INSTRUCTION MANUAL
Meade® 7" LX200 Maksutov-Cassegrain Telescope
8", 10", and 12"
LX200 Schmidt-Cassegrain Telescopes
3.
Precise Polar Alignment it's necessary
A. INTRODUCING THE MEADE LX200
As a new LX200 owner, you are preparing for a journey into the universe
with the most advanced amateur telescope ever produced. The advent of this
instrument is the culmination of twenty years of innovation and design
at Meade Instruments; never before have the features you have in your hands
been available to amateur astronomers: from robotic object location to
the revolutionary Smart Drive and the most stable mounting structure ever.
Your telescope comes to you ready for adventure; it will be your tour guide
and traveling companion in a universe of planets, galaxies, and stars.
Meade 8", 10", and 12" LX200 Schmidt-Cassegrain and 7"
Maksutov-Cassegrain telescopes are instruments of advanced mirror-lens
design for astronomical and terrestrial applications. Optically and mechanically,
the 7", 8", 10", and 12" telescope models are perhaps
the most sophisticated and precisely manufactured telescopes ever made
available to the serious amateur. These telescopes enable the visual astronomer
to reach out for detailed observations of the Solar System (the planets:
Jupiter, Saturn, Mars) and beyond to distant nebulae, star clusters, and
galaxies. The astrophotographer will find a virtually limitless range of
possibilities since, with the precision Meade worm-gear motor drive system,
long exposure guided photography becomes not a distant goal, but an achievable
reality. The capabilities of the instrument are essentially limited not
by the telescope, but by the acquired skills of the observer and photographer.
The 7", 8", 10", and 12" LX200 are, with the exception
of a few assembly operations and features, almost identical operationally.
Most standard and optional accessories are interchangeable between the
three telescopes. The instructions in this manual generally apply to all
three telescopes; when exceptions to this rule occur, they are clearly
pointed out.
IMPORTANT NOTE
If you are anxious to use your Meade LX200 Telescope for the first time,
at the very least be sure to read Telescope Assembly and Quick Start sections
of this manual. Thereafter, we urge you to read the balance of this manual
thoroughly at your leisure, in order that you may fully enjoy the many
features offered by the instrument.
1. What Is the LX200? An Overview
Meade LX200 SCT's mark a new era in telescope technology for the amateur
astronomer, whether beginner or seasoned veteran. For the beginner LX200
electronics permit the location and observation of the major planets as
well as hundreds of deep-sky objects the very first night you use the
telescope. For the experienced amateur the telescopes' pushbutton electric
slewing, digital readouts, Smart Drive, and much more open up visual and
photographic capabilities heretofore undreamed of.
a. Heavy-Duty Mounts with 9-speed Dual-Axis Electronics
DC-servo-motor-controlled worm gear drives on both telescope axes permit
observatory-level precision in tracking, guiding, and slewing. The 9-speed
dual-axis drives cover every possible contingency of telescope positioning:
Press the SLEW button on the keypad controller for rapid motion of the
telescope across the skies at up to 8 degrees per sec. (6 degrees per sec.
for the 12" LX200) on both axes simultaneously; once near the target,
switch instantly to the FIND speed for centering in the viewfinder at 2
degrees per sec. Observing the object in the main telescope, use the CNTR
speed (32x sidereal) to place the object in the center of the field. During
long-exposure astrophotography press the GUIDE button for precise corrections
at 2x sidereal speed.
b. Built-in 64,359-Object Library
Enter into the keypad any of the 110 Messier objects, 7,840 of the finest
NGC objects (galaxies, diffuse or planetary nebulae, star clusters), one
of the 8 major planets from Mercury to Pluto, one of 351 alignment stars
or any one of 56,050 SAO, UGC, IC or GCVS objects, press GO TO, and the
telescope automatically slews, or moves, to the object at up to 8°
per sec., centering it in the main telescope field.
c. Altazimuth Mode Operation
For all visual observing applications, and for lunar and planetary photography,
Meade LX200's may be set up in the Altazimuth mode. Just attach the telescope's
drive base directly to the tripod, use the fast 1-star alignment procedure,
and the telescope's computer actuates 2-axis tracking that keeps objects
precisely centered in the field, even at high powers, during the entire
observing session.
d. Terrestrial Operation
Meade LX200's make incredible land-view telescopes. Set the telescope up
in the Altazimuth format, activate the Land menu option on the telescope's
computer, and use the Keypad to track land objects on both axes at any
of the same 4 drive speeds!
e. Keypad and Power Panel Functions
The multifunction capability of LX200's includes direct connection of popular
CCD autoguider/imagers; RS- 232 serial interface with a personal computer
(PC), allowing the user to perform all of the Keypad functions through,
or write custom telescope software for a PC; brightness level control of
an illuminated reticle eyepiece from the Keypad and including special pulse-mode
reticle operation.
2. Standard Equipment
a. 7" Model LX200
lncludes 7" Maksutov-Cassegrain optical tube assembly with EMC super
multi-coatings (D = 178mm, F = 2670mm-f/15); heavy-duty fork mount, with
4"-dia. sealed polar ball bearing, quartz-microprocessor-controlled
5.75" worm gears on both axes; setting circles in RA and Dec; handheld
keypad Electronic Command Center with digital readout display, permanently-programmable
Smart Drive, 9-speed drive control on both axes, GO TO controller, High-Precision
Pointing, and 64,340-object onboard celestial software library; internal
tube-cooling fan for rapid image stabilization; 25 ft. power cord and adapter
for telescope operation from 115v.AC; 8 x 50mm viewfinder; eyepiece-holder
and diagonal prism (1.25"); Series 4000 SP26mm eyepiece; variable-height
field tripod; operating instructions.
b. 8" Model LX200
lncludes 8" Schmidt-Cassegrain optical tube assembly with EMC super
multi-coatings (D = 203mm, F = 1280mm-f/6.3 or 2000mm-f/10); heavy-duty
fork mount, with 4"-dia. sealed polar ball bearing, quartz-microprocessor-controlled
5.75" worm gears on both axes, and multi-function power panel display
on the drive base; manual and electric slow-motion controls on both axes;
setting circles in RA and Dec; handheld keypad Electronic Command Center
with digital readout display, PPEC Smart Drive, 9-speed drive control on
both axes, GO TO controller, High-Precision Pointing, and 64,340-object
onboard celestial software library; 25 ft. power cord and adapter for telescope
operation from 115v.AC; 8 x 50mm viewfinder; eyepiece-holder and diagonal
prism (1.25"); Series 4000 SP26mm eyepiece; variable-height field
tripod; operating instructions.
c. 10" Model LX200
lncludes 10" Schmidt-Cassegrain optical tube assembly with EMC super
multi-coatings (D = 254mm, F = 1600mm-f/6.3 or 2500mm-f/10); heavy-duty
fork mount, with 4"-dia. sealed polar ball bearing, quartz-microprocessor-controlled
5.75" worm gears on both axes, and multi-function power panel display
on the drive base; manual and electric slow-motion controls on both axes;
setting circles in RA and Dec; handheld keypad Electronic Command Center
with digital readout display, PPEC Smart Drive, 9-speed drive control on
both axes, GO TO controller, High-Precision Pointing, and 64,340-object
onboard celestial software library; 25 ft. power cord and adapter for telescope
operation from 115v.AC; 8 x 50mm viewfinder; eyepiece-holder and diagonal
prism (1.25"); Series 4000 SP26mm eyepiece; variable-height field
tripod; operating instructions.
d. 12" Model LX200
lncludes 12" Schmidt-Cassegrain optical tube assembly with EMC super
multi-coatings (D = 305mm, F = 3048mm-f/10); heavy-duty fork mount, with
4"-dia. sealed polar ball bearing, quartz-microprocessor-controlled
5.75" worm gears on both axes, and multi-function power panel display
on the drive base; manual and electric slow-motion controls on both axes;
setting circles in RA and Dec; handheld keypad Electronic Command Center
with digital readout display, PPEC Smart Drive, 7-speed drive control on
both axes, GO TO controller, High-Precision Pointing, and 64,340-object
onboard celestial software library; 25 ft. power cord and adapter for telescope
operation from 115v.AC; 8 x 50mm viewfinder; 2" diagonal mirror with
1.25" adapter; Series 4000 SP26mm eyepiece; giant field tripod; foam-fitted
carrying case; operating instructions.
B. UNPACKING AND INSPECTION
As you begin to unpack your telescope from its cartons, you will probably
be interested in setting it up right away; we certainly understand your
excitement but please take a few minutes to read this page before doing
so. You should verify that you have all the proper equipment, and that
it has arrived to you undamaged.
We strongly recommend that you keep your original packing materials.
If it should ever become necessary for you to return your telescope
to the Meade factory for servicing, these will help ensure that no shipping
damage will occur.
Meade LX200 telescopes supplied to countries outside the U.S.A. are identical
to those offered domestically, with the exception of the AC wall adapter.
1. What You Should Have
Carefully unpack and remove all the telescope parts from their packing
material. Compare each part to the Standard Equipment list on page 9. You
may wish to place a check next to each item as you identify it. These Packing
Programs represent the original specifications for this instrument. Each
telescope has been inspected twice at the factory to confirm the inclusion
of every item.
2. Please Look Everything Over
Meade Instruments and your shipper have taken precautions to ensure that
no shipping damage will occur, but if your shipment has suffered severe
vibration or impact damage (whether or not the shipping cartons show damage)
then it is important that you retain all the original packing and contact
the shipper to arrange a formal inspection of the package or packages.
This procedure is required prior to any warranty servicing by Meade Instruments.
3. Inspecting the Optics: Note on the "Flashlight" Test
If a flashlight or other high-intensity light source is pointed down the
main telescope tube, you may at first be shocked at the appearance of the
optics. To the uninitiated, the view (depending on your line of sight and
the angle the light is coming from) may reveal what would appear to be
scratches, dark or bright spots, or just generally uneven coatings, giving
the appearance of poor surface quality. 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
the giant research telescopes in use today. It should be pointed out, however,
that optical quality cannot be judged by this grossly misleading "test",
but through careful star testing. The Flashlight Test causes even the very
best optics to look "terrible."
As the high intensity light passes through the Schmidt corrector plate,
most of it is transmitted through (about 98%+) while the rest of the light
scatters through the glass. As the light hits the mirrored surfaces, most
of it is reflected back (about 94%) while the rest of it scatters across
the coatings. The total amount of scattered light will be significant,
and its effects allow you to see microscopic details that are normally
invisible to the unaided eye. These anomalous details are real, but their
combined effects will in no way impose limits on the optical performance,
even under the most demanding observing or imaging criteria.

Figure 3: 8" LX200 Telescope
Figure 4: LX200 Declination (Vertical) System

4. Caution: All LX200 Owners
Serious damage to the drive gears may result from shock in handling, while
transporting or commercially shipping the LX200, should the R.A. Lock (7,
Fig. 3), and/or the Dec. Lock (2, Fig. 4) be left engaged. Always release
the locks when storing in the case, or when crating for commercial shipment
to allow the telescope to give, if the case or crate is sharply jarred
or dropped.
Also, the optical and mechanical axes of all LX200 telescopes have been
carefully aligned at the factory to ensure accurate object pointing. Do
not loosen or remove the fork arms or optical tube assembly from the drive
base; the resulting misalignment of the axes will result in inaccurate
slewing of the telescope in the GOTO mode.
5. Caution: 10" and 12" LX200 Owners
Do not attempt to turn the focuser knob of the optical tube until you have
read this note!
Next to the base of the focuser you will see a red-colored slotted head
bolt. This bolt is used only for safety in shipment. Remove this bolt before
attempting to turn the focuser knob. In its place, insert the rubber plug
provided as a dust protector (this rubber plug is included with your hardware
package).
Your focuser is now operational.
Warning! The 10" and 12" LX200 should never be commercially
shipped without this red-colored bolt in place. This is essential during
commercial transport where rough handling may occur. For your personal
transport and storage, you will never have to use this bolt again.
a. TO COMMERCIALLY RE-SHIP THE 10" OR 12" LX200, BE SURE TO FOLLOW
THIS PROCEDURE:
1. Turn the focuser knob clockwise until it stops. This will bring the
primary mirror all the way back in the tube.
2. Remove the rubber plug and insert the red-headed bolt. Thread it in
to a firm snug feel. Do not overtighten. (If you have misplaced the red-headed
bolt, you may use any other bolt that is 1/4-20x1" long.
3. When packaging the 10" or 12" LX200, be sure to release
the R.A. Lock (7, Fig. 3), and Dec. Lock (2, Fig. 3), to prevent shock
to the gears in the motor assemblies should the package suffer severe handling.
Please note that commercial shipment of the 10" and 12" LX200
Telescope without the safety bolt in place and packed in the original factory
supplied shipping containers as described above is done at the owner's
risk and your warranty may be voided if shipping damage results.
6. Keypad Version Number
The current keypad version is 3.20 (see sticker on back of keypad). This
does not indicate the telescope software versionwhich is displayed on the
keypad LED at power-up.
C. TELESCOPE ASSEMBLY
Use the following steps to assemble your telescope. Note: Section headings
list which LX200 model (7", 8", 10" or 12") is covered
under that heading.
Figure 1: Field Tripod

Figure 2: Field tripod
(Collapsed)
1. The Field Tripod (7", 8", 10" and 12" LX200
Models)
The Field Tripods (Figs. 1 and 2) for Meade 8", 10", and 12"
LX200 telescopes are supplied as completely assembled units, except for
the spreader bar (4, Fig. 1) and the 6 lock knobs (2 knobs for each of
the 3 tripod legs) used to adjust the height of the tripod. These knobs
are packed separately for safety in shipment.
For visual (i.e. non-photographic) observations, the drive base
(17, Fig. 3) of the telescope's fork mount is attached
directly to the field tripod. The telescope in this way is mounted in an
"Altazimuth" ("Altitude-Azimuth," or "vertical-horizontal")
format. The telescope in this configuration moves along vertical and horizontal
axes, corresponding respectively to the Declination and Right Ascension
axes (explained later in this manual) in an astronomical observing mode.
Alternately, the field tripod can be used in conjunction with the appropriate
optional equatorial wedge (see Appendix A for instructions of the use of
the equatorial wedge) for long exposure astrophotography. The equatorial
wedge permits alignment of the telescope's Polar Axis with the Celestial
Pole (or North Star).
After removing the field tripod from its shipping carton, stand the
tripod vertically, with the tripod feet down and with the tripod still
fully collapsed (see Fig. 2). 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.
Thread in the 6 lock-knobs (2 on each tripod leg) near the foot of each
tripod leg. Refer to Fig. 1. These lock-knobs are used to fix the height
of the inner, extendible tripod leg sections. Note: "Firm
feel" tightening is sufficient; over-tightening may result in stripping
of the knob threads or damage to the tripod legs and results in no additional
strength.
The spreader bar (4, Fig. 1) has been removed for shipment. To replace,
first remove the threaded rod (2, Fig. 1) from the tripod head (1, Fig.
1); a small piece of plastic holds the threaded rod in place. Remove the
small plastic bag that is stapled to the threaded rod. This bag contains
the "C" clip retainer (used below) and an extra clip.
Slide the spreader bar onto the threaded rod (note the correct orientation
as shown in Fig. 1) and position the threaded rod back through the tripod
head. Place the clip retainer ( a "C" clip) into the slot in
the threaded rod. This clip holds the threaded rod in place. See Fig. 2.
Position the spreader bar so that the 3 arms of the spreader bar are lined
up with the 3 tripod legs.
Place the entire telescope (as shown in Fig. 3) onto the top of the tripod
head, and thread the threaded rod into the central threaded hole in the
bottom of the drive base of the telescope. Tighten the tension knob (3,
Fig. 1); firm tightening of the tension knob is sufficient to result in
rigid positioning of the tripod legs.
To vary the tripod height, loosen the 6 lock-knobs, slide the 3 inner tripod
leg sections out to the desired height, and firmly re-tighten (but do not
overtighten) the 6 lock-knobs.
To collapse the tripod (after removing the telescope and equatorial wedge,
if applicable) for storage follow these steps:
1. Rotate the spreader bar 60° from its assembled position, so that
one spreader bar arm is located between each adjacent pair of tripod legs.
2. At the base of the tripod is a 3-vane extension strut system, with a
circular hub at its center (7, Fig. 1). Grasp the tripod head (1, Fig.
1) with one hand and, with the other hand, pull directly "up"
on the central hub of the extension strut system. This operation will cause
the tripod legs to move inward to a collapsed position.
PRECAUTIONARY NOTES
1. If the tripod does not seem to extend or collapse easily, do not
force the tripod legs in or out. By following the instructions above, the
tripod will function properly, but if you are unclear on the proper procedure,
forcing the tripod into an incorrect position may damage the extension
strut system.
2. Do not overtighten the 6 lock-knobs used to fix the inner tripod leg
sections at various heights. "Firm feel" tightening is sufficient.
3. Be sure the spreader bar (4, Fig. 1) is not upside-down on the threaded
rod.
2. Mounting the Viewfinder (7", 8", 10", and 12"
LX200 Models)
Each 7", 8", 10", and 12" LX200 telescope is supplied
as standard equipment with an 8x50mm straight-through viewfinder. The bracket
for this viewfinder is packed separately from the finder itself, and 6
black nylon thumbscrews for collimation are pre-threaded into the viewfinder
bracket. The viewfinder bracket mounts onto the telescope with a quick-release
mount. See Fig. 3.
a. Attaching the Viewfinder
The viewfinder is shipped separately from the bracket and must be installed
into the bracket. Slide the viewfinder into the bracket and lightly tighten
the 6 collimation (alignment) screws (2, Fig. 3).
The quick-release mount allows the viewfinder to be easily attached or
removed from the telescope. To attach the unit, simply slide the viewfinder
with bracket into the mating base on the telescope and tighten the two
thumbscrews.
b. Focusing the Viewfinder
The viewfinder has been pre-focused at the factory. However, should it
become necessary to adjust the focus, follow these steps:
1. Loosen the Focus Lock Ring (18, Fig. 3).
2. While looking at a star, rotate the Dew Shield (1, Fig. 3) until the
star is in focus. (This refocuses the objective lens.) CAUTION! Take
care when rotating counter clockwise. You are unthreading the dew shield
and it may fall off if rotated too far. Refocusing the objective lens will
only require a few turns of the Dew Shield at most.
3. When the Dew Shield is rotated to the sharpest focus for your eye, tighten
the Focus Lock Ring against the Dew Shield to fix its position.
c. Collimating the Viewfinder
The viewfinder will require alignment, or collimation, with the main telescope.
Using the 26mm eyepiece, point the main telescope at some easy to find
land object (e.g. the top of a telephone pole or corner of a building)
at least 200 yards distant. Center a well-defined object in the main telescope.
Then, simply turn the 6 nylon collimation thumbscrews (2, Fig. 3) until
the crosshairs of the viewfinder are precisely centered on the object already
centered in the main telescope. With this collimation accomplished, objects
located first in the wide-field viewfinder will then be centered in the
main telescope's field of view.
3. Attaching the Diagonal Prism and Eyepiece
The eyepiece holder (6, Fig. 3) threads directly onto the rear-cell thread
of the 8" and 10" telescopes. The diagonal prism (13, Fig. 3)
slides into the eyepiece holder of the 7", 8" and 10" telescopes,
while the 2" diagonal mirror threads directly into the rear-cell thread
of the 12" telescope. In turn, both the diagonal prism and diagonal
mirror accept the supplied 1 1/4" O.D. eyepiece.
For astronomical observations, the diagonal prism or mirror generally provides
a more comfortable right-angle viewing position. Alternately, in the 8"
and 10" telescopes, an eyepiece may be inserted directly into the
eyepiece holder for straight-through observations, the 12" telescope
requires the accessory eyepiece holder. Note in this case, however, that
the image will appear inverted and reversed left-for-right. With the diagonal
prism and mirror, telescopic images appear correctly oriented up-and-down,
but still reversed left-for-right. For terrestrial applications, where
a fully corrected image orientation is desired, both up-and-down and left-for-right,
the optional #924 Erecting Prism* or #928 45° Erect-Image Diagonal
Prism* should be ordered separately. Eyepieces and the diagonal prism are
held in their respective places on the telescope by a moderate tightening
of the thumbscrews on the diagonal prism and eyepiece holder.
4. Checking the Collimation of the Optics
The optical systems of all Meade Schmidt-Cassegrains are precisely collimated,
or aligned, before leaving the factory. However, if the telescope has received
a severe jolt in shipment the optics can become de-collimated, a situation
which may result in serious image degradation. Recollimating the optics
is, however, a simple procedure which is easily performed by the telescope
user. We urge all LX200 owners to confirm the collimation of their telescope,
and to recollimate the optics if necessary.
There is no collimation procedure required for the Meade 7" Maksutov-Cassegrain
telescope. Factory alignment assures optimal viewing accuracies.
5. 12" Tube Swing-Through Limit
The length of the 12" LX200 optical tube prohibits the correcting
plate end of the tube from swinging through the fork armsthe tube will
hit the mount. When the telescope is aligned, the software will stop the
telescope from moving into the mount. If the telescope is not aligned,
there are also mechanical stops.
When in LAND or ALTAZ modes, this limit does not restrict any sections
of the sky, since the limit is set at 45° from straight down. But when
in the POLAR mode, some parts of the sky might be restricted, depending
on the latitude of the observing site.
Observing sites with latitudes higher than 45° will not have any restrictions.
Latitudes below 45° will have the southern horizon restricted somewhat.
To determine the amount of sky not available, subtract the latitude of
the observing site from 45. This will give the number of degrees of southern
horizon that the 12" LX200 will not move to. For example, if the latitude
of the observing site is 35°, then 10° (45-35) of southern sky
is unavailable for observations.
6. 7" Tube Swing-Through Limit
The length of the 7" LX200 optical tube prohibits the correcting plate
end of the tube from swinging through the fork arms--the tube will hit
the mount. When the telescope is aligned, the software will stop the telescope
from moving into the mount. If the telescope is not aligned, there are
also mechanical stops and some parts of the sky might be restricted if
using a wedge, depending on the latitude of the observing site.
Observing sites with latitudes higher than 45° will not have any restrictions.
Latitudes below 45° will have the southern horizon somewhat restricted
when using a wedge and polar aligning. To determine the amount of sky not
available, subtract the latitude of the observing site from 45, this will
give the number of degrees of the southern horizon that the 7" LX50
will not reach. For example, if the latitude of the observing site is 35°,
then 10° (45 35) of southern sky is unavailable for observations. No
restrictions of observable sky occur in the altaz mode of alignment and
operation.
7. Maksutov Fan
The Maksutov optics are equipped with a fan which will assist in the stabilization
of the temperature of these optics. The fan will operate when a special
power cord (supplied in the accessory box) is plugged into the fan and
the LX50 panel plug marked "Aux" with the power switch in the
"on" position. The amount of time required to stabilize the temperature
will be dependent upon ambient conditions including the observation site
and preexisting condition of the telescope. The fan should be activated
at the beginning of the observation session to accelerate the temperature
stabilization. As soon as the optics have reached an equilibrium with the
environment the fan should be turned off by unplugging the fan power cord.
Fan operation time should range between 5 and 25 minutes. While it is permissible
to run the fan continuously it is not recommended because the very slight
vibration of the fan may cause noticeable movement of the objects observed
in the sensitive optics.
D. QUICK START
To utilize all the features of the telescope, it is necessary to enter
some information into the telescope's computer memory, and learn the menu
structure of the Keypad hand controller, which is described in the rest
of this manual. As advanced as LX200 electronics are, the telescope is
very straightforward to operateeven if you have no experience whatsoever
in using a personal computer.
If you are reading this manual for the first time and are anxious to "look
through the telescope", this section will describe how to use the
telescope without going through the rest of the manual. But be sure to
come back and read the details, for most of the telescope's features can
not be accessed without a full knowledge of these details.
1. Using the LX200 Manually
The easiest way to use the telescope is to simply operate it manually.
With the telescope mounted on the Field Tripod, and with the diagonal prism
and eyepiece in place, you are ready to make observations through the telescope.
Even without the viewfinder (if not yet installed), terrestrial objects
will be fairly easy to locate and center in the telescope's field of view
with a low power eyepiece, simply by "gun sighting" along the
side of the main telescope tube.
By unlocking the R.A. Lock (7, Fig. 3), the telescope
may be turned rapidly through wide angles in Right Ascension (R.A.). The
reason for the terminology "Right Ascension" and its complementary
term, "Declination" will be made clear further on in this manual.
For now, "Right Ascension" simply means "horizontal"
and "Declination" means "vertical". Fine adjustments
in R.A. are made by turning the R.A. Slow-Motion Control Knob (8, Fig.
3), while the R.A. lock is in the "unlocked" position.
DO NOT ATTEMPT TO MOVE THE TELESCOPE MANUALLY IN A HORIZONTAL DIRECTION
WHEN THE R.A. LOCK IS IN THE "LOCKED" POSITION.
Figure 4: LX200 Declination (Vertical)
System
The R.A. Slow-Motion Control Knob may be turned, if desired, with the
R.A. Lock in a "partially locked" position. In this way, a comfortable
"drag" in R.A. is created. But do not attempt to operate
the R.A. Slow-Motion Control Knob with the telescope fully locked in R.A.,
as such operation may result in damage to the internal gear system.
Releasing the Declination Lock Knob (2, Fig. 4), permits sweeping the telescope
rapidly through wide angles in Declination.
To use the Declination fine-adjust, or Manual Slow-Motion Knob, lock the
telescope in Declination using the Declination Lock Knob (2, Fig. 4), and
turn the Declination Slow-Motion Knob (1, Fig. 4).
With the above mechanical operations in mind, select an easy to find terrestrial
object as your first telescope subject -- for example, a house or building
perhaps one-half mile distant.
Unlock the Declination Lock Knob (2, Fig. 4), and R.A. Lock (7, Fig. 3),
center the object in the telescopic field of view and then re-lock the
Dec. and R.A. locks. Precise image centering is accomplished by using the
Dec. and R.A. slow motion controls.
The Focus Knob (5, Fig. 3) is located at the "4 o'clock" position
as you face the rear cell of the telescope. Focusing is accomplished internally
by a precise motion of the telescope primary mirror so that, as you turn
the focus knob, there are no externally moving parts. You will find that
if you turn the focus knob counter-clockwise you are focusing towards the
infinity setting, and turning clockwise is for close distance. There are
about 45 complete turns to go from one end of focus to the other, and it
is possible to focus past infinity. Be patient during focusing as images
quickly go in and out of focus with only a slight amount of turning of
the focus knob.
Before using the telescope manually during the daytime, be sure to read
"Daytime Slewing."
2. Using the LX200 In Land
The 7", 8", 10", and 12" LX200 telescopes are shipped
with the microprocessor set to Land, the align menu option you will wish
to use to view terrestrial objects. In this menu option 4 different motion
speeds are active, allowing the telescope to be moved electronically by
means of the Keypad. To use the telescope in Land, follow these
steps.
1. Loosen the Dec. Lock Knob (2, Fig. 4) and position the optical tube
assembly approximately level, so that the Dec. Circle (3, Fig. 3) reads
0°. Retighten the Dec. Lock Knob.
2. Loosen the R.A. Lock (7, Fig. 3) and rotate the telescope so that the
R.A. Pointer (9, Fig. 3) and the Hour Angle (HA) Pointer (16, Fig. 3) are
approximately in line with each other. This will position the fork arms
so that they are parallel to the Power Panel (11, Fig. 3). Tighten the
R.A. lock
The above two steps are not necessary for the telescope to work, so don't
worry about having to get it exactly right. The telescope has some "illegal"
positions, places where the telescope will not go and these two steps insure
proper operation.
3. After setting up the telescope, plug in both coil cords with the Keypad,
one of the supplied power sources, either the AC Wall Adapter Power Converter
(for AC current wall outlets), or the optional DC Cigarette Lighter Power
Cord (used in an automobile's cigarette lighter outlet, with the ignition
turned on only to allow the electric power on from the car battery).
Figure 5: LX200 Keypad
Hand Controller 
Motion Speeds
GUIDE = 30 arcsec/sec, CNTR = 480 arcsec/sec, FIND = 2°/sec, SLEW =
8°/sec (8", 10"), = 6°/sec (12")
4. Turn on the power switch on the Power Panel of the LX200. The Keypad
Display (1, Fig. 5) will show "MEADE" for several seconds as
the microprocessor does a self-diagnostic test. When the self-diagnostic
test is complete, the display will show "TELESCOPE" on the top
line, "OBJECT LIBRARY" on the lower line, and the red LED light
next to the "SLEW" button will light up.
5. At this point, the LX200 is ready to use. Select the speed at which
you want to move the telescope by pressing the appropriate Speed Selection
Key (4, Fig. 5). Note that you will be able to "see" the telescope
move only in the SLEW and FIND modes; CNTR (center) and GUIDE motions can
only be seen while looking through the telescope. The red LED next to that
key (3, Fig. 5) will light, indicating the speed selected. Then press one
of the four direction keys (2, Fig. 5) to move the telescope in that direction
at the selected speed.
The LX200 can also be moved manually with the R.A. and Dec. locks released,
or as described above only. The Declination Manual Slow-Motion Knob (1,
Fig.4) is non-functional when power is supplied
to the telescope. When the power is "on", only use the N, S,
E, and W keys on the Keypad Hand Controller. Serious damage can occur
to the internal gears of the motor assembly if the Declination Manual Slow-Motion
Knob is turned even a slight amount by hand.
Before using the telescope during the daytime, be sure to read "Daytime
Slewing."
3. Using the LX200 In Altazimuth (ALTAZ)
The two quick start methods described above allow you to use the telescope,
but do not make use of any of the computer features available, including
finding objects from the Object Library and automatic tracking of stars.
In order for these features to work, the telescope's power needs to be
"on", and the computer needs some basic information, which is
entered through the Keypad. Once entered, the information is permanently
remembered by the telescope's computer and need never be entered again,
even if the telescope is turned "on" and "off" many
times.
This section will explain what keys to push to get the minimum data required
into the computer, without any detailed explanation. Later, see Section
G, LX200 Modes for detailed instructions. These steps will only take a
few minutes and will allow you to begin making use of all the LX200 features.
Note also, much of this information can be skipped if using the UNKNOWN
site.
a. Entering Basic Information
In order for the LX200 to make the conversions between the stellar coordinate
system (R.A. and Declination) and the Altazimuth coordinate system (Altitude
and Azimuth), it needs to know three pieces of information. This information
only needs to be entered one time--the LX200 remembers the data even when
the power is off.
Displays 1-7
1) Latitude and Longitude of the Observing Site.
NOTE: The SITE information cannot be entered if the telescope is in LAND
mode. If the telescope is in LAND mode, the SITE menu option (Display
2, below) will appear in lower case letters. Follow steps 4-8 to change
the telescope's operation to Altazimuth (ALTAZ) mode before proceeding.
You should find the position of your observing site to within 1 or 2 minutes
of arc in both latitude and longitude. Many automobile, pilot, and topographical
maps, as well as most atlases show latitude and longitude in 15 minute
increments or better. The accuracy of the LX200 will depend on how close
you get, so take a little time to get as accurate as you can.
Once the above information is determined, it can be entered into the telescope.
It is easiest to enter the data with the telescope sitting on a table indoorsdo
not try to do it outside at night.
Each step below is given without any details or explanations to keep the
process as simple and fast as possible. Next to each step will also be
a sample of what the Keypad Hand Controller display (1, Fig. 5) should
look like after each step.
As an example, we will enter the data for Costa Mesa, CA (LAT=33°35',
LONG=117°42'). If at any time you get "lost," simply turn
off the telescope and restart this procedure.
1. Turn the telescope on. After a few seconds (after the self-diagnostic
test is complete), the display will look like Display 1.
2. Press the ENTER key. This selects the TELESCOPE functions. The display
should look like Display 2.
3. Press the ENTER key. This selects the SITE functions. The display should
look like Display 3.
4. Press and Hold the ENTER key until the Keypad Hand Controller
beeps. This selects the first site for editing. The display should look
like Display 4, with the first "A" flashing.
5. Press the ENTER key. The display should look like Display 5.
6. Use the number keys to enter your Latitude. The underline designates
the current cursor position. Mistakes can be corrected by moving back (using
the "E" and "W" keys). A negative latitude can be entered
by positioning the cursor under the "+" and hitting the "NEXT"
key (lower right-hand key). When the Latitude is correct, press ENTER.
The display will look like Display 6.
7. Use the number keys to enter your Longitude as above. When complete,
the display will look like Display 7.
8. Press ENTER to complete the site information input. The display will
go back to Display 3.
9. Press MODE to go back to Display 2.
10. Press MODE again to go back to Display 1.
It is important to note that the longitude standard used in the LX200 starts
at 0 degrees in Greenwich U.K. and increases Westerly only to 359 degrees
59 minutes. Many maps will show Easterly longitudes which cannot be entered
into the Keypad Display. As an example, if your map indicates that you
are at an Easterly longitude of 18 degrees 27 minutes, then you would enter
341 degrees 33 minutes.
Do not concern yourself with differences in longitude and latitude as they
pertain to different map spheroid projections, those minor differences
are too small to adversely affect the longitude and latitude data input.
Displays 8-11
2) Local Time and Date.
The local time should be set as accurately as possible, using the 24
hour format. The local time and date are used to determine sidereal time
(star time) and the pointing accuracy of the telescope will depend on the
accuracy of the time entered. Choose a reliable source as a reference for
accurate time such as your local airport, or telephone company. In the
U.S.A. you can double check the accuracy of the exact minutes by dialing
WWV for the universal coordinated time at (303) 499-7111 (be sure to enter
your local time hour information, not the U.T. hour). For the example,
we will use 4:25:00 P.M. on Jan. 15, 1992.
1. The display should look like Display 1. If it does not, press the MODE
key until it does.
2. Press the MODE key twice. The display will look like Display 8, but
with a random LOCAL and SIDE times.
3. Press and HOLD the ENTER key until the Keypad Hand Controller beeps
(display like Display 9).
4. Using the number keys, enter the current local time to within 5 seconds.
(Remember, 4:25:00 P.M. is 16:25:00 in the 24 hour format.) Corrections
can be made by moving the flashing cursor using the W and E keys. The display
should look like Display 10.
5. Press the ENTER key when the time is correct. The display will change
to Display 11.
The next step is to enter the Greenwich Mean Time (GMT) time zone shift.
(This procedure is a lot easier than it sounds.) Simply look up your time
zone in the table below to find the GMT time zone shift.
Table 1: U.S.A. Time Zones

Use the top row during Standard Time and the bottom row during
Daylight Savings Time.
For example: You live in the Pacific Time Zone and you are on Daylight
Savings Time. The GMT time zone shift is +7 hours.
6. Use the number keys to enter the GMT time zone shift determined from
the table above. Press ENTER when done; the display will go back to Display
8. If you are using the LX200 East of Greenwich U.K., then you must enter
a - (minus) GMT time zone shift by moving the blinking cursor backwards
in the display with the W key and then pressing the NEXT key. The + (plus)
sign will change to - (minus). Use the number keys to enter the Westerly
(+) GMT time zone shift determined from the table above or your calculated
Easterly (-) time zone shift.
Displays 12-14 
7. Press the ENTER key. This will select the DATE display (Display 12),
with a random date showing.
8. Press and Hold the ENTER key until the Keypad Hand Controller
beeps. The display will look like Display 13, with the blinking cursor
over the first number.
9. Use the number keys to enter the current date. The display should look
like Display 14. Use the W and E keys to move the blinking cursor left
and right to correct any mistakes.
10. Press the ENTER key when the date is correct.
After you press the ENTER key, the Keypad Hand Controller will display
"Updating planetary data". The position of the planets
depends on the date, so anytime the date is changed, the planet positions
are recalculated.
This is all the information the LX200 needs to make use of all features.
The next steps actually align the telescope with the night sky.
Figure 3: 8" LX200 Telescope
Figure 4: LX200 Declination (Vertical)
System
b. Setting Up the Telescope
After the basic information has been entered into the telescope, the telescope
is ready to actually set-up and use. Follow Section A: Telescope Assembly
to setup the telescope outside, and follow these steps:
1. Using the Bubble Level (15, Fig. 3) located on the telescope's drive
base, level the telescope. Position the drive base so that the power panel
faces North (i.e. to view the power panel, you must face South.)
2. Loosen the Dec. Lock Knob (2, Fig. 4 ) and position the optical tube
assembly approximately level (so that the Dec. Circle (3, Fig. 3) reads
0°. Retighten the Dec. Lock Knob.
3. Loosen the R.A. Lock (7 Fig. 3) and rotate the telescope so that the
R.A. Pointer (9, Fig. 3) and the Hour Angle (HA) Pointer (16, Fig. 3) are
approximately in line with each other. This will position the fork arms
so that they are parallel to the Power Panel (11, Fig. 3). Lock the R.A.
lock.
Displays 15-25 
Steps 2 and 3 above, are not necessary for the telescope to work, so
don't worry about having to get it exactly right. The telescope has some
"illegal" positions (places where the telescope will not go)
and these two steps ensure proper operation.
4. Turn the telescope on. After a few seconds (after the self-diagnostic
test is complete), the display will look like Display 15.
5. Press the ENTER key. This selects the TELESCOPE functions. The display
should look like Display 16.
6. Press the NEXT key. This will move the arrow to the lower line (see
Display 17).
7. Press the ENTER key to select the ALIGN function. The display will look
like Display 18. (If the display looks like Display 19 - with a checkmark
already next to ALTAZ, go to step 9.)
8. Press the ENTER key to activate the ALTAZ mode. The Keypad Hand Controller
will beep and display a checkmark next to the ALTAZ (see Display 19).
9. Press the ENTER key to use the checked mode (ALTAZ). The Keypad Hand
Controller display will look like Display 20.
10. If you have not already leveled the telescope, do so now. When the
telescope is level, select 1 STAR or 2 STAR alignment. The display will
look like Display 21.
11. This message simply reminds you what you should do next. Press ENTER
to show a display like Display 22.
12. Using the monthly star charts in Appendix C, pick an alignment star.
Look at the chart for the current month and face the direction indicated.
The constellations shown are easily found -- even in the city. The charts
are approximately 90 degrees wide, with the top of the chart indicating
straight up. If the time is after 9:00 P.M., then use the next month's
chart. Once you identify the constellation, pick any of the labeled stars
that is not within a 10 degree radius of overhead, but do not choose Polaris,
for reasons made clear below. Polaris is also known as the North Star,
and is shown for reference only.
The TELESCOPE and OBJECT LIBRARY features are accessed through a series
of menus, which are shown on the Keypad Hand Controller Display. You can
scroll up or down through the list of choices by using the PREV and NEXT
keys, and select the indicated menu option with the ENTER key. Menu choices
that are shown in lower case letters are unavailable in the current operating
mode (LAND, ALTAZ, or POLAR). If you try to select a lower case menu option,
the Keypad Hand Controller will emit three warning beeps. Three beeps always
indicate an attempt to perform an invalid telescope operation.
When aligning in ALTAZ, overhead stars can confuse the LX200 because
of an illegal position that prevents the optical tube assembly from slewing
past 90 degrees Altitude to protect the viewfinder from hitting the fork
arm. The LX200 will track an overhead object, but it does so by moving
higher in Altitude up to the illegal position, then the drive speeds up
and move 180 degrees in Azimuth so that the optical tube assembly can now
be lowered in Altitude to keep up with the overhead object. Confusion arises
because the LX200 does not know which side of 180 degrees of Azimuth that
it is on. Similarly, Polaris presents position problems in ALTAZ alignment
because it is so close to the North Celestial Pole. In this region of the
sky, the lines of Right Ascension are so close together that even the LX200's
high-resolution encoders can yield ambiguous data.
In our example of January 15, we would use the January chart, face Southeast
and look up about 45 degrees. Orion is probably the easiest constellation
to recognize, and we will use the star Betelgeuse for our example. Use
the PREV and NEXT key to scroll through the list of alignment stars until
the arrow is positioned on Betelgeuse (Display 23).
13. Press the ENTER key to select Betelgeuse. The Keypad Hand Controller
displays a message (Display 24).
14. Center the alignment star (Betelgeuse in our example) in the eyepiece
of the telescope. You can manually move the telescope by loosening the
Dec. Lock Knob and R.A. Lock or electrically by using the N, S, W, and
E keys. If moving the telescope electrically, be sure to use the speed
keys, SLEW to get close, FIND to center in the viewfinder, and CNTR to
center the star in the eyepiece. When the star is centered, press ENTER.
The telescope is now aligned and fully functional, and will automatically
begin to track objects. From this point on, make all telescope movements
by use of the Keypad Hand Controller. Manual movements by loosening the
Dec. or R.A. locks will cause the LX200 to "lose" position, requiring
realignment.
c. Using the Telescope
1) The MODE Key
The LX200 has 5 basic Keypad Hand Controller displays, and the MODE key
is used to move between them. The 5 modes are:
1. Telescope Functions. The TELESCOPE mode is where all telescope functions
are changed or activated and the OBJECT LIBRARY is where the features of
the object library are accessed.
2. Telescope Position. The first display shows the RA and DEC (telescope
position in stellar coordinates) and the second display (accessed by pressing
the ENTER key) shows the telescope position in ALTAZ coordinates.
3. Time and Date. The first display shows local time and Sidereal time
and the second display (accessed by pressing the ENTER key) shows the date.
4. Timer and Freq. This display is a countdown timer and allows the user
to change drive rates. These are advanced features.
5. All Off. This mode simply turns off all displays and backlighting. You
can also adjust the backlighting brightness by pressing the ENTER key and
using the PREV and NEXT keys to adjust the brightness.
2) Library Object Keys
While in any of the 5 main Keypad displays, you can directly access the
library objects by using the M, STAR, or CNGC keys (see Appendix D of this
manual for a listing of the 64,359 Object Library). Simply press an object
key, and type in the number of the object desired, followed by ENTER. For
example, a good first object for the first part of the year is M42--the
Great Orion Nebula. Press: the M key, the 4 key, the 2 key, and finally
the ENTER key. The display will show data on the object (name, rating,
object type, brightness, and size). Now press GO TO. The telescope will
automatically slew to M42.
If the object entered is not above the horizon, the Keypad Hand Controller
will display the message "OBJECT BELOW HORIZON."
Other good first objects (if above the horizon) are any of the M objectsfrom
M1 to M 110, and the planets. To find a planet enter:
Table 2: Object Library Planet
Legend

If the planet is too close to the Sun for safe viewing (closer than
15 degrees) the Keypad will display a message to that effect.
3) Daytime Slewing
Some amateurs may want to use the slewing feature of the LX200 to locate
the planets or other astronomical objects during the daytime. If not
done correctly, this can be very dangerous.
The LX200 "knows" where the planets are in relation to the
Sun, but the telescope does not "know" where the Sun actually
is. When the GO TO button is pushed, the telescope will slew to the object
by the most direct route, which may move directly over the Sun. Use extreme
caution before using the GO TO feature of the telescope to locate objects
in the daytime! Looking into the telescope or viewfinder, even for the
shortest fraction of a second, with sunlight entering the optics, will
cause instant and irreversible eye damage. The telescope itself may also
suffer serious damage if it is pointed at or near the Sun.
A responsible adult should supervise every aspect of telescope operation
when children are observing in the daytime.
Use the following procedure to safely locate objects during the daytime,
whether by manual slewing, using the N,E,W,S keys, or using the GO TO key:
1. Before allowing the telescope to move, place the dust covers on the
main telescope and viewfinder (or remove the viewfinder from the telescope
completely). This will keep the Sun's damaging light out of the telescope
should it move across the Sun.
2. Press the GO TO button or manually move the telescope.
3. After the telescope has stopped moving, visually check the telescope's
position to be sure it is not pointing near the Sun. If there is any question
in your mind that the telescope may be pointing at or near the Sun, do
not look through the telescope.
4. Only when you are absolutely convinced that the telescope is pointing
away from the Sun should you remove the telescope's dust cover and observe
the object.
5. Above all, be careful and use common sense. Observing the Sun,
even for the shortest fraction of a second, will cause instant and irreversible
eye damage.
Copyright © 1996 Meade Instruments Corporation, All Rights
Reserved.
Brought to you in night vision red by BlackLine Design
Meade Lx200 manual page 1