Autostar II Hand Controller TECHNICAL MANUAL FOR TELESCOPE ASSEMBLY AND OPERATING PROCEDURES Copyright Meade Instruments, 2003 All Rights Reserved / 73 Pages Provided on line as a courtesy to our customers by Company Seven Showroom: 14300 Cherry Lane Court Laurel, Maryland 20707 U.S.A.
Primary Mirror In the Schmidt-Cassegrain design of the Meade 8", 10", 12", 14", and 16" LX200GPS models, 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.
APPENDIX G page 66, for features unique to the 14" model. ® The name "Meade" and the Meade logo are trademarks registered with the U.S. Patent Office and in principal coun- tries throughout the world. "LX200GPS" and "Autostar II" are trademarks of Meade Instruments Corporation.
Take the from its packaging and place LX200GPS the entire telescope onto the top of the tripod head, inserting the threaded rod into the central hole in the bottom of the drive base of the tele- scope. Tighten the tension knob (see above fig- ure) to a firm feel only;...
Autostar II handbox. Attach microfocuser: Remove the dust cap from the rear cell port (A) of the telescope (Note: Telescope not shown for clarity). Thread the micro- focuser adapter (B) into the rear cell port thread.
OFF. The red power indicator LED next to the switch illuminates when power is supplied to the Autostar II handbox, the microfocuser, and to the telescope’s motor drives (the LED can be turned off in the Panel Light menu; see page 27).
G. RS232 Ports (2): Provides connection with a PC and for current and future Meade accessories. Your PC can control your scope using serial commands. Go to the Meade website (www.meade.com) to download the latest serial commands and device pinouts.
Download the Want to learn more about latest satellite data, star and object catalogs, tours, serial commands list, and soft- downloading the latest ware revisions, directly from the Meade website (www.meade.com). (Requires the updates of Autostar II software from the optional...
"spiral search." Arrow Keys: The Arrow keys have several functions. Press an Arrow key to slew the telescope in a specific direction (up, down, left, and right), at any one of nine different speeds. See SLEW SPEEDS to move the telescope vertically up and down.
Autostar II handbox. Coil Cord: Plug one end of the Autostar II coil cord into the HBX port (13F, Fig. 1) of the computer control panel of the telescope and the other end into the Autostar II coil cord port. See above.
Place the entire telescope onto the top of the tripod head, and insert the thread- ed rod into the central hole in the bottom of the drive base of the telescope. Tighten the tension knob (Fig. 4); firm tightening of the tension knob is sufficient to result in rigid positioning of the tripod legs.
Fig. 6: Microfocuser and eyepiece assembly. (A) Rear cell of telescope (shown separate from the telescope assembly for the sake of clarity, see 5, Fig. 1); (B) Microfocuser adapter; (C) Microfocuser; (D) 1.25" accessory adapter. SC accessory adapter (L) may be used in this position instead if Schmidt-Cassegrain accessories are being used.
Low power eyepieces offer a wide field of view, bright, high-contrast images, and eye relief during long observing sessions. To find an object with a telescope, always start with a lower power eyepiece such as the Super Plössl 26mm. When the object is located and centered in the eyepiece, you may wish to switch to a higher power eye- piece to enlarge the image as much as practical for prevailing seeing conditions.
The power, or magnification of a telescope is determined by the focal length of the tel- escope and the focal length of the eyepiece being used (an eyepiece's focal length is printed on the side of the eyepiece).
"unlock" position, until it feels loose. For more precise focusing, see Once you get a feel for how your telescope moves and focuses, try to view some- thing more challenging, like a bird or a distant moving train. You can also observe stars and objects in the night sky using this method, but note that objects begin to slowly drift across the eyepiece field.
Super Plössl 26mm. Speeds 7 or 8: Best used for rough centering of an object in the viewfinder. Speed 9: Moves the telescope quickly from one point in the sky to another. Bring the object into focus (see below).
Autostar II menu options. Observe the Moon Point your telescope at the Moon (note that the Moon is not visible every night) and practice using the Arrow keys, the microfocuser and the slew speeds to view different features. The Moon contains many interesting features, including craters, mountain ranges, and fault lines.
When the home position is found, the system knows the limiting positions of the telescope and can avoid tangling cables and over-rotating the telescope. Detects “level” of the base of the telescope; finds tilt and tip. To detect level, Autostar II must calculate "level" at three compass points. See...
Observe a Star using the Automatic Tracking Feature Now that your telescope has been aligned, you are able to track celestial objects. In this example, the Autostar II Arrow keys are used to find a star, and then Autostar II's tracking capability automatically keeps the star centered in your telescope's eye- piece.
LX200GPS Detecting True Level To detect level of the base of the telescope, Autostar II must calculate the tip and tilt of the telescope at three compass points and then compensate for it. Finding level involves the geometric calculations of a "plane." In order to define a plane, three positions are necessary.
"Event: Sunrise" is displayed. OBJECT MENU Want to see Mars? The Orion nebula? The Andromeda galaxy? Select from over 145,000 objects and press GO TO to move the telescope automatically to an object. Select Item: Event EVENT MENU Display the time of...
Navigating Autostar II Autostar II's menus are organized for quick and easy navigation: Tip: When multiple choices are available within a menu option, the current option is usually dis- played first and highlight- ed by a right pointing arrow (>). Press the Scroll Down key once to display the "Sunset"...
Align on Home Date Time Daylight Saving Smart Mount Configuration Train Update Load Save As Delete Erase Telescope Mount Model Focal Length Max Slew Rate Mount Upper Limit Mount Lower Limit Park Position Calibrate Home Anti-Backlash Train Drive Calibrate Sensors...
GO TO once to change the second line to the name of the bright- est star in the constellation. 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.
Press ENTER. Autostar II searches the libraries for the identity of the object being observed. If the telescope is not directly on an Autostar II library object, the nearest library object is located and displayed on the screen. Press GO TO and the telescope slews to that object.
Alarm: Selects a time for an alarm signal to sound as a reminder. To use the Alarm, press ENTER, then choose "Set" or "Start/Stop." Eyepiece Calc: Calculates information about an eyepiece for the specific telescope to which Autostar II is connected.
Daylight Saving menu (see above) to turn the Daylight Saving option on or off. Keep in mind that the telescope is receiving the correct time whether or not you set this option to display your local time.
R.A. and the Dec. axes by entering a number from 0% to 199%. This sets the backlash in the way the Arrow keys move the telescope along an axis. If you enter a value near 199%, telescope responds more quickly as you hold down an Arrow key.
"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.
Autostar II handbox. Software: Receives only the basic Autostar II software. This is useful if one user has downloaded a new version of Autostar II software from the Meade website (www.meade.com) and wants to pass this software along to friends.
If you plan to observe using Autostar II at different geographic locations, you can store observation sites in Autostar II's memory to help simplify your telescope setup. Perform these procedures using the Site options (Add, Select, Delete, Edit) of the Setup menu.
Press ENTER to select the site. Make sure Autostar II has been initialized and the telescope has been aligned. 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.
Satellite orbits change and new satellites (including the Space Shuttle) are launched. Visit the Meade website (www.meade.com) approximately once a month to get updated information and instructions on how to download this data to Autostar II. If orbital parameters are more than one month old, the satellite pass may not happen at the time predicted by Autostar II.
"Landmark: Add" displays. If you wish to add more landmarks, repeat steps 5 through 8. To Select a landmark from the database: Make sure the telescope is located and aligned exactly as when the desired land- mark was entered into memory. Display the "Landmark: Select" menu option. Press ENTER.
In this procedure, you will center an object you wish to have identified by Autostar II 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 II database.
Autostar II to signify that the message has been read and understood. 6. Autostar II displays "Align: Automatic." You are now ready to align your telescope using one of the three alt/az alignment pro- cedures. Easy (Two-Star) Alignment In this method, Autostar II automatically picks two stars from its libraries for alignment.
Set Home Position. Place the telescope in the home position. To Set the Home Position Manually: a. See Figs. 19 and 20, page 37. Loosen the telescope’s Dec. lock (17, Fig. 1). Set the optical tube to 0° on the Dec. setting circle (Fig. 20).
On and Off Menu Options Select "On" when you want the telescope to use the training information. Select "Off" when you do not want for the telescope to use the training information. Select "On" to enable the Smart Drive. , page 42). PEC training is available...
T-Mount. Rotate the camera body to achieve proper orientation of the object; then re-tighten the adjustment screws. The #62 T-Adapter permits close-coupling of a camera body to the telescope. In this format vignetting occurs: The photographic image appears on film with a slight dark- ening (vignetting) at the corners of the 35mm frame (Fig.
A wide assortment of professional Meade accessories is available for the telescope models. The premium quality of these accessories is well-suited to the qual- ity of the instrument itself. Consult the Meade General Catalog for complete details on these and other accessories.
Moon and planets. Each filter threads into the barrel of any Meade 1.25" eyepiece, and into the barrels of virtually all other eye- piece brands as well. Meade filters are available in 12 colors for lunar and planetary applications, and in Neutral Density as a lunar glare-reduction filter.
This dew formation may be inhibited to a significant extent by the addition of a dew shield, essentially an extension tube attaching to the front-cell of the telescope. #608 for Meade 7" Maksutov and 8" Schmidt-Cassegrain models; #610 for all 10" Schmidt-Cassegrain models;...
As part of final optical testing, every Meade Schmidt-Cassegrain is precisely collimat- ed 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.
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.
Customer Service hours are 8:30 AM to 4:30 PM, Pacific Time, Monday through Friday. In the unlikely event that your write or call the Meade Customer Service Department first, before returning the tele- scope to the factory, giving full particulars as to the nature of the problem, as well as your name, address, and daytime telephone number.
The fan operates when a special power cord (sup- plied in the accessory box) is plugged into the fan unit of the telescope and the12v DC OUT (13E, Fig. 1) of the computer control panel with the power switch in the “ON”...
Fig. 36) is located on the top surface of the telescope’s drive base. The Declination circle (Fig. 35) is located at the top of the fork tine. With the telescope pointed at the North Celestial Pole, the Dec. circle should read 90° (understood to mean +90°).
Note: The Meade equatorial wedge is designed solely for use in conjunction with your Meade tripod. The wedge should never be used without the tripod (e.g., by placing the wedge alone on a table top and then mounting the tele- scope on the wedge—the wedge may become seriously unbalanced, to the...
This tracking may be accomplished automatically with the If the telescope is reasonably well aligned with the pole, very little use of the tele- scope’s Declination slow motion control is necessary. Virtually all of the required tele- scope tracking will be in Right Ascension.
10 minutes or longer). In particular, the number of Declination corrections required is a direct function of the precision of polar alignment. Precise polar alignment requires the use of a crosshair eyepiece. The Meade Illuminated Reticle Eyepiece (see...
NASA, Hubble, HST, astronomy, Messier, satellite, nebula, black hole, variable stars, etc. Check Meade’s website for the latest product and technical information. You can download the latest software revisions, links to other astronomical sites, coordinates of celestial objects and the latest satellite tracking information for your Autostar II handset.
APPENDIX B: LATITUDE CHART Latitude Chart for Major Cities of the World To aid in the polar alignment procedure (see page 52), latitudes of major cities around the world are listed below. To determine the latitude of an observing site not listed on the chart, locate the city closest to your site. Then follow the procedure below: Northern hemisphere observers (N): If the site is over 70 miles (110 km) North of the listed city, add one degree for every 70 miles.
More commands will be added from time-to-time to the list below. Periodically visit Meade's website (www.meade.com) for future additions. When a Guided Tour is selected, Autostar II slews your telescope to a predetermined list of objects and displays information about each object, such as type of object, con- stellation location, R.A.
TITLE TEXT PLANET MOON COMET LUNAR ECLIPSE METEOR SHOWER CONSTELLATION STAR PICK ONE/PICK END AUTO SLEW 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.
PLANET "name" Enter PLANET and then the name of the desired planet in quotes. Autostar II provides the user with a description of the selected planet from its database. For example: PLANET "Pluto" MOON This command accesses information about the Moon from the Autostar II database. SATELLITE "name"...
PICK ONE AUTO SELECT MESSIER 13 AUTO SELECT MESSIER 15 AUTO SELECT MESSIER 92 AUTO SELECT MESSIER 4 AUTO SELECT MESSIER 68 AUTO SELECT NGC 1234 AUTO SELECT TEXT "None Available" "I'm sorry. There are no bright globular" "clusters visible at this time." PICK END AUTO SLEW ON / AUTO SLEW OFF With AUTO SLEW ON enabled in the tour, Autostar II automatically slews the tele-...
APPENDIX D: TRAINING THE DRIVE Train the telescope motors using Autostar II. Perform this procedure if you are experiencing any pointing accuracy problems. Fig. 41 depicts the complete Drive Training procedure. Use a terrestrial object, such as a telephone pole or lamp post, to train the drive. Complete this exer- Note: cise once every 3 to 6 months to maintain the highest level of telescope pointing accuracy.
Fig 1). The resulting misalignment of the axes will result in inaccurate slew- ing of the telescope in the GO TO mode. Do not attempt to turn the focus knob of the optical tube (6, Fig. 1) until you have read the following note.
Use the following procedure to assemble your telescope: To Assemble the 16” Super Field Tripod The 16” Super Field Tripod (Figs. 44 and 45) for the Meade 16” is supplied as a completely assembled unit, except for the spreader bar (4, Fig. 44) and the six lock-knobs (5, Fig.
See Fig. 51. e. A fifth 3/8”-16x3/4” long bolt is supplied with the telescope. Just using your fingers, loosely tighten this bolt under the plate. See Fig. 51. This bolt acts as a safety fea- ture to prevent the DB-15 connector and cable from being damaged when you dis- assemble the telescope.
Attaching the Power and Data Cords Several power and data cords are supplied with the 16” be attached before powering up the telescope. a. Confirm that the power switch (A, Fig. 43) on the power panel is in the OFF posi- tion.
Next, remove the battery holder and install the batteries as described in step #2 on page 13. Replace the holder and close the compartment. Replace the screws if you plan to use the telescope in equatorial alignment. These screws are not necessary when using the telescope in altazimuth alignment.
(K, Fig. 6) up against the adapter ring as shown in Fig. 60. Take care not to tighten or loosen the adapter ring as you position and tighten the microfocuser in place. 4. Tighten to a firm feel the other two microfocuser hex screws. 5. Attach the de-rotater to the rear cell of the telescope.
OUNT PDATE above). If Smart Mount was "On" when you last powered off your telescope, it will be "On" when you start the next session. When Smart Mount is "Off," the telescope will not use any model you have created to refine pointing accuracy.
Moon, and our solar system comes from observations made by ama- teur astronomers. So as you look through your Meade mind Galileo. To him, a telescope was not merely a machine made of glass and metal, but something far more—a window of incredible discovery.
The disk of Venus appears white as Sunlight is reflected off the thick cloud cover that completely obscures any surface detail. 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.
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.