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Instruction Manual 8", 10", 12" LX90 GPS Schmidt-Cassegrain T elescopes A utoStar ® — GPS— Smar tFinder ™ ™ ...
Primary Baffle Tube Field Stops Primary Mirror Ray (1) Ray (2) (2) (1) (2) (1) Secondary Mirror Correcting Plate S econdary B affle (2) (1) F ocal P lane In the Schmidt-Casseg rain design of the Meade LX90, light enters from the right, passes through a thin lens with 2-sided aspher ic correction (“correcting plate”), proceeds to a s ...
Quick-Start Guide .......................................................... 4 T elescope Features ...................................................... 6 T o Attach the Handbox Holder .................................. 8 A utoStar ® F eatures ........................................................ 9 Getting Star ted ............................ ...
4 QUICK-ST AR T GUIDE It is recommended that you attach the supplied tripod to the LX90 f or obser ving. P erf or m the telescope and AutoStar setup indoors in the light so that you become f amiliar with the par ts and operation bef ore moving the telescope outside into the dark for observing. 1. Remov e the field tripod from the shipping car ton. ...
5 R ib Battery H older B attery C ompar tment 8. Tighten, to a firm feel only , the Dec and R.A. locks ( X and X, Fig. 1) . Remove the dust co ver from the end of the telescope tube. 10. “Press 0 to align or Mode f or Men u” displays . Y ou can use the Arrow k eys to slew (mo ve) the tele- scope up , down, right, or left. T o change the t ...
6 Fig. 1 : The LX90 T elescope and AutoStar Handbo x. TELESCOPE FEA TURES 2 D 3 6 8 J M O P Q A R K N 2! 1@ 2) A B C D D E (not sho wn) 9 1 Eyepiece 2 Ey epiece Holder Thumbscre w 3 Eyepiece Holder 4 Diagonal Prism 5 Optical T ube 6 Dec. Lock 7 Fork Arms 8 Focus Knob 9 R.A. Lock 10 R.A. Setting Circle 11 Dec. Setting Circ le/Dec. P ointer 12 GPS Re ...
7 LX90: Y our P ersonal Window to the Universe The Meade LX90 is an e xtremely versatile, high-resolution telescopes with f eatures similar to those av ailable only with larger and more specializ ed imaging systems. With pushbutton controls, automatic trac king of celestial objects and software downloading capability , the LX90 telescope ma y be al ...
8 D . A uxiliary (AUX) P or t (2) : Pro vides connection f or the Smar tFinder LNT module, and also current and future Meade accessories, such as the Meade Accessor y P or t Module . See OPTIONAL A CCESSORIES , page 43. E. 12v P ower Connector : Provides connection so that the telescope assemb ly may be powered from either a 12v DC auto cigarette l ...
9 Fig. 2: The LX90 A utoStar Handbox. L 1 B D E H I J K C F G T our the Cosmos with Just the Push of a Button Control of the LX90 is through the operation of the standard-equipment A utoStar . Nearly all functions of the telescope are accomplished with just a f ew pushes of A utoStar’ s buttons. Some of the major f eatures of AutoStar are: • A ...
10 The A utoStar Computer Controller provides control of vir tually ev er y telescope function within a compact handbo x. AutoStar has soft-touch k eys designed to ha ve a positiv e feel. The LCD (Liquid Cr ystal Displa y) is backlit with a red LED (Light Emitting Diode) f or easy viewing in the dark. The backlit displa y , key arrangement, and seq ...
11 8. The Smar tFinder’ s red dot will now blink on f or 10.2 seconds and turn off for 0.7 seconds , and then repeat the cycle until you change the v alues again. Press and hold MODE c to e xit this function. Similar ly , you can set the Intensity v alue by scrolling through the intensity v alues with the Scroll keys h . The Intensity option lets ...
12 Getting the telescope ready f or first obser vations requires only a f ew minutes . When first opening the packing bo x, note carefully the f ollowing par ts: • LX90 T elescope with fork mount system and attached Smar tFinder • A utoStar handbox and interf ace coil cord • Eyepiece holder and 1.25” diagonal pr ism • 8 x 50 Viewfinder ? ...
13 6. Place the entire telescope onto the top of the tripod head, and inser t the threaded rod into the centr al hole in the bottom of the drive base of the telescope . Tighten the tension knob ( 3, Fig. 3 ); firm tightening of the tension knob is sufficient to result in r igid positioning of the tr ipod legs. 7. T o vary the tr ipod height, loosen ...
14 Choosing an Eyepiece A telescope’ s ey epiece magnifies the image formed by the telescope’ s main optics. Each ey epiece has a focal length, e xpressed in millimeters, or “mm. ” The smaller the focal length, the higher the magnification. For e xample, an e yepiece with a f ocal length of 9mm has a higher magnification than an ey epiece w ...
15 Aligning SmartFinder In order f or the Smar tFinder to be useful, it must first be aligned with the main telescope, so that both the Smar tFinder and the main telescope are pointing at precisely the same location. T o align the Smar tFinder : 1. Point the main telescope at some w ell-defined distant (perhaps a mile awa y) land object, such as a ...
16 OBSER VING Observing By Moving the T elescope Manually If you wish to observe a distant land object, such as a mountain top or a bird, y ou can obser ve by merely pointing the telescope and looking through the e yepiece. 1. Loosen the telescope’ s R.A. lock ( 9, Fig. 1 ) and Dec loc k ( 6, Fig. 1 ). 2. Mov e your telescope to observe distant s ...
17 2. V erify that AutoStar is properly connected to your telescope . See HO W T O ASSEMBLE Y OUR TELESCOPE , page 13. 3. Flip the telescope power s witch to the ON position. The A utoStar screen is activated and a cop yright message displays briefly , f ollowed b y a shor t beep. Then AutoStar takes a f e w moments to star t up the system. “Pres ...
18 Astronomical Observing Used as an astronomical instr ument, your telescope has many optical and electromechanical capabilities. It is in astronomical applications where the high lev el of optical performance is readily visible . The range of observable astronomical objects is , with minor qualification, limited only b y the observer’ s motivat ...
19 A utoStar also deter mines the positioning ( i.e ., tilt and tip) of the optical tube . b. Finds North. Locates magnetic Nor th, then calculates true Nor th. See FINDING TRUE NORTH, page 21. c. Attempts a "GPS Fix ." The GPS receiv er attempts to acquire and sync up with signals from GPS satellite system. "Getting GPS Fix" di ...
20 Go T o Saturn After perf or ming the Automatic Alignment procedure , the motor dr ive begins oper ating and the telescope is aligned f or a night of viewing. Objects in the ey epiece should maintain their position e ven though the Ear th is rotating beneath the stars. IMPORT ANT NOTE : Once aligned, only use the GO TO or Arro w ke ys to mov e th ...
21 LX90 T ips Fig. 9: The GPS Receiver . GPS Receiv er The Global Positioning System The Global P ositioning System (GPS) is comprised of 24 satellites orbiting the Ear th that are constantly transmitting their precise position and time. The system provides highly accurate , worldwide positioning and navigation inf or mation for an y number of appl ...
22 It is impor tant to understand that menu selections are set in a loop ( Fig. 11 ). This means that pressing the Scroll Down k ey ( 7, Fig. 2 ) cycles down through all the a vailab le options within a giv en categor y , then retur ns to the first option. The Scroll Up ke y ( 7, Fig. 2 ) cycles up through the options in the opposite order . Note t ...
23 T o Calculate Sunset time: 1. Press the MODE ke y sev eral times, until “Select Item: Object” is displa yed. 2. Press the Scroll Down k ey once to displa y the “Ev ent” option in the “Select Item” menu. 3. Press the ENTER ke y to choose the "Event" option and mo ve down a le v el. "Event: Sunr ise" is display ed. ...
MENUS AND MENU OPTIONS 24 T o night's Best H o w F ar is F ar A Star's Life D o wnloaded T ours U s er-created T ours Solar System M e rcury Etc . M o on A s teroids C omets C onstellations A n dromeda Etc . Dee p S k y N amed Obj ect G ala x ies N e b ulae M e ssier Etc . Star N amed S A O C atalog D o u b le V aria b le Etc. Satellite S ...
25 Object Menu Almost all obser ving with A utoStar is performed using the Object menu categor y . ( NO TE: Exceptions include Guided T our and Landmark Sur vey . ) See GO T O SA TURN , page 20, f or an e xample of obser ving using the Object menu. Also see USING THE GUIDED T OUR , page 20. Many A utoStar menu categories contain databases. An A uto ...
26 Event Menu The Event men u provides access to dates and times of astronomical e vents. The Event database includes: Sunrise and Sunset calculates the time that the Sun rises or sets on the current date. Find rise and set times for other dates b y entering a new date into the “Setup: Date” menu. See D A TE, page 28. Moonrise and Moonset calcu ...
27 J Set : Enter the time of day f or the alarm to sound, in hours, minutes, and seconds , then press ENTER. J Start/Stop : Activates the alarm set previously . Use the Scroll keys to toggle betw een ON and OFF . When ON is display ed, press ENTER to activate the alarm. When the alarm time arrives, A utoStar beeps. Press ENTER to deactivate the ala ...
28 P ark Scope is designed for a telescope that is not mov ed between observing sessions. Align the telescope one time , then use this function to park the telescope. Next time it is po wered up , enter the correct date and time – no alignment is required. Pressing ENTER causes the telescope to mov e to its pre-deter mined P ark position. Once pa ...
29 c. Custom : Allows entry of user-defined tracking rates . J Rever se L/R: Rev erses the functions of the Left and Right Arrow ke ys ( i.e. , the Right k ey mov es the telescope to the left ). J Rever se UP/DO WN: Rev erses the functions of the Up and Down Arrow k eys ( i.e . , the Up ke y mov es the telescope down ). J Rever se L/R: Rev erses th ...
30 J Delete : Deletes a stored site from the database. J Edit : Edits a selected site, including: the name, latitude, longitude , and time zone. Time Zone ref ers 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 s ...
31 AD V ANCED A UT OST AR FEA TURES Adding Observing Sites If you plan to observe using A utoStar at different geog raphic locations, y ou can store up to six obser vation sites in A utoStar's memory to help simplify your telescope setup . P erform these procedures using the Site options (Add, Select, Delete, Edit) of the Setup menu. T o Add a ...
32 4. Using the Arrow k eys, change the name of the site so that it no w reads the name of your obser ving location. Press ENTER. "Edit: Name" displays again. 5. Press the Scroll Down k ey and "Edit: Latitude" displays. Press ENTER. 6. Using the Number K eys , enter the latitude of your obser ving site and then press ENTER. &quo ...
33 9. A utoStar then prompts you to enter the magnitude of the object. This step is also optional. Use the Number ke ys to enter this information, if so desired, and press ENTER to go to the ne xt display . "User Object: Add" displays again. T o GO T O a user-entered object: In this procedure, y ou will choose an object from the User Obje ...
34 How to Create Y our Own Guided T our When a Guided T our is selected, AutoStar sle ws your telescope to a predetermined list of objects and displa ys information about each object, such as type of object, constellation location, R.A. and Dec coordinates, and so f or th. AutoStar contains a f ew Guided T ours which are programmed at the f actor y ...
35 Writing a T our Using the list of commands listed abov e, a custom tour can be created. Placing the word A UT O SELECT bef ore any of the command lines activates A utomatic Mode and, when selected, A utoStar automatically searches and finds the designated object. The f ollowing is a list of command lines, complete with k eywords and necessary st ...
36 ASTER OID "name" Enter ASTEROID and then the name of the desired asteroid in quotes . A utoStar displays inf or mation about the asteroid from its database. For e xample: ASTEROID: "Ceres" COMET "name" Enter COMET and then the name of the desired comet in quotes. AutoStar displa ys inf or mation about the comet from ...
37 A UT O SLEW ON / A UT O SLEW OFF With A UT O SLEW ON enabled in the tour , AutoStar automatically sle ws the telescope to objects first bef ore displaying the te xt description. This f eature is useful when designing tours in which obser ving cer tain objects is required. For e xample, an astronom y professor ma y require his students to obser v ...
38 2. Displa y the "Landmar k: Select" menu option. Press ENTER. 3. Use the Scroll ke ys to scroll through the list of objects you ha ve pre viously entered. When the desired object displa ys, press ENTER to select the object. Use the Scroll ke ys to scroll through location inf or mation about the object, if desired. Press GO TO to sle w ...
39 T wo-Star alt/az alignment procedures, y ou will (unlike the A utomatic and Easy alignment pro- cedures) manually place the telescope in the home position. The procedures f or equator ial (polar) alignment are discussed in APPENDIX A , page 50; the three alternative alt/az alignment methods are discussed below . Easy (T wo-Star) Alignment In thi ...
40 One-Star Alt/Az Alignment One-Star Alignment requires some knowledge of the night sky . AutoStar provides a library of br ight stars. One-Star Alignment is identical to T wo-Star Alt/Az: Alignment (see TWO-ST AR AL T/AZ ALIGNMENT , page 38), e xcept only one star from the database is chosen by the observer f or alignment. Bro wse This menu allow ...
41 Photog raph y through the LX90 requires the addition of the optional #62 T–Adapter . See OPTIONAL A CCESSORIES, page 43. With the #62 T -Adapter and a T -mount attached to the telescope ( Fig. 15 ), through-the-telescope photograph y is possible with an y 35mm camera body with a remov able lens. In this wa y , the telescope effectiv ely become ...
42 Shor ter exposure times is one of the biggest dr awback. Long exposures with digital cameras introduce undesirab le noise and ar tif acts into a digital image. This limits the range of astro images to the Moon, planets and bright stars. Some tips f or better digital photos: • If you cannot remo ve the lens to y our camera, look for a commercia ...
43 OPTIONAL A CCESSORIES A wide assor tment of professional Meade accessories is av ailable f or the LX90 telescope. The premium quality of these accessories is well-suited to the quality of the instrument itself. Consult the Meade General Catalog for complete details on these and other accessories. Some of the Meade Series 4000 and 5000 Ey epieces ...
44 #62 T -Adapter: The T -Adapter ( Fig. 22 ) is the basic means of pr ime-focus photogr aphy through all Meade Schmidt-Cassegrain models . Thread the T -Adapter on to the rear cell of your telescope, f ollowed b y a T -Mount for your 35mm camer a, and the camera body is rigidly coupled to the telescope. V ariable T ele-Extender: For e yepiece-proj ...
45 MAINTENANCE The LX90 is a precision optical instrument designed to yield a lifetime of re warding applications. Given the care and respect due an y precision instrument, the LX90 will rarely , if e ver , require f actor y ser vicing. Maintenance guidelines include: a. A void cleaning the telescope’ s optics: a little dust on the front surface ...
46 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. F ollow these steps for collimation of the optical system: a. The only adjustments possible , or necessar y , on the LX90 ar ...
47 Inspecting the Optics A Note About the “Flashlight T est:" 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) ma y rev eal what appears to be scratches, dark or bright spots, or just generally une ven coatings , ...
48 8” LX90 Specifications Optical design ............................................................Schmidt-Cassegrain Clear aper ture ............................................................8" F ocal length ................................................................2000mm F ocal ratio (photographic speed) ......................... ...
49 12” LX90 Specifications Optical design ............................................................Schmidt-Cassegrain Clear aper ture ............................................................12" F ocal length ................................................................3048mm F ocal ratio (photographic speed) ....................... ...
50 P olar Alignment In P olar Alignment, the telescope is oriented so that the horizontal and vertical axes of the telescope are lined up with the celestial coordinate system. In order to P olar align your telescope , it is essential to hav e an understanding of how and where to locate celestial objects as they mo ve across the sky . This section p ...
51 Locating the Celestial P ole T o get basic bearings at an obser ving location, tak e note of where the Sun rises (East) and sets (W est) each day . After the site is dar k, face North b y pointing y our left shoulder toward where the Sun sets. T o precisely point at the pole, find the Nor th Star (P olaris) by using the Big Dipper as a guide ( F ...
52 Note that the R.A. circle is double-inde xed (i.e ., there are two series of numbers running in opposite directions around the circumf erence of the R.A. circle). The upper series of numbers (increasing counterclockwise) applies to observers located in the Earth’s Norther n Hemisphere; the lower series of numbers (increasing cloc kwise) applie ...
53 Begin polar aligning the telescope b y locating P olar is. Finding P olar is is simple. Most people recognize the “Big Dipper . ” The Big Dipper has two stars that point the wa y to P olaris ( Fig. 29 ) . Once P olaris is found, it is a straightf orward procedure to obtain a rough polar alignment. T o line up with P olaris, follo w the proce ...
54 1. Obtain a rough polar alignment as described ear lier . Place the illuminated reticle ey epiece (or ey epiece/Bar low combination) into the e yepiece holder of the telescope. 2. P oint the telescope, with the motor drive running, at a moderately bright star near where the meridian (the Nor th-South line passing through your local zenith) and t ...
55 NORTH AMERICA City State/Pro v ./Country Latitude Albuquerque New Me xico 35° N Anchorage Alaska 61° N Atlanta Georgia 34° N Boston Massachusetts 42° N Calgary Alber ta 51° N Chicago Illinois 42° N Clev eland Ohio 41° N Dallas T exas 33° N Denv er Colorado 40° N Detroit Michigan 42° N Honolulu Ha w aii 21° N J ac kson Mississippi 32° ...
56 T rain the telescope motors using A utoStar . P erform this procedure if you are e xperiencing any pointing accuracy problems . Fig. 33 depicts the complete Drive T raining procedure. NO TE: Use a terrestrial object, such as a telephone pole or lamp post, to train the dr ive . Complete this e xercise once e very 3 to 6 months to Fig. 33: T raini ...
57 In the ear ly 17th centur y Italian Scientist Galileo, using a crude telescope considerab ly smaller than the LX90, turned it to look towards the sky instead of distant trees and mountains. What he sa w , and what he realized about what he sa w , fore v er changed the wa y mankind thought of the universe . Imagine what it must hav e been like be ...
58 Planets Planets change positions in the sky as they orbit around the Sun. T o locate the planets on a given da y or month, consult a monthly astronomy magazine , such as Sky and T elescope or Astronom y . Y ou can also consult AutoStar f or inf or mation about planets. Scroll to the "Object: Solar System" menu and scroll through the li ...
59 ...
14-6700-00 01/06 (800) 626-3233 www .meade.com MEADE LIMITED W ARRANTY Every Meade telescope, spotting scope, and telescope accessory is warranted b y Meade Instruments Cor poration (“Meade”) to be free of defects in materials and workmanship f or a period of ONE YEAR from the date of original purchase in the U .S.A. and Canada. Meade will repa ...
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