is relevant only after the telescope has
been aligned and is pointing at an object. If the
“ENTER to Sync” feature is accessed by mistake,
press MODE to return to the previous screen. See
High Precision, page 29, for more details about
this feature.
•
Moves the telescope – Use the Up and
Down Arrow keys to move the telescope
vertically up and down. The Left Arrow key
rotates
the
telescope
horizontally
counterclockwise, while the Right Arrow key
rotates it clockwise.
•
Data entry – When the scope is prompting
for user entered data, use the Up and Down
Arrow keys to scroll through the letters of the
alphabet and numerical digits. The Down
Arrow key starts with the letter “A” and the
Up Arrow key starts with the digit “9.” The
Left and Right Arrow keys are used to
move the blinking cursor left and right across
ᕣ
MODE Key: Returns to the previous menu or data
level in the AutoStar database until the top level,
“Select Item” is reached. The MODE key is similar
to the ESCAPE key on a computer.
the LCD display.
ᕦ
Number Keys: Input digits 0 - 9 and changes the
slew speeds (see Slew Speeds, see below). The
“0” key also turns on and off the red utility light on
the top of the handbox.
Note: Pressing MODE while in the “Select Item”
level moves AutoStar to the topmost screen:
“Select Item: Object”.
If MODE is pressed and held for two seconds or
more, information about the telescope’s status
displays. When the status displays, press one of
the Scroll keys (Pg. 19, Fig. 5, 7) to display the
following information:
Slew Speeds
LTSeries has nine slew speeds that are directly
proportional to the sidereal rate (the rate at
which stars appear to drift across the sky)
and have been calculated to accomplish
specific functions. Pressing a Number key
changes the slew speed, which is shown for
about two seconds on AutoStar’s display.
•
•
Right Ascension and Declination (astronomical)
coordinates
Altitude (vertical) and Azimuth (horizontal)
coordinates
To
change
the
speed,
press
the
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appropriate key shown below.
Nine available speeds are:
essentially an on-screen instruction manual.
If you have a question about an AutoStar
operation, e.g., INITIALIZATION, ALIGNMENT,
etc., hold down the ? key and follow the directions
that scroll on the second line of the LCD screen.
When a word appears in [brackets], press ENTER
to access the AutoStar Glossary. A definition or
more detailed information is displayed. Press
MODE to return to the scrolling AutoStar Help
display.
Number Key “1” = 1x (Guide)
Number Key “2” = 2x
Number Key “3” = 8x
Number Key “4” = 16x
Number Key “5” = 64x
Number Key “6” = 0.50°/sec
Number Key “7” = 1.0°/sec
Number Key “8” = 1.5°/sec
Number Key “9” = 4.0°/sec (Max)
When satisfied with the Help provided, press
MODE to return to the original screen and continue
with the chosen procedure.
Speeds “1”,“2”, or “3” Best used for fine
centering of an object in the field of view of
a higher power eyepiece, such as a 12mm or
a 9mm eyepiece.
ᕩ
µ
Coil Cord Port: Plug one end of the AutoStar coil
cord into this port (pg. 19, Fig. 5, 9) located at the
bottom of the AutoStar handbox.
Coil Cord: Plug one end of the AutoStar coil
cord into the HBX port (Pg. 14, Fig. 4, 10A) of the
computer control panel of the telescope and the
other end into the coil cord port.
Speeds “4”, “5”, or “6”: Enables centering
an object in the field of a low-to-moderate
power eyepiece, such as the standard Super
Plössl 26mm.
¸
¹
Serial Port: plug an serial accessory (#505)
cable into AutoStar for updating functions such
as “Download” or “Clone”. See page 29 for
more details.
Speeds “7” or “8”: Best used for rough
centering of an object in the Red Dot
Viewfinder.
Speed “9”: Moves the telescope quickly from
Utility Light: Use this built-in red light to illuminate
star charts and accessories without disturbing
your eye’s adaptation to darkness.
one point in the sky to another.
ᕧ
Scroll Keys: Accesses options within a selected
menu. The menu is displayed on the first line of
the screen. Options within the menu are displayed,
one at a time, on the second line. Press the Scroll
keys to move through the options. Press and hold
a Scroll key to move quickly through the options.
Observing Using AutoStar’s Arrow
Keys
You may observe land and astronomical objects using
AutoStar’s Arrow keys to move the telescope.
The Scroll keys also scroll through the letters of
the alphabet and numerical digits.
1. Verify the telescope is fully assembled and
that AutoStar is properly connected to your
telescope. See Getting Started on page 5.
Note: The Scroll Down key and the Down Arrow key
move forward through the alphabet & digits (A to
Z, 0 to 9). The Scroll Up key and the Up Arrow key
move backward (Z to A, 9 to 0). Common symbols
are also available in the list.
2. Flip the telescope power switch to the ON
position. The AutoStar screen is activated and
a copyright message displays briefly, followed
by a short beep. Then AutoStar takes a few
moments to start up the system. “Press 0 to
align or Mode for Menu” displays (if you select
“0”, Alignment will begin).
ᕨ
? Key: Accesses the “Help” file. “Help” provides
on-screen information on how to accomplish
whatever task is currently active.
Hold down the ? key and then follow the prompts
on the display to access details of AutoStar
functions in the Help feature. The Help system is
3. The Arrow keys are now activated. Press the
Arrow keys (Pg. 19, Fig. 5, 5) to slew (move)
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the telescope up, down, right, or left.
If you wish to observe a distant land object, such as a
mountain top or a bird, you want to use your telescope
in its Terrestrial Observing mode. To start up the
telescope in Terrestrial mode:
4. Press a Number key (Pg. 19, Fig. 5, 6) to
change the telescope’s slew speed. See Slew
Speeds, on pg 20 for more information.
1. Turn on the telescope.
5. Use the viewfinder (Pg. 13, Fig. 1, 13) to locate
an object and practice using the AutoStar’s
Arrowkeystocentertheobjectinthetelescope’s
field of view.
2. Move your telescope using the direction arrows
on the handbox while looking through the Red-
Dot Finder to put your target in the eyepiece.
6. Use the telescope’s focus knob (Pg. 14,
Fig. 2, 9) to bring the object into focus.
3. Focus on the target with the focus knob (pg. 14,
Fig. 2, 9).
Observe the Moon
Point your telescope at the Moon (note that the Moon
is not visible every night) and practice using the Arrow
keys and the slew speeds to view different features.
The Moon contains many interesting features, including
craters, mountain ranges, and fault lines. The best time
to view the Moon is during its crescent or half phase.
Sunlight strikes the Moon at an angle during these
periods and adds a depth to the view. No shadows
are seen during a full Moon, causing the overly bright
surfacetoappearflatandratheruninteresting. Consider
the use of a neutral density Moon filter when observing
the Moon. Not only does it cut down the Moon’s bright
glare, but it also enhances contrast, providing a more
dramatic image.
LT Series TIPS
Observing Considerations
•
Try to pick an observing site away from street
and house lights and car headlights. While
this is not always possible, the darker the site,
the better.
• Try not to use
a
standard flashlight.
Experienced observers use red LED
flashlights, the red utility light on the AutoStar
#497 handbox, or tape red cellophane over
their flashlights to use for setup and map
reading so they don’t have to continually
readjust their eyes to the darkness. Be
careful not to shine bright lights if there are
other observers in the area. Do not shine a
flashlight into the telescope while someone is
observing!
Terrestrial Observing
The LT Series is 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.
•
•
Dress warmly. It gets chilly when you’re sitting
for prolonged periods.
Practice setting up your equipment during the
day or in a lighted area to become familiar
with it before going to a dark site.
•
Use your 26mm eyepiece to view terrestrial
objects and wider areas of space, such as
open star clusters. Use optional higher power
eyepieces, such as a 9mm eyepiece, when
you wish to view something up close, such as
craters on the Moon or the rings of Saturn.
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AutoStar Operation
Important Note: No matter how many levels into
AutoStar are traveled, each press of the MODE
key moves up a level, until the top level, “Select
Item”, is reached. Once in the Select Item level,
press MODE to return to the topmost level,
“Select Item: Object”.
AutoStar Navigation Exercise
To demonstrate how the AutoStar menu structure
works, the following exercise calculates Sunset time
so an evening observing session can be planned.
To Calculate Sunset time:
1. Press the MODE key several times, until “Select
Item: Object” is displayed.
Fig. 8: The AutoStar Universe: The six primary cate-
gories listed in the Select Item menu of AutoStar.
2. Press the Scroll Down key once to display the
“Event” option in the “Select Item” menu.
3. Press the ENTER key to choose the “Event”
option and move down a level. “Event: Sunrise”
is displayed.
It is important to understand that menu selections are
set in a loop (Fig. 10). This means that pressing the
Scroll Down key (Pg. 19, Fig. 5, 7) cycles down through
all the available options within a given category, then
returns to the first option. The Scroll Up key (Pg. 19,
Fig. 5, 7) cycles up through the options in the opposite
order. Note that this capability is a quick way to get
to an option that is near the bottom of the list. The
following example demonstrates this capability.
4. Press the Scroll Down key once to display the
“Sunset” option in the Event menu.
5. Press the ENTER key to choose the “Sunset”
option and move down another level.
6. AutoStar calculates the Sunset time based on
the current date, time, and location. AutoStar
then displays the results of the calculation.
Example:
7. Press MODE once to start moving back up
through the AutoStar levels. The first level up
is the Event menu.
To navigate to the “Select Item: Setup” menu option
when the “Select Item: Object” menu is displayed:
1. Press the Scroll Down key four times or the
Scroll Up key once.
8. Press MODE again to move up another level.
This is the top level, “Select Item”.
The screen in Fig. 9º displays two lines of information.
The top line shows the current menu level. The second
line displays an option which may be selected within
that menu level. Some options are choices that select
the next menu level down. The Scroll keys move up
and down within the list of available options, showing
one option at a time.
9. Press MODE again to return to the starting
point of “Select Item: Object”.
When the desired option is displayed on the second
line, press the ENTER key to choose that option and
move down one menu level.
Figure 9: AutoStar Levels
Press the MODE key to leave a level; e.g., the wrong
menu option is chosen.
Figure 10: Menus set in
loop
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object in the eyepiece of the telescope for you to view.
The telescope comes pre-loaded with:
Entering Data into AutoStar
• To enter numbers and text:
a) Use the Number keys, or
•
“Tonight’s Best”, a selection of the most
interesting objects visible on any night.
b) Use the Arrow keys to scroll through numbers
0 - 9 and the alphabet. The Down Arrow key
begins with the letter “A”; the Up Arrow key
begins with digit “9”.
•
“A Star’s Life”, tours how stars are formed,
created, changes through their lives and finally
die using examples that are visible tonight.
•
“How Far is Far”, tour showing the phenomenal
• To move the cursor across the display: Use
the Right or Left Arrow key (Pg. 19, Fig. 5, 5) to
move the cursor from one number to the next in
the display
distances you can see with your LT Series.
AutoStar Suite also allows you to create your own
guided tours of the skies, including your own objects
and titles (for complete instructions on how to use the
authoring tools please refer to the reference manual
included on the AutoStar Suite DVD).
• Press ENTER when the desired information
has been entered.
Navigating AutoStar
Object Menu
AutoStar’s menus are organized for quick and
easy navigation:
Almost all observing with LT Series is performed using
the Object menu category. (NOTE: Exceptions include
Guided Tour and Landmarks).
• Press ENTER to go deeper into AutoStar’s
menu levels.
Many LT Series menu categories contain databases.
An LT Series database is a list of objects, such as stars,
planets, comets, nebulae and so forth. When one of
these objects is selected from a database by pressing
“ENTER” and then “GO TO”, LT Series moves your
telescope (when properly aligned) and points it at the
selected object.
• Press MODE (Pg. 19, Fig. 5, 3) to move back
toward the top menu level.
• Press the Scroll keys to move up and down
through the options or lists.
• Press theArrow keys to move the cursor across
the display.
• Press the Help (?) key to access on-line help.
The Object Menu options include:
When multiple choices are available within a menu
option, the option that is currently selected is usually
displayed first and highlighted by a right pointing
arrow (>).
Solar System is a database of the eight planets (Earth
is not included) in ascending orbits from the Sun,
followed by the Moon, asteroids, and comets.
Constellation is a database of all 88 Northern and
Southern Hemisphere constellations. When this menu
option is chosen and a constellation name appears
on the first line of the screen, press GO TO once to
change the second line to the name of the brightest
star in the constellation.
Guided Tour Menu
When Guided Tours is selected, LT Series shows you
a list of theme tours that will help you explore the night
sky. These tours are pre programmed presentations of
objects that are visible for the user’s particular location,
time and date.
Press GO TO a second time to slew the telescope to
that star. Use the Scroll keys to cycle through the list of
stars in the constellation, from brightest to dimmest.
The most popular tour is “Tonight’s Best” that guides
the user to the best objects that are currently up
in the night sky. This tour is the easiest way to get
started exploring the cosmos with your new LT Series
telescope.
Deep Sky is a database of objects outside our Solar
System such as nebulae, star clusters, galaxies, and
quasars grouped in various catalogs like Messier,
Caldwell and NGC.
Each tour will select the objects, present information
about the object and, if you press “GoTo”, put that
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AutoStar #497 MENU TREE
Figure 11: The AutoStar #497 Menu Tree
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Star is a database of stars listed in different categories
keep pressing MODE until the “Select Item: Object”
menu is displayed. Press ENTER to select this menu.
such as named, double, variable, or nearby.
Important Note: When you are looking at descriptive
object text, pressing “ENTER” will synchronize the
telescope’s coordinates with the object. This is most
useful when synching on bright stars to achieve better
pointing in the vicinity of the star.
2. Scroll through the Object menu options until the
“Object: Identify” screen appears.
3. Press ENTER. AutoStar searches the database for
the identity of the object being observed.
User Objects allows the user to define and store in
memory deep-sky objects of specific interest that are
not currently in the LT Series database. See page 38
for more information (for complete instructions on how
to use the authoring tools please refer to the reference
manual included on the AutoStar Suite DVD).
4. If the telescope is not directly on an AutoStar
database object, the nearest database object is located
and displayed on the screen. Press GO TO and the
telescope slews to that object.
Browse allows you to search the database for objects
with certain parameters, much like a search engine.
“Edit Parameters” lets you set various parameters for
the search, such as: Object Type, Minimum Elevation,
Largest, etc. Once you have set the parameters of
the search, select “Start Search” and press ENTER.
AutoStar will display the results of the search. See
page 40 for more information.
Satellite is a database of Earth-orbiting objects such
as the International Space Station (ISS), the Hubble
Space Telescope (HST), Global Positioning System
(GPS) satellites, and geosynchronous orbit satellites.
In order to find and track satellites, you must download
recent orbital data into the telescope.
Landmarks stores the location of terrestrial points of
interest that you create in the permanent LT Series
database.
Event Menu
The Event menu provides access to dates and times of
astronomical events. The Event database includes:
IMPORTANT NOTE: To use the Landmark function,
the telescope must be located and aligned exactly as
when the landmark was added to the database.
Sunrise and Sunset calculates the time that the Sun
rises or sets on the current date.
•
Select – To select a Landmark already in the
database (see ADD below), choose the “Select”
option and scroll through the list. Press “ENTER”
to select a Landmark,then press“GOTO”andthe
telescope slews to the object.
Moonrise and Moonset calculates the time that the
Moon rises or sets on the current date.
Moon Phases displays the date and time of the next
New, 1st Quarter, Full and 3rd Quarter Moon.
• Add – To add a Landmark, choose the “Add”
option. Enter a name for the Landmark. Locate
and center the Landmark in the eyepiece, then
press “ENTER”.
Meteor Showers provides information on upcoming
meteor showers, such as the Perseids, the Leonids,
etc. Also lists the dates of the showers and when they
reach maximum.
NOTE: Meteors are fast moving objects that cover
large areas of the sky and are usually best observed
with the naked eye.
Identify is an exciting feature for an observer who
wants to scan the night sky and start exploring. After
the telescope has been properly aligned, use the
AutoStar Arrow keys to move about in the sky. Then
follow this procedure:
Solar Eclipse lists upcoming Solar Eclipses, including
the date and type (total, annular, or partial) of eclipse,
and the location and time of the first and last contacts
of the Moon’s shadow. Use the Scroll Up and Down
keys to display the available data. Remember, never
use a telescope to look at the Sun!
Important Note: Only use the Arrow keys to move the
telescope during the Identify procedure. Do not move
the telescope manually or the alignment will be lost.
Lunar Eclipse lists upcoming Lunar Eclipses,
1. When a desired object is visible in the eyepiece,
including the date and type (total, partial, penumbral)
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of eclipse. Use the Scroll Up and Down keys to display
the available data.
• Start/Stop: Activates the timer set previously.
Use the Scroll keys to toggle between ON and
OFF. When ON is displayed, press ENTER to
activate the timer. When the timer runs out, four
beeps sound and the timer is deactivated.
Min. (Minimum) of Algol is the minimum brightness
of the dramatic eclipsing binary star system, Algol. It is
relatively close at a distance of 100 light years. Every
2.8 days during a 10 hour period, Algol undergoes a
major change in apparent magnitude as one of the
two stars passes behind the other. The combined
magnitude of the two stars thus dips from +2.1 to a
minimum of +3.4 halfway through the eclipse as the
second star is hidden. LT Series calculates minimum
magnitude time at mid-eclipse.
Alarm selects a time for an alarm signal as a reminder.
To use the Alarm, press ENTER, then choose “Set” or
“Start/Stop”.
• Set: Enter the time of day for the alarm to
sound, in hours, minutes, and seconds, then
press ENTER.
• Start/Stop: Activates the alarm set previously.
Use the Scroll keys to toggle between ON and
OFF. When ON is displayed, press ENTER to
activate the alarm. When the alarm time arrives,
AutoStar beeps. Press ENTER to deactivate
the alarm.
Autumn and Vernal Equinox calculates the time and
date of the fall or spring equinox of the current year.
Winter and Summer Solstice calculates the time
and date of the winter or summer solstice of the
current year.
Eyepiece Calc calculates information about an
eyepiece for the specific telescope to which AutoStar
is connected.
Glossary Menu
The Glossary menu provides an alphabetical listing of
definitions and descriptions for common astronomical
terms and AutoStar functions. Access directly through
the Glossary menu or through hypertext words
embedded in AutoStar. A hypertext word is any word
in [brackets], usually found when using the AutoStar
Help function or when reading a scrolling message
such as a description of a planet or star. Press ENTER
whenever a hypertext word is on screen and AutoStar
goes to the glossary entry for that word.
• Field of View: Scroll through a list of available
eyepieces. When an eyepiece is selected, the
field of view is calculated.
• Magnification: Scroll through a list of available
eyepieces. When an eyepiece is selected, the
magnification is calculated.
• Suggest: AutoStar calculates and suggests
the best eyepiece for viewing, based on the
telescope and the object being viewed.
To access directly from the Glossary menu, use the
Scroll keys to scroll through the alphabet. Press
ENTER on the desired letter. Scroll to the desired entry
and then press ENTER to read the description.
Brightness Adj adjusts the brightness of the display
using the Scroll keys. When complete, press ENTER.
Contrast Adj adjusts the contrast of the display using
Utilities Menu
the Scroll keys. When complete, press ENTER.
The Utilities menu provides access to several extra
features within AutoStar, including a countdown timer
and an alarm. The Utilities functions include:
Note: This feature is usually only required in very cold
weather.
Landmark Survey automatically slews the telescope
to all user-defined landmarks with a short pause at
each location. Press ENTER to start the survey. While
a slew is in progress, press any key to skip that object
and go to the next landmark on the list. To observe
a landmark for a longer period, press MODE when
paused on the object to stop the survey. Press ENTER
to restart the survey at the first object on the list. See
Landmarks, page 37.
Timer selects a countdown timer. This feature is useful
for functions such as astrophotography and tracking
satellites. See OBSERVING Satellites, page 32. To
use the Timer, press ENTER, then choose “Set” or
“Start/Stop.”
• Set:Enterthetimetobecounteddown, inhours,
minutes, and seconds, then press ENTER.
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Sleep Scope is a power saving option that shuts
down AutoStar and the telescope without forgetting its
alignment. With “Sleep Scope” selected, press ENTER
to activate the Sleep function. AutoStar goes dark, but
the internal clock keeps running. Press any key, except
ENTER, to re-activate AutoStar and the telescope.
Telescope accesses the several options, including:
• Model: Allows you to select the telescope
model connected to AutoStar.
• Focal Length: Displays the focal length of the
selected telescope.
• Az Ratio and Alt Ratio: The Az (Azimuth)
ratio and Alt (Altitude) ratio refers to the gears
of the telescope’s motors. Do not alter these
numbers.
ParkScopeisdesignedforatelescopethatisnotmoved
between observing sessions. Align the telescope one
time, then use this function to park the telescope. Next
time it is powered up, enter the correct date and time –
no alignment is required. Pressing ENTER causes the
telescope to move to its pre-determined Park position.
Once parked, the screen prompts to turn off power.
• Az Percent: The Az (Azimuth) Percent allows
you to change the azimuth backlash, i.e., the
way the Arrow keys move the telescope along
the azimuth (horizontal) axis. If you enter a
value near 100, the telescope tube responds
more quickly (it responds immediately at 100%)
as you hold down an Arrow key and also slews
(moves) the tube more quickly. If you enter
a value near 0, it takes longer for the tube to
respond as you hold down an Arrow key and
also slews the tube more slowly. Experiment
with this option. Try changing the percent value
until you get a “feel” for the Arrow keys that is
comfortable for you.
Important Note: When the “Park Scope” option is
chosen and the display prompts you to turn off the
telescope’s power, AutoStar is unable to be returned to
operation without turning the power off and then back
on.
Cord Wrap, when set to “On”, moves the telescope in
such a way as to prevent the cords and cables attached
to your telescope assembly from getting wound around
the assembly and tangled as the telescope slews to
objects. “Off” is the default setting.
• Alt Percent: TheAlt (Altitude) Percent operates
identical to the Az Percent option (see above),
but allows you to change the altitude backlash,
i.e., the way theArrow keys move the telescope
when moving along the altitude (vertical) axis.
Setup Menu
The Setup menu’s primary function is to align the
telescope. However, there are numerous other features
available within the Setup menu, including:
• Train Drive: Trains the Altitude and Azimuth
Date changes the date used by AutoStar. This function
is useful to check events in the past or future. For
example, set the Date menu for a day three months in
the future. Then check the “Select Item: Event” menu
for the Sunset time on that date. See EVENT MENU,
page 26.
motors to locate objects with more precision.
If you are experiencing any problems with
pointing accuracy, follow the procedure
described in APPENDIX A: TRAINING THE
DRIVE, page 44, to insure accurate pointing
and tracking.
Time changes the time entered into AutoStar. Setting
the correct time is critical for AutoStar to properly
calculate locations and events. Time may be set to
24-hour mode (military time) by selecting the “blank”
option which follows the “AM” and “PM” options.
• Tracking Rate: Changes the speed at which
the telescope tracks targets in the sky.
a. Sidereal: The default setting for AutoStar;
sidereal rate is the standard rate at which stars
move from East to West across the sky due to
the rotation of the Earth.
Daylight Saving is used to enable or disable Daylight
Savings time.
Note: Daylight Savings Time may be referred to by
different names in various areas of the world. Check
local time to verify.
b. Lunar: Choose this option to properly track the
Moon over long observing sessions.
c. Custom: Allows entry of user-defined tracking
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rates.
you observe will remain centered in the eyepiece.
If “Terrestrial” is selected, the tracking motor is
turned off..
• Reverse L/R reverses the functions of the Left
and Right Arrow keys (i.e., the Right key moves
the telescope to the left).
Site provides access to several options including:
• Reverse UP/DOWN reverses the functions of
the Up and Down Arrow keys (i.e., the Up key
moves the telescope down).
• Select: Displays the currently selected
observing site. Use the Scroll keys to cycle
through all available sites (see Add below).
Press ENTER when the site you wish to select
displays. Use this option when you move to a
different geographic location.
• Quiet Slew sets the maximum slew rate to 1.5°
for quieter operation.
• Max Elevation allows you to enter a value in
degrees that sets a limit as to how far the optical
tube can swing upward during a programmed
slew. (Note that it does not prevent you from
performing a manual slew past this limit.) This
is useful when you have a camera or other
peripheral attached to the telescope—you can
prevent it from striking the telescope base.
• Add: Allows you to add new observing sites to
the database (up to six sites may be stored).
Scroll through the list of Countries/States.
Press ENTER when the site you wish to add
displays. Then choose the desired city in the
same manner.
• Delete: Deletes
the database.
a
stored site from
• Min AOS (Acquisition of Signal) allows you
enter a value in degrees. This value represents
the altitude at which your telescope begins
to slew when acquiring a satellite track. This
is useful when you are observing satellites,
but a tall tree or building is obstructing the
telescope. For example, you might begin to
track the satellite at 15° altitude, instead of 5°.
See Observing Satellites, page 32, for more
information about satellites.
• Edit: Edits a selected site, including: the name,
latitude, longitude, and time zone. Time Zone
refers to the Greenwich Mean Time (GMT) time
zone shift. Users West of Greenwich, England
use “-” hours, East of Greenwich use “+” hours.
For the United States, look up the time zone
shift in the table at left.
AutoStar compensates for daylight savings
time, if selected. See Setup Menu: Daylight
Saving, page 28.
• Calibrate Motor if the telescope motors appear
to have a problem, use this option to retest
the motors before performing a Reset. This
option is also used if an AutoStar unit is moved
between telescopes, to match AutoStar to the
new telescope. To calibrate the motors, select
this option and press ENTER.
Owner Info accesses the owner information menu,
including:
• Name: Users may enter both their first and last
names using the Up and Down Arrow keys to
cycle through the alphabet. Use the Right and
Left Arrow keys to move through the text. Press
ENTER when the entry is complete.
• High Precision if turned on, when looking for
a faint celestial object (i.e., a nebula or galaxy),
AutoStar first slews to a nearby bright star and
displays “ENTER to Sync”. Center the star in
the eyepiece, then press ENTER. At that point
the telescope has a high precision alignment
to that part of the sky and it then slews to the
object that was originally requested.
• Address: Use the Up and Down Arrow keys
to enter your street address, city, state, and
zip code. Press ENTER when the entry is
complete.
Download transfers information from anotherAutoStar
during cloning (see below). During the operation, the
warning “Downloading Do Not Turn Off” appears.
Targets switches between Astronomical targets and
Terrestrial targets. If “Astronomical” is selected, the
telescope tracking motor is activated and any object
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Note: The Download function requires the optional
#505 Astrofinder Software and Cable Connector Kit.
See the instruction sheet included with the kit for more
information on how to download. Also see OPTIONAL
ACCESSORIES, page 16.
Clone uploads information from one AutoStar handbox
to another. Three options are available:
• Catalogs: Sends only user-defined object
information, such as new satellite orbits or
comet data to another AutoStar handbox.
• Software: Sends only the basic AutoStar
software. This is useful if one user has
downloaded a new version ofAutoStar software
wants to pass this software along to friends.
• All: Everything – user-defined information
and AutoStar software
another AutoStar.
–
is sent to
Statistics provides basic statistical data about
AutoStar, including:
• Characters Free: Shows how much room is
available in user-defined object memory.
• Version: Shows the current version of the
AutoStar software.
Reset completely resetsAutoStar. Most values entered
into the menus revert to factory defaults.
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Advanced AutoStar Features
press ENTER so that the site is added to your
Adding Observing Sites
observing sites list. Choosing a site already
on the list (as opposed to using the “Custom”
feature) makes it easier to edit, as the “Time
Zone” value may not need to be changed.
If you plan to observe using AutoStar at different
geographic locations, you can store up to six
observation sites in AutoStar’s memory to help simplify
your telescope setup. Perform these procedures using
the Site options (Add, Select, Delete, Edit) of the
Setup menu.
2. Scroll to “Site: Edit” and press ENTER. “Edit:
Name” displays. Press ENTER.
3. The name of the site you have just entered
to your list displays; if it does not, scroll to
the site.
To Add a Site to the user-defined site
list:
In this example, you will choose a city and add it to the
database list. You will then select the site to enable it.
4. Using the Arrow keys, change the name of
the site so that it now reads the name of your
observing location. Press Enter. “Edit: Name”
displays again.
1. Navigate to the “Setup: Site” menu.
Press ENTER,
2. Scroll through the options until “Site: Add”
displays. Press ENTER.
5. Press the Scroll Down key and “Edit: Latitude”
displays. Press ENTER.
3. You are given a choice to enter a zip code
(press “1”) or select a city from the list (press
“2”). If you choose “Zip”, enter the digits of your
zip code and press ENTER.
6. Using the Number Keys, enter the latitude of
your observing site and then press ENTER.
“Edit: Latitude” displays again.
7. Press the Scroll Down key and “Edit: Longitude”
displays. Press ENTER.
4. If you choose “City”, scroll through the list of
countries/states. Press ENTER when the
country/state you wish to add displays.
8. Using the Number Keys, enter the longitude
of your observing site and then press ENTER.
“Edit: Longitude” displays again.
5. Scroll through the list of cities. Press ENTER
when the city you wish to select displays. The
sites you choose will appear at the top of the
Select list (all other available sites will be listed
after the sites you have chosen).
9. Press the Scroll Down key and “Edit:Time Zone”
displays. Press ENTER. (If the site you chose
from the list in step 1 has the same Time Zone
as the site you are editing, just press ENTER
again to go on to the next step.) “Time Zone”
refers to the Greenwich Time Zone shift. Users
West of Greenwich, use “-” hours (one hour per
time zone) and users East of Greenwich use
“+” hours. For the United States, look up the
shift in Table 1, at the left.
6. To choose a site, navigate to “Site: Select”.
Press ENTER. Scroll through the list of sites.
Both Zip Codes and Cities are displayed.
When the desired zip code or site displays,
press ENTER.
To Edit a Site:
In this procedure, you will enter a location that is not
available in the AutoStar database by editing data of a
nearby site. You will edit the location’s name, latitude,
longitude and the time zone shift. You will then select
the site to enable it.
10. After entering the shift, press ENTER. “Edit
Time Zone” displays.
11. Press MODE. “Site: Edit” displays.
12. Using the Arrow keys, scroll to “Site: Select”.
The site you have just edited displays. Press
ENTER to select the site or press MODE
to exit.
You will need to know the latitude and longitude of your
location to perform this procedure. This information is
available on most maps.
1. Using the Add option, choose a site on the
list that is closest to your observing site and
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keys to enter the digits for the Right Ascension
coordinate of your object. When you are
finished, press ENTER.
Using AutoStar to Find Objects Not in
the Database
In this procedure, you will enter coordinates of celestial
objects that do not appear in any of the AutoStar
database lists. You will enter the object’s name and
R.A. and Dec. coordinates (required information).
You may also enter the object’s magnitude and size
(optional information).
7. “Declination:+00°.00’”displays.UsetheNumber
keys to enter the digits for the Declination
coordinate of your object. If necessary, use the
Scroll Keys to change “+” to “-”. When you are
finished, press ENTER.
8. AutoStar then prompts you to enter the size
of the object. This step is optional. Use the
Number keys to enter the size (in arc-minutes),
if so desired, and press ENTER to go to the
next display. If you do not wish to enter this
information, simply press ENTER.
Although AutoStar contains an extensive database of
celestial objects (stars, nebulae, planets, etc.) that you
can observe, you may eventually want to view objects
that are not part of the database. AutoStar provides
a feature that allows you to enter an object’s R.A.
and Dec. coordinates in the “User: Objects” option of
the Object menu and allows automatic slewing of the
telescope to the user-entered coordinates.
9. AutoStar then prompts you to enter the
magnitude of the object. This step is also
optional. Use the Number keys to enter this
information, if so desired, and press ENTER
to go to the next display. “User Object: Add”
displays again.
In order to use this menu option, you first need to look up
the R.A. and Dec. coordinates of the object or objects
you wish to observe. Check out your local library,
computer store, or bookstore for astronomy books,
CD ROMs, or magazines (such as Sky & Telescope
or Astronomy), to find coordinates of celestial objects.
The objects/coordinates you enter become part of your
own permanent database, called “User Objects”.
To GO TO a user-entered object:
In this procedure, you will choose an object from the
User Object list and GO TO the object.
1. With “User Object: Add” displayed, press the
Scroll Up key once. “User Object: Select”
displays. Press ENTER.
To enter coordinates of an object into the “User:
Objects” option of the Object menu:
1. Make sure AutoStar has been initialized and
the telescope has been aligned.
2. Use the Scroll keys (if necessary) to scroll to
the desired object. Press ENTER.
2. After the telescope is aligned, “Select Item:
Object” displays. (If necessary, use the Scroll
keys to scroll through the menus, as previously
described, to find this option.) Press ENTER.
3. The name of the object and the RightAscension
and Declination coordinates display.
4. Press GO TO and the telescope slews to
the object.
3. “Object: Solar System” displays. Keep pressing
the Scroll Up key until “Object: User Object”
displays and press ENTER.
Observing Satellites
In this procedure, you will prepare your telescope to
observe a satellite pass.
4. “User Object: Select” displays. Press the Scroll
Down key once. “User Object: Add” displays.
Press ENTER.
1. Navigate to the “Object: Satellite” menu option
and press ENTER.
5. “Name” displays on the top line and a blinking
cursor on the second line. Use the Arrow keys,
as previously described, to enter the name of
the object you wish to add to the database.
When you are finished, press ENTER.
2. Use the Scroll keys to scroll through the list
of satellites.
3. Select a satellite from list and press ENTER.
6. “Right Asc.: 00.00.0” displays. Use the Number
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4. “Calculating...” and then “Tracking...” displays.
If the satellite is going to make a pass,
“Located” displays.
Cable Connector Kit. See OPTIONALACCESSORIES,
page 16.
NOTE:Satelliteobservingisanexcitingchallenge.Most
satellites are in low orbit, travelling at approximately
17,500 mph. When visible, they move quickly across
the sky and are only in the field of view for a few minutes,
requiring AutoStar to slew the telescope rapidly. Best
viewing is near Sunrise or Sunset when the sky is
still dark. Viewing in the middle of the night can be
problematic because the satellite may pass overhead,
but not be visible as it is in the Earth’s shadow.
5. Use the Scroll keys to display data about the
pass: aos—acquisition of signal and los—loss
of signal. If you subtract the aos from the los,
you can calculate how long the satellite will be
visible. Location information also displays.
6. “Alarm” displays after the location information.
Press ENTER and AutoStar automatically
sets the alarm to sound a minute before the
satellite’s scheduled appearance. You may
return to regular observations until the alarm
goes off.
How to Create Your Own Guided Tour
When a Guided Tour is selected, AutoStar slews your
telescopetoapredeterminedlistofobjectsanddisplays
information about each object, such as type of object,
constellation location, R.A. and Dec. coordinates, and
so forth. AutoStar contains a few Guided Tours which
are programmed at the factory. But it is also possible
for an observer to create a custom Guided Tour.
7. When the alarm goes off, return to the Satellite
menu and press a Scroll key until the desired
satellite is on the top line of the display.
8. Press GO TO. AutoStar slews the telescope to
where the satellite should appear. The motor
drive stops and a countdown is displayed.
Atour is basically anASCII text file that contains a list of
directions and descriptions. Each line of a tour is either
a comment line, a command line, or a description.
Note: If the scheduled appearance position of
the satellite is obstructed (i.e., by a building,
tree, or hill), press ENTER and AutoStar starts
to move the telescope along the expected
satellite track. When the track clears the
obstruction, press ENTER again to pause the
telescope, then continue with this procedure.
What you will need:
•
A PC with text editor or word processing software
installed (the tour must be saved as a “text only” or as
a “MS-DOS text” file).
•
The Meade #505 Cable Connector Kit to download
9. With about 20 seconds left on the countdown
timer, start watching through the telescope
Viewfinder (Pg. 13, Fig. 1, 13) for the satellite
to enter the field of view.
tour information to the AutoStar handbox.
Tour Modes
The objects chosen for a tour list are selected from
AutoStar’s database or by entering the object’s R.A.
and Dec. coordinates. The tour is presented in one of
two modes:
10. When the satellite enters the viewfinder field
of view, press ENTER. The telescope starts to
track with the satellite.
Automatic Mode: The title of an object appears on first
11. Use the AutoStar Arrow keys to center the
object in the viewfinder, then look through the
eyepiece to view the object.
line and descriptive text scrolls on line 2.
Interactive Mode: Tour name appears on the first line
of the AutoStar display and the name of the object
displays on line 2. To display descriptive text in this
mode, the user must press ENTER.
Satellite orbits change and new satellites (including
the Space Shuttle) are launched. Visit the Meade web
to get updated information and instructions on how to
download this data to AutoStar. If orbital parameters
are more than one month old, the satellite pass may not
happen at the time predicted byAutoStar. Downloading
requires the optional #505 AstroFinder™ Software and
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Description String: Description of an object. Must be
surrounded by quotation marks. If the description is
longer than one line, each line must end with a quotation
mark and a hard return. Begin the next description line
with a quotation mark.
Comment Line
Information in the Tour program that is not displayed,
such as authorship, revision history,
copyrights, etc. All comments begin with a “/” character
in column 1 of the line. For example:
If quotation marks are to be displayed in the on-screen
description, use two quote marks at the beginning
and end of the desired phrase. For example: “The
Orion Nebula is considered “awesome” by many who
view it”.
/ Extreme Object
/ (c) 2009 Meade Instruments Corporation
Writing a Tour
Command Line
Using the list of commands listed above, a custom
tour can be created. Placing the word AUTO SELECT
before any of the command lines activates Automatic
Mode and, when selected, AutoStar automatically
searches and finds the designated object.
This line contains programming commands, including:
R.A. and DEC. coordinates, a title string, a description
string, and a keyword.
R.A.: Enter the Right Ascension of an object in the
following format: HH:MM:SS.
The following is a list of command lines, complete with
keywords and necessary strings:
Eg., 18:51:05
TITLE
Dec.: Enter the Declination of an object in the following
format: DDdMMmSSs. Eg., – 06d16m00s
Title must be the first keyword in your tour after any
comment lines and must be 15 characters or less.
AutoStar displays this title when “Guided Tour” is
selected from the menus.
Title String: Text within a title string is displayed as
the title of the object. A title string can contain up to
16 characters and must be surrounded by quotation
marks. For example. “M64” or “My Favorite Star”.
For example: TITLE “A Star’s Life”
TEXT “title string” “description string”
In Interactive Mode, the title string appears on line 2
until it is selected with the ENTER key.
This command allows you to display a text title and
description.
In Automatic Mode, or after Interactive Mode selection,
the title string appears on line 1 while the description
scrolls across line 2.
USER ra dec “title string” “description string”
Keywords: Action to be performed during a tour.
AutoStar recognizes the following keywords:
This command line allows you to access a specific
object with your own description. Enter USER, then
the R.A. and DEC. of a desired object, and its title and
description. Use the format described in the Command
Line section.
TITLE
TEXT
USER
NGC
IC
SAO
MESSIER
PLANET
CALDWELL
MOON
SATELLITE
COMET
ASTEROID
LUNAR ECLIPSE
DEEP SKY
STAR
The following commands specify objects that are
already in the AutoStar database. If these commands
follow the command AUTO SELECT, the object’s title
displays on line 1 and its description scrolls across
line 2.
METEOR SHOWER
CONSTELLATION
LANDMARK
PICK ONE/PICK END
#END
DEFINE
AUTO SLEW ON/OFF
Do not add a description string after the following
command lines; these commands access objects with
existing description in the AutoStar database.
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NGC xxxx
information about the satellite from its database. For
example: SATELLITE: “Intl Space Stn”
Enter NGC followed by the desired New General
Catalog number and AutoStar provides the user with
a description of the object from its database. For
example: NGC 4256
ASTEROID “name”
Enter ASTEROID and then the name of the desired
asteroid in quotes. AutoStar displays information
about the asteroid from its database. For example:
ASTEROID: “Ceres”
IC xxxx
Enter IC followed by the desired Index Catalog number
and AutoStar provides the user with a description of
the object from its database. For example: IC 1217
COMET “name”
Enter COMET and then the name of the desired
comet in quotes. AutoStar displays information
about the comet from its database. For example:
COMET: “Halley”
SAO xxxxxx
Enter SAO followed by the desired SAO number and
AutoStar provides the user with a description of the
object from its database. For example: SAO 30200
LUNAR ECLIPSE
Messier xxx
If LUNAR ECLIPSE is part of the tour, AutoStar checks
its database every time the tour is activated to see if
a lunar eclipse is visible that evening. If no eclipse is
visible, this option is skipped and the tour proceeds on
the next object.
EnterMESSIERfollowedbythedesiredMessiernumber
and AutoStar provides the user with a description of
the object from its database. For example: M 101
CALDWELL xxx
METEOR SHOWER
Enter CALDWELL followed by the Caldwell number
and AutoStar provides the user with a description
of the object from its database. For example:
CALDWELL 17
If METEOR SHOWER is part of the tour, AutoStar
checks its database every time the tour is activated
to see if a meteor shower is visible that evening. If no
meteor shower is visible, this option is skipped and the
tour proceeds on to the next object.
PLANET “name”
Enter PLANET and then the name of the desired planet
in quotes. AutoStar provides the user with a description
of the selected planet from its database. For example:
PLANET “Pluto”
DEEP SKY “name”
Enter DEEP SKY followed by the name of the desired
object in quotes. For example:
DEEP SKY “Small Magellanic Cloud”
MOON
CONSTELLATION “name”
This command accesses information about the Moon
from the AutoStar database.
Enter CONSTELLATION followed by the name of
the desired constellation in quotes. For example:
CONSTELLATION “Leo Major”
SATELLITE “name”
Enter SATELLITE and then the name of the desired
satellite in quotes. AutoStar displays
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There are no bright globular” “clusters visible at
this time”.
STAR “name”
Enter STAR followed by the name of the desired star in
quotes. For example: STAR “Vega”
PICK END
AUTO SLEW ON / AUTO SLEW OFF
With AUTO SLEW ON enabled in the tour, AutoStar
automatically slews the telescope to objects first before
displaying the text description. This feature is useful
when designing tours in which observing certain objects
is required. For example, an astronomy professor may
require his students to observe six objects, four of
which AutoStar automatically slews to in a tour. The
students would have to manually slew to the last two
objects. He would then place AUTO SLEW ON before
his first required object and AUTO SLEW OFF after the
fourth object.
LANDMARK az alt “title” “description”
Enter the azimuth (az) for the desired object in
the following format: xxxdxxmxxs. For example:
123d27m00s. Then enter the altitude of the desired
object in the following format: xxdxxmxxs. Then enter
the title string and description string in quotes. For
example:
LANDMARK 123d27m00s 57d20m20s “Landmark 1”
“North corner of apartment building”
PICK ONE / PICK END
#END
These two statements are used to surround a list of
items that AutoStar can choose from during a tour.
AutoStar begins at the top of the PICK ONE list and
displays the first object from the list that is above the
horizon and ignores the rest.
To end a tour, type the command #END on a separate
line at the very end of the tour.
Downloading Tours
This statement is useful for developing tours that can
be presented year round. For each object type you wish
to use to illustrate in your tour, pick 10 to 12 examples
spaced across the range of right ascension. Bracket
them by the PICK ONE / PICK END statements. One
current example displays for the user. For example:
Once a tour is written and stored as anASCII file (saved
either as a “text only” or “MS DOS text” file), load it into
AutoStar using the AutoStar Update Utility on your PC.
As tours are downloaded into the handbox, AutoStar
examines the programming. If it doesn’t understand
the terminology used within a tour, it flags questionable
areas and displays them in a pop-up window on your
computer screen. Make the necessary corrections
and try to download again. See the instruction
sheet with your #505 Cable Connector Kit for more
information about downloading data to and interfacing
with AutoStar.
AUTO SELECT TEXT “Globular Cluster” “Globular
clusters are huge balls of stars”.
“They contain 50,000 to 100,000 stars and are located
on the fringes of our “galaxy”.
PICK ONE
Landmarks
AUTO SELECT MESSIER 13
AUTO SELECT MESSIER 15
AUTO SELECT MESSIER 92
AUTO SELECT MESSIER 4
AUTO SELECT MESSIER 68
AUTO SELECT NGC 1234
This menu option allows you to define and store
terrestrial objects in the Landmark database. First,
a landmark needs to be stored in memory using the
“Landmark: Add” option. To view a landmark, use the
“Landmark: Select” option. Landmarks may also be
viewed using the “Landmark Survey” option in the
Utilities menu.
AUTO SELECT TEXT “None Available” “I’m sorry.
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To Select a landmark from the database:
To Add a landmark to the database:
1. Make sure the telescope is located and aligned
exactly as when the desired landmark was
entered into memory.
In this procedure, you will store the location of terrestrial
landmarks in AutoStar’s memory.
2. Display the “Landmark: Select” menu option.
Press ENTER.
1. Set the telescope in the home position, if
necessary. Note for future reference where the
telescope is located and if you have aligned the
telescope, which alignment method is used.
3. Use the Scroll keys to scroll through the list
of objects you have previously entered. When
the desired object displays, press ENTER to
select the object. Use the Scroll keys to scroll
through location information about the object, if
desired. Press GO TO to slew the telescope to
the landmark.
IMPORTANT NOTE: To use the Landmark
function, the telescope must be located and
aligned exactly as when the landmark(s) was
added to the database.
2. Display the “Setup: Targets” menu option.
Choose“Terrestrial”andpressENTER–“Setup:
Targets” displays again. Choosing this option
turns off tracking for astronomical objects and
is not useful for the viewing of terrestrial objects
such as those in the Landmark database. Be
suretochangethisoptionbackto“Astronomical”
when you wish to view celestial objects again.
4. Press MODE to exit.
To perform a Landmark Survey
This procedure allows you to perform a tour of the
objects entered in the “Object: Landmark” menu
option – note that the Landmark Survey will function
only if you have previously entered objects in the
Landmark menu.
3. Press MODE once. “Select Item: Setup”
displays.
1. Navigate to “Utilities: Landmark Survey” menu
and press ENTER.
4. Press the Scroll Down key once and “Select
Item: Object” displays. Press Enter. “Object:
Solar System” displays.
2. “Landmark Survey: Slewing...” displays. The
telescopemovestothefirstobjectontheSurvey
list and displays the name of the object.
5. Press the Scroll Up key twice and “Object:
3. Press MODE to pause the Survey. Press
Enter to restart the survey at the first object of
the survey.
Landmarks”
displays.
Press
ENTER.
“Landmark: Select” displays.
6. Press the Scroll Down key once. “Landmark:
Add” displays. Press ENTER.
To check on the available amount of memory in
AutoStar.
7. “Landmark Name” displays. Using Arrow
keys, enter a name for the landmark you
wish to add to the database. When finished,
press ENTER.
AutoStar has a limited amount of memory. Once you
begin to store Landmarks, User Objects and other bits
of information in AutoStar, you will begin to use up
memory. This procedure allows you to check on how
much memory is still available.
8. “Center Landmark. Press Enter” displays.
Using only the Arrow keys (do not manually
move the telescope), move the telescope to
the desired landmark and center the object in
the eyepiece. Press Enter. The object is now
stored in memory.
1. Navigate to the “Setup: Statistics” menu option
and press ENTER.
2. “Statistics: 97.4K Char. Free” displays. This is
the amount of memory that is still available to
the user.
9. “Landmark: Add” displays. If you wish to add
more landmarks, repeat steps 5 through 7.
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Advanced Alt/Az Alignment
Identify
If you would rather choose your own alignment
stars from the Autostar database during the Alt/Az
alignment procedure, Autostar offers two methods
described below.
This procedure allows you to use AutoStar to identify
objects you have found in the night sky using the
Arrow keys. If the object is not in AutoStar’s database,
AutoStar displays information about an object in its
database that is closest to the one you queried about.
Two-Star Alt/Az Alignment
Important Note: The telescope must be
successfully aligned before the Identify feature
can be used. Once aligned, it cannot be
physically moved from that location. Moving
the telescope disrupts the telescopes frame
of reference to the night sky and will prevent it
from identifying objects.
Two-Star Alignment requires some knowledge of the
night sky. AutoStar provides a database of bright stars
and two stars from this database are chosen by the
observer for alignment.
1. Turn the telescope on: Turn the telescope
power switch to the ON position. The AutoStar
beeps and the display screen is activated.
AutoStar then takes a few moments to start up
the system.
In this procedure, you will center an object you wish to
have identified by AutoStar in the telescope eyepiece
and use the “Identify” menu to find out information about
the object or the nearest object to it in the AutoStar
database.
2. Select Alignment Procedure: “Press 0 to Align
or Mode for Menu” displays. Press “Mode” to
access the AutoStar menu.
1. Center the object you wish to have identified in
3. Testing Motors: The telescope then tests the
motor function of the telescope by moving in
the horizontal and vertical directions.
the telescope’s eyepiece.
2. Navigate to the “Object: Identify” option and
press ENTER.
4. Set Your Location or Zip Code: The Location
screen displays. This screen asks you if you
wish to choose either the zip code of your
observing location or the location (i.e., entering
the city and state or country of your observing
location). Press “1” to select the zip code option
or “2” to enter the city and state.
3. “Searching...” displays. When AutoStar finishes
calculating, the name of the closest object
displays.
4. Press a Scroll key to display information about
this object. AutoStar displays some or all the
following information about the object with each
press of a Scroll key:
Note:Thelocationsettings(country/state/province
and city, or zip code) are only asked for the first
time you turn on the control panel. If you wish to
change this setting later on, use the Site menu.
See SITE, page 29 for more information.
Displayed information:
Example:
Catalog or common name...Messier 107, NGC 6171,
Orion Nebula, etc
Type of object......................Globular Cluster, Nebula,
Black Hole, etc.
a. If you chose the zip code option, the left most
“0” is highlighted. Use the Number keys to enter
the digits. As you enter a digit, the next digit to
the right will be highlighted. Enter the next digit.
Repeat this process until all 5 digits of your zip
code are entered. Press ENTER.
Right Ascension.................. 16:32:4
Declination.......................... 13°03’
Constellation ...................... Virgo, Orion, etc.
Magnitude........................... 3
Size..................................... 2’
b. If you chose the location option, the next
screen asks for the country or state/province
(listed alphabetically) of the observing site.
Scrolling message...............“This Globular Cluster is
10,000 light years
away...”
c. Use the Scroll keys to scroll through the list of
countries, states, and provinces. Press ENTER
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13.Repeat procedure for the second alignment
star. The telescope is aligned and you are now
ready to use Autostar’s GO TO capabilities for
a night of observing.
when the correct location displays.
d. The next screen asks for the city (listed
alphabetically) closest to the observing site.
Use the Scroll keys to scroll through the list
of cities. Press ENTER when the correct city
appears on screen.
5. Daylight Savings Time: The next screen
requests the status of Daylight Savings Time.
If Daylight Savings Time is active, press the
1 key. If Daylight Savings Time is not active,
press the 2 key.
Note: Daylight Savings Time may be referred
to by a different name in various areas of
the world.
6. Telescope Model: AutoStar then asks for the
Telescope Model. Using the scroll keys (Pg. 19,
Fig. 5, 7) on the AutoStar locate the model of
your telescope and press enter.
LT Series TIPS
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’s aperture
and atmospheric 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. 12a and 12b to the left). Powers above 400X
should be employed only under the steadiest
atmospheric conditions.
7. Now
enter
the
current
date,
then
press ENTER.
8. Enter the current time. Select “AM,” “PM,” or
24-hour clock (blank). Then press ENTER.
9. With “Align: Easy” displayed, use the Scroll
Keys to display “Align: Two Star”. Press Enter.
10. Setting the Home Position: “North Method:
1=True 2=Compass” displays. AutoStar is
asking which Home Position method to use
to setup the telescope. See page 9 “The LT
Series Home Position” for more information.
The easiest way to set the telescope in the
home position is using the Magnetic North
method. Follow the steps on page 9 to set the
home position. If using True North, press the “1”
key, or press the “2” key to use Magnetic North.
Press enter when complete.
Most observers should have three or four
additional eyepieces to achieve the full range
of reasonable magnifications possible with
the LT Series telescopes. See OPTIONAL
ACCESSORIES, page 16.
11. “Select Star” displays. Autostar then displays a
database of stars for the observer to choose
from. Use the Scroll keys to scroll to a star on
the list that you wish to align upon. Select a
star that you can easily locate in the night sky.
Press ENTER.
12.The telescope slews to the star. Use the Arrow
keys to move the telescope until the star is
centered in the eyepiece. Press ENTER.
Figs. 12a & 12b: Jupiter; examples of the right amount of
magnification and too much magnification.
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One-Star Alt/Az Alignment
One-Star Alignment requires some knowledge of the
night sky. Autostar provides a database of bright stars.
One-Star Alignment is identical to Two-Star Alt/Az:
Alignment (see “Two-Star ALT/AZ Alignment,” above),
except only one star from this database is chosen by
the observer for alignment.
IMPORTANT NOTE : The accuracy of One-
Star Alt/Az Alignment, unlike the Two-Star and
Easy (Alt/Az) Alignment procedures, depends
on how well the observer levels the telescope
and how close to North the telescope is pointed
when setting the Home Position (Pg. 9, Fig. 6).
Because the other methods use two stars to
align upon, they are more precise than One-
Star Alignment.
Browse
Thismenuallowsyoutosearchthedatabaseforobjects
with certain parameters, much like a search engine.
“Edit Parameters” lets you set various parameters for
the search, and “Start Search” activates the search. A
typical search might be performed as follows:
1. Select “Browse” from the Object menu. Press
ENTER. “Browse: Start Search” displays.
2. Press one of the Scroll Keys and “Browse: Edit
Parameters” displays. Press Enter.
3. “Edit Parameters: Largest (mins)” displays.
“Mins” stands for arc-minutes. Press ENTER.
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MAINTENANCE
The LTSeries is a precision optical instrument designed
to yield a lifetime of rewarding viewing.
7. If the LT Series is not to be used for an extended
period, perhaps for one month or more, it is
advisable to remove the batteries from the
telescope. Batteries left in the telescope for
prolonged periods may leak, causing damage to
the telescope’s electronic circuitry.
Given the care and respect due any precision
instrument, the LT Series will rarely, if ever, require
factory servicing. Maintenance guidelines include:
1. Avoid cleaning the telescope’s optics: a little dust
on the front surface of the telescope’s correcting
lens causes virtually no degradation of image
quality and should not be considered reason to
clean the lens.
8. Do not leave the LT Series inside a sealed car on
a
warm summer day; excessive ambient
temperatures can damage the telescope’s
internal lubrication and electronic circuitry.
2. When absolutely necessary, dust on the front lens
should be removed with gentle strokes of a camel
hair brush or blown off with an ear syringe
(available at any pharmacy). DO NOT use a
commercial photographic lens cleaner.
Collimation
The optical collimation (alignment) of any astronomical
telescope used for serious purposes is important, but
in the case of the Schmidt-Cassegrain design of the
LT Series, such collimation is absolutely essential
for good performance. Take special care to read and
understand this section well so that your LT Series will
give you the best optical performance.
3. Organic materials (e.g., fingerprints) on the front
lens may be removed with a solution of 3 parts
distilled water to 1 part isopropyl alcohol. You
may also add
1
drop of biodegradable
As part of final optical testing, every Meade LT Series
is precisely collimated at the Meade factory before
shipment. However, vibrations in shipping can cause
the optical system to become misaligned. Re-aligning
the optics is, however, a straightforward process.
dishwashing soap per pint of solution. Use soft,
white facial tissues and make short, gentle
strokes. Change tissues often.
4. CAUTION:Donotusescentedorlotionedtissues
that can damage the optics.
To check the collimation of your LT Series, center
a bright star that is overhead, or use a “hot spot” of
reflected Sunlight from a chrome car bumper, with
the supplied 26mm eyepiece. Allow the telescope
to adjust to the temperature of your observation site
before proceeding; temperature differences between
the optics and the outside air can cause distortion in
5. Do not, for any reason, remove the correcting
plate from its machined housing for cleaning
or other purposes. You will almost certainly
notbeabletoreplacethecorrectorinitsproper
rotationalorientationandseriousdegradation
of optical performance will result. Meade
Instruments assumes no liability for damage
incurred to the telescope in this way.
6. If the LT Series is used outdoors on a humid
night, water condensation on the telescope
surfaces will probably result. While such
condensation does not normally cause any
damage to the telescope, it is recommended that
the entire telescope be wiped down with a dry
cloth before the telescope is packed away. Do
not, however, wipe any of the optical surfaces.
Rather, simply allow the telescope to sit for some
time in the warm indoor air, so that the wet optical
surfaces can dry unattended.
(1)
(2)
(3)
Figure 13: Collimation
the images.
With the star or hot spot centered, de-focus
the image.
You will notice that the out of focus star image looks
like a ring of light surrounding a dark central spot; the
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dark central spot is in fact the shadow of the secondary
mirror. Turn the focus knob until the ring of light fills
about 10% of the eyepiece field-diameter. If the dark
central spot is offset in (i.e., not concentric with) the ring
of light, your telescope’s optical system is misaligned
and requires collimation.
3. Using the Arrow keys at the slowest slew speed,
move the defocused image to the edge of the
eyepiece field of view (Pg. 41, Fig. 13 , 2), in the
same direction as the darker shadow is offset in
the ring of light.
4. Turn the set screw that you found with the
pointing exercise while looking in the eyepiece.
You will notice that the star image will move
across the field. If while turning the defocused
star image flies out of the eyepiece field, then
you are turning the screw the wrong way. Turn
the opposite direction and bring the image back
to the center of the field.
Follow these steps for collimation of the
optical system:
1. The only adjustments possible, or necessary, on
theLTSeriesarefromthethreeinnermostscrews
Collimation Screws
5. If the screw you are turning becomes very loose,
tighten the other two screws by even amounts. If
the screw you are turning gets too tight, un-thread
the other two by even amounts.
6. When you bring the image to center (Pg. 41, fig.
13, 3), carefully examine the evenness of the ring
of light (concentricity). If you find that the dark
center is still off in the same direction, continue to
make the adjustment in the original turning
direction. If it is now off in the opposite direction,
you have turned too far and you need to turn in
the opposite direction. Always double check the
image in the center of the field of the eyepiece.
Figure 14: The LT Series Collimation
located at the inner surface of the secondary
mirror housing.
CAUTION:Donotforcethethreecollimationscrews
past their normal travel and do not loosen them
more than two full turns in a counterclockwise
direction or the secondary mirror may come loose
from its support. You will find that the adjustments
are very sensitive, usually requiring only one-half
turn or less to produce the desired result.
7. You may find after your initial adjustment that the
dark center is off in a new direction (e.g., instead
of being off side-to-side it is now off in an up-and-
down direction). In this case repeat steps 2
through 6 to find the new adjustment screw.
2. While looking at the defocused star image, notice
which direction the darker shadow is offset in the
ring of light or notice which part of the ring is the
thinnest (Pg. 41 Fig. 13, 1). Place your index
finger in front of the telescope so that it touches
one of the collimation set screws. You will see the
shadow of your finger in the ring of light. Move
your finger around the edge of the black plastic
secondary mirror support until you see the
shadow of the finger crossing the thinnest part
of the ring of light. At this point, look at the front of
the telescope where your finger is aiming. It will
either be pointing directly at a set screw, or it will
be between two set screws aiming at the set
screw on the far side of the black plastic
secondary mirror support. This is the set screw
that you will adjust.
8. Now try a higher power eyepiece (e.g., 9mm or
less) and repeat the above tests. Any lack of
collimation at this point will require only very
slight adjustments of the three set screws. You
now have good collimation of the optics.
9. As a final check on alignment, examine the star
image in focus with the higher power eyepiece
as suggested above, under good viewing
conditions. The star point should appear as a
small central dot (commonly referred to as an
“Airy disc”) with a diffraction ring surrounding it.
To give a final precision collimation, make
extremely slight adjustments of the three set
screws, if necessary, to center the Airy disc in the
diffraction ring. You now have the best alignment
of the optics possible with this telescope.
42
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Inspecting the Optics
CUSTOMER
SERVICE
A Note About the “Flashlight Test”: If a flashlight or
other high-intensity light source is pointed down the
main telescope tube, the view (depending upon the
observer’s line of sight and the angle of the light) may
reveal what appears to be scratches, dark or bright
spots, or just generally uneven coatings, giving the
appearance of poor quality optics. These effects are
only seen when a high intensity light is transmitted
through lenses or reflected off the mirrors, and can be
seen on any high quality optical system, including giant
research telescopes.
If you have a question concerning your LT Series
telescope, call the Meade Instruments Customer
Service Department at (800) 626-3233. Customer
Service hours are 7:00 AM to 5:00 PM, Pacific Time,
Monday through Friday. In the unlikely event that
the LT Series requires factory servicing or repairs,
before returning the telescope to the factory, write
or call the Meade Customer Service Department
to provide an explanation of the problem, as well as
your name, address and daytime telephone number.
The great majority of servicing issues can be resolved
by telephone, avoiding return of the telescope to
the factory.
The optical quality of a telescope cannot be judged by
the “flashlight test;” the true test of optical quality can
only be conducted through careful star testing.
Gauging the Movement of
the Telescope
A common complaint of many first-time telescope
owners is that they cannot see the telescope “move”
when the motor drive is engaged. If fact, when the
batteries are installed, the power is on, the telescope
is moving. However, the movement is at the same
speed as the hour hand of a 24-hour clock; as such,
the movement is difficult to discern visually.
To check the movement of your telescope, look at an
astronomical object through the telescope’s eyepiece
with the telescope polar aligned and with the motor
drive on. If the object remains stationary in the field
of view, your telescope is operating properly. If not,
check to ensure that “Astronomical” is selected in the
“Targets” option of the setup menu.
Updating Your LT Series Firmware
Meadeisconstantlyrefiningandimprovingtheoperating
firmware that controls our computerized telescopes and
we even add new features and capabilities from time to
time. Your new LT Series shipped with the most current
firmware at the time of manufacture, but there may
well be a new version available through the AutoStar
Updated program supplied on the AutoStar Suite DVD
supplied with your telescope. The Updater goes online
to the Meade web site and checks to see if there is a
newer version available and can download it directly
to the telescope using the #505 Cable Connector Kit.
See the instruction sheet included with the kit for more
information.
43
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APPENDIX A:
Verify that AUTOSTAR
INITIALIZATION is
complete.
Press > until it
is centered
1
2
12
TRAINING THE DRIVE
Scope slews left.
Bring target back
to center using
Perform this procedure if you are experiencing any
pointing accuracy problems. Fig. 15 depicts the
complete Drive Training procedure.
Press MODE until
Select Item is displayed.
the Right Arrow key.
Select Item
3
Object
Press < until it
is centered
13
Press the scroll
up key once.
NOTE: Use a far away terrestrial object, such as a
telephone pole or lamp post, to train the drive.
Scope slews right.
Bring target back
to center using
Complete this exercise once every 3 to 6 months.
Select Item
Setup
4
the Left Arrow key.
Access the Setup
menu.
Train Drive
Az. Train
14
Menu returns to
Az. training.
Setup
5
Align
Multiple presses.
Train Drive
Alt. Train
Altitude
15
16
Setup
6
(vertical)
training.
Telescope
Access the
Telescope menu.
Drive Setup
For this op. . .
Reminder to
use terrestrial
target.
Telescope
Telescope Model
7
Multiple presses.
Center reference
17
object
Center target
using Arrow
keys.
Telescope
Train Drive
8
Choose the Train
Drive option.
Press until it
is centered
18
Scope slews down.
Bring target back
to center using
Train Drive
Az. Train
Azimuth
9
the Up Arrow key.
(horizontal)
training.
Press until it
is centered
19
Drive Setup
For this op. . .
Reminder to
10
Scope slews up.
Bring target back
to center using
use terrestrial
target.
the Down Arrow key.
Center reference
object.
Train Drive
Az. Train
Multiple presses.
11
20
Center target
using Arrow
keys.
MODE
Select Item
Object
21
Figure 15: Training the Drive
44
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APPENDIX B:
BASIC ASTRONOMY
In the early 17th century Italian Scientist Galileo, using
a crude telescope considerably smaller than the LT
Series, turned it to look towards the sky instead of
distant trees and mountains. What he saw, and what
he realized about what he saw, forever changed the
way mankind thought of the universe. Imagine what it
must have been like being the first human to see moons
revolve around the planet Jupiter or to see the changing
phases of Venus! Because of his observations, Galileo
correctly realized Earth’s movement and position
around the Sun, and in doing so, gave birth to modern
astronomy. Yet Galileo’s telescope was so crude, he
could not clearly make out the rings of Saturn.
The Moon is, on average,
a distance of 239,000 miles
(380,000km) from Earth
and is best observed during
its crescent or half phase
when Sunlight strikes the
Moon’s surface at an angle.
It casts shadows and adds
a sense of depth to the
view. No shadows are seen
during a full Moon, causing
the overly bright Moon
to appear flat and rather
uninteresting through the
Galileo’s discoveries laid the foundation for
understanding the motion and nature of the planets,
stars,andgalaxies.Buildingonhisfoundation,Henrietta
Leavittdeterminedhowtomeasurethedistancetostars;
Edwin Hubble proposed a glimpse into the origin of the
universe; Albert Einstein unraveled the relationship
of time and light. Almost daily, using sophisticated
successors to Galileo’s crude telescope, such as the
Hubble Space Telescope, more and more mysteries of
the universe are being solved and understood. We are
living in a golden age of astronomy.
telescope. Be sure to use a neutral Moon filter when
observing the Moon. Not only does it protect your eyes
from the bright glare of the Moon, but it also helps
enhance contrast, providing a more dramatic image.
Using the LT Series, brilliant detail can be observed
on the Moon, including hundreds of lunar craters and
maria, described below.
Craters are round meteor impact sites covering most
of the Moon’s surface. With no atmosphere on the
Moon, no weather conditions exist, so the only erosive
force is meteor strikes. Under these conditions, lunar
craters can last for millions of years.
Unlike other sciences, astronomy welcomes
contributions from amateurs. Much of the knowledge
we have on subjects such as comets, meteor showers,
variable stars, the Moon and our solar system comes
from observations made by amateur astronomers. So
as you look through your Meade LT Series telescope,
keepGalileoinmind.Tohim,atelescopewasnotmerely
a machine made of glass and metal, but something far
more - a window through which the beating heart of the
universe might be observed.
Maria(pluralformare)aresmooth,darkareasscattered
across the lunar surface. These dark areas are large
ancient impact basins that were filled with lava from
the interior of the Moon by the depth and force of a
meteor or comet impact.
Twelve Apollo astronauts left their bootprints on the
Moon in the late 1960’s and early 1970’s. However,
no telescope on Earth is able to see these footprints or
any other artifacts. In fact, the smallest lunar features
that may be seen with the largest telescope on Earth
are about one-half mile across.
Objects in Space
Listed below are some of the many astronomical
objects that can be seen with the LT Series
45
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Planets change positions in the sky as they orbit
around the Sun. To locate the planets on a given day or
month, consult a monthly astronomy magazine, such
as Sky and Telescope or Astronomy. You can also
consult LT Series for information about planets. Scroll
to the “Object: Solar System” menu and scroll through
the lists of planets. When a planet you are interested
in displays, press “ENTER”. Use the Scroll keys to
display information about the planet, such as the
planet’s coordinates, and the rise and set times (Tip:
enter a date in the Date menu and you can determine
if a planet) will be visible during the night of the entered
date by checking its rise and set times). Listed below
are the best planets for viewing through the LT Series.
moons can also be seen
as a bright, star-like object
near the planet.
Deep-Sky Objects
Star charts can be used
to locate constellations,
individual stars and deep-
sky objects.
Examples
deep-sky
of
various
are
objects
given below:
Stars are large gaseous
objects that are self-
illuminated by nuclear fusion in their core. Because
of their vast distances from our solar system, all stars
appear as pinpoints of light, irrespective of the size of
the telescope used.
Mars is about half the diameter of Earth, and appears
through the telescope as a tiny reddish-orange disk.
It may be possible to see a hint of white at one of the
planet’s Polar ice caps. Approximately every two years,
when Mars is closest to Earth in its orbit, additional
detail and coloring on the planet’s surface may
be visible.
Nebulae are vast interstellar clouds of gas and dust
where stars are formed. Most impressive of these is
the Great Nebula in Orion (M42), a diffuse nebula that
appears as a faint wispy gray cloud. M42 is 1600 light
years from Earth.
Jupiter is the largest planet
in our solar system and is 11
times the diameter of Earth.
Open Clusters are loose groupings of young stars,
all recently formed from the same diffuse nebula.
The Pleiades is an open cluster 410 light years away.
Through the LT Series, numerous stars are visible.
Constellations are large, imaginary patterns of stars
believed by ancient civilizations to be the celestial
equivalent of objects, animals, people, or gods. These
patterns are too large to be seen through a telescope.
To learn the constellations, start with an easy grouping
of stars, such as the Big Dipper in Ursa Major. Then,
use a star chart to explore across the sky.
Theplanetappearsasadisk
with dark lines stretching
across the surface. These
lines are cloud bands in
the atmosphere. Four of
Jupiter’s 16 moons (Io,
Europa, Ganymede, and
Callisto) can be seen as
“star-like” points of light
when using even the lowest
magnification. These moons orbit Jupiter so that the
number of moons visible on any given night changes
as they circle around the giant planet.
Galaxies are large assemblies of stars, nebulae,
and star clusters that are bound by gravity. The most
common shape is spiral (such as our own Milky Way),
but galaxies can also be elliptical, or even irregular
blobs. The Andromeda Galaxy (M31) is the closest
spiral-type galaxy to our own. This galaxy appears
fuzzy and cigar-shaped. It is 2.2 million light years
away in the constellation Andromeda, located between
the large “W” of Cassiopeia and the great square of
Pegasus.
Saturn is nine times the diameter of Earth and appears
as a small, round disk with rings extending out from
either side. In 1610, Galileo, the first person to observe
Saturn through a telescope, did not understand that
what he was seeing were rings. Instead, he believed
that Saturn had “ears.” Saturn’s rings are composed of
billions of ice particles ranging in size from a speck of
dusttothesizeofahouse.ThemajordivisioninSaturn’s
rings, called the Cassini Division, is occasionally visible
through the LT Series. Titan, the largest of Saturn’s 18
46
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APPENDIX C:
SPECIFICATIONS
Model and Product Number
6" LT ACF # 0610-04-10
Optical System
Optical Design
Advanced Coma-Free (ACF)
Primary Mirror Diameter
Primary Mirror Material
Focal Length, Focal Ratio
Optical Coatings
6” (152mm)
Pyrex® Glass
1524mm, f/10
Ultra-High Transmission Coatings (UHTC™)
Resolving Power (arc seconds)
Limiting Visual Stellar Magnitude
Viewfinder
0.76
14
Red Dot
Mount
Mount Type
Drives
Aluminum Single-Arm Fork Altazimuth
4.875 inch Precision Worm Drive
8 “C” Cell Batteries or AC Adapter
20 hours
Power
Battery Life
Tripod
New Adjustable-Height Steel Leg Tripod
Electronics
Controller Hand Box
AutoStar #497
Included Accessories
Eyepiece Holder
Eyepiece
1.25” Diagonal Prism
Super Plössl 26mm
SC Adapter
SC Thread to 1.25” Accessory Adapter
Weight
Telescope
Tripod
30 lbs.
9 lbs
47
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SPECIFICATIONS
Model and Product Number
6" LT SC # 0610-04-12
Optical System
Optical Design
Schmidt Cassegrain (SC)
Primary Mirror Diameter
Primary Mirror Material
Focal Length, Focal Ratio
Optical Coatings
6” (152mm)
Pyrex® Glass
1524mm, f/10
Ultra-High Transmission Coatings (UHTC™)
Resolving Power (arc seconds)
Limiting Visual Stellar Magnitude
Viewfinder
0.76
14
Red Dot
Mount
Mount Type
Drives
Aluminum Single-Arm Fork Altazimuth
4.875 inch Precision Worm Drive
8 “C” Cell Batteries or AC Adapter
20 hours
Power
Battery Life
Tripod
New Adjustable-Height Steel Leg Tripod
Electronics
Controller Hand Box
AutoStar #497
Included Accessories
Eyepiece Holder
Eyepiece
1.25” Diagonal Prism
Super Plössl 26mm
SC Adapter
SC Thread to 1.25” Accessory Adapter
Weight
Telescope
Tripod
30 lbs.
9 lbs
48
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APPENDIX D:
ACF AND SC OPTICAL SYSTEMS
(2)
(1)
(2)
(1)
Ray (2)
Ray (1)
(2)
(1)
Secondary
Mirror
Focal
Plane
Secondary
Baffle
Primary Baffle Tube
Field Stops
Correcting
Plate
Primary Mirror
The Meade Advanced Coma-Free Optical System
Unlike
Schmidt-Cassegrain
systems,
Meade’s
mirror.
Advanced Coma-Free (ACF) optical system provides
razor-sharp pin-point star images all the way to the very
edge of the field of view. This aplanatic (coma-free)
optical system brings the highest level of performance
to the amateur astronomer.
All models of the Meade LT includes oversize primary
mirrors, yielding
a
fully illuminated field-of-view
significantly wider than is possible with a standard-size
primary mirror. Note that light ray (2) in the figure would
be lost entirely, except for the oversize primary. It is
this phenomenon which results in Meade ACF having
off-axis field illuminations about 10% greater, aperture-
for-aperture, than other systems utilizing standard-size
primary mirrors. Field stops machined into the inside-
diameter surface of the primary mirror baffle tube
significantly increase lunar, planetary, and deep-space
image contrast. These field stops effectively block off-
axis stray light rays.
In the ACF design of the Meade LT Series, light enters
from the right, passes through a thin lens with 2-sided
aspheric correction (“correcting plate”), proceeds to
a spherical primary mirror, and then to a hyperbolic
secondary mirror. The hyperbolic secondary mirror
multiplies the effective focal length of the primary
mirror and results in a focus at the focal plane, with light
passing through a central perforation in the primary
(2)
(1)
(2)
(1)
Ray (2)
Ray (1)
(2)
(1)
Secondary
Mirror
Focal
Plane
Secondary
Baffle
Primary Baffle Tube
Field Stops
Correcting
Plate
Primary Mirror
The Meade Schmidt-Cassegrain Optical System
In the Schmidt-Cassegrain design of the Meade LT,
illuminated field-of-view significantly wider than is
possible with a standard-size primary mirror. Note that
light ray (2) in the figure would be lost entirely, except
for the oversize primary. It is this phenomenon which
results in Meade Schmidt-Cassegrains having off-axis
field illuminations about 10% greater, aperture-for-
aperture, than other Schmidt-Cassegrains utilizing
standard-size primary mirrors. Field stops machined
into the inside-diameter surface of the primary mirror
baffle tube significantly increase lunar, planetary,
and deep-space image contrast. These field stops
effectively block off-axis stray light rays.
light enters from the right, passes through a thin lens
with 2-sided aspheric correction (“correcting plate”),
proceeds to a spherical primary mirror, and then to
a convex secondary mirror. The convex secondary
mirror multiplies the effective focal length of the
primary mirror and results in a focus at the focal plane,
with light passing through a central perforation in the
primary mirror.
All models of the Meade LT Schmidt-Cassegrain
includes oversize primary mirrors, yielding a fully
49
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APPENDIX E:
FEDERAL COMMUNICATIONS COMMISSION
DECLARATION OF CONFORMITY (DoC)
FOR THE FOLLOWING EQUIPMENT:
PRODUCT NAME
MODEL NO
: MEADE LT SERIES TELESCOPE
: LT
TRADE NAME
: MEADE INSTRUMENTS CORP.
IS HERE WITH CONFIRMED AND FOUND TO COMPLY WITH THE
REQUIREMENTS OF CFR47 PART 15 REGULATION. THE RESULTS OF
ELECTROMAGNETIC EMISSION EVALUATION ARE SHOWN IN THE REPORT NO.:
(5209)251-0926, ISSUED ON SEPTEMBER 16, 2009.
THIS DEVICE COMPLIES WITH PART 15 OF THE FCC RULES. OPERATION IS
SUBJECT TO THE FOLLOWING TWO CONDITIONS:
(1)THIS DEVICE MAY NOT CAUSE HARMFUL INTERFERENCE AND,
(2)THIS DEVICE MUST ACCEPT ANY INTERFERENCE RECEIVED, INCLUDING
INTERFERENCE THAT MAY CAUSE UNDESIRED
OPERATION.
THE FOLLOWING MANUFACTURER/IMPORTER IS RESPONSIBLE FOR THIS
DECLARATION:
MEADE INSTRUMENTS CORP.
27 HUBBLE
IRVINE, CA. 92618 U.S.A.
(Tel) 800-626-3233
(Name) Bob LaTouche (Title) Director of Quality
(Date) NOVEMBER 03, 2009
50
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RECYCLING INFORMATION
(EU Countries only)
Correct Disposal of this Product
(Waste Electrical & Electronic Equipment)
This marking shown on the product or its literature
indicates that it must not be disposed of in unsorted
municipal waste at the end of its working life
To prevent possible harm to the environment or human
health from uncontrolled waste disposal, please separate
this from other types of wastes and recycle it as required
by law. Household users should contact either the
retailer where they purchased this product, or their local
government office, for details of where and how they
can take this item for environmentally safe recycling.
Business users should contact their supplier and check the terms and conditions of the
purchase contract
This product should not be mixed with other commercial wastes for disposal.
51
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MEADE LIMITED WARRANTY
Every Meade telescope, spotting scope, and telescope accessory is warranted by Meade Instruments
Corp. (“Meade”) to be free of defects in materials and workmanship for a period of ONE YEAR from the
date of original purchase in the U.S.A. and Canada. Meade will repair or replace a product, or part thereof,
found by Meade to be defective, provided the defective part is returned to Meade, freight-prepaid, with
proof of purchase. This warranty applies to the original purchaser only and is non-transferable. Meade
products 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 must be obtained from Meade by writing, or calling (800) 626-3233. Each returned part or
product must include a written statement detailing the nature of the claimed defect, as well as the
owner’s name, address, and phone number.
This warranty is not valid in cases where the product has been abused or mishandled, where unauthorized
repairs have been attempted or performed, or where depreciation of the product is due to normal wear-
and-tear. Meade specifically disclaims special, indirect, or consequential damages or lost profit which
may result from a breach of this warranty. Any implied warranties which cannot be disclaimed are hereby
limited to a term of one year from the date of original retail purchase.
This warranty gives you specific rights. You may have other rights which vary from state to state.
Meade reserves the right to change product specifications or to discontinue products without notice.
27 Hubble, Irvine, California 92618
55-09004
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