Important Note: Once the telescope is aligned, only use the Arrow keys to move the tele- scope. Once the telescope has been aligned, do not loosen the telescope locks (12 and 17, Fig. 1), or move the base manually, or alignment will be lost.

Important Notes:

It is recommended that you do not attempt a GPS fix indoors.

It is also recommended that you CALIBRATE SEN- SORS the first time your telescope takes a GPS fix. See page 29 for more information.

Important Note:

The Daylight Saving menu enables or disables the Daylight Savings Time setting: Remember to turn this setting off or on the two days a year when Daylight Saving changes. See TIMING IS EVERYTHING, page 28.

5."Automatic Alignment" displays. The system now performs the following routines (press any AutoStar II key to abort Automatic Alignment; see IMPORTANT NOTE, at the bottom left of page 18.) :

Caution: As the telescope performs the following operations, it will swing and rotate. Keep a safe distance from the telescope. The telescope now finds the level and tilt position of the telescope, and also detects where true North is. It may not actually level or tilt the telescope or point to North—it is just detecting these positions. This make take a minute or two.

a.Finds the home position. Moves the telescope to find the "home" position. 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.

b.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 FINDING TRUE LEVEL in on page 21.

AutoStar II also determines the positioning (i.e., tilt and tip) of the optical tube.

c.Finds North. Locates magnetic North, then calculates true North. See

FINDING TRUE NORTH, page 21.

d.Attempts a "GPS Fix." The GPS receiver attempts to acquire and sync up with signals from GPS satellite system. "Getting GPS Fix" displays. See THE GLOBAL POSITIONING SYSTEM on page 21.

After performing these operations, AutoStar II now knows:

The telescope's limiting positions

Where level is for the telescope

The location of true North

The observing site's location

The date and time

Note: Press any key to abort the GPS fix. You will then be prompted to enter the time, date and location.

e.Once the level, tilt and North are detected, the telescope will “Go To” 2 alignment stars. The telescope will go to these stars in order to orient itself to the sky. Once it has done this, it will be able to point to any of the more than 145,000 stars in its database.

“Automatic Alignment: Selecting Star” and “Slewing” display. Finally, when it is

close to the alignment star “Center Brightest Star: Press ENTER” displays. Use the Arrow keys to center the alignment star in the eyepiece. The alignment star will be the brightest star in that area of the sky (and hence, “brightest star”). When the alignment star is entered, press ENTER.

Note: If you press the “?” key while “Ctr Brightest Star” displays, the alignment star

that AutoStar has chosen will display. For example, “Arcturus: Press ENTER” may display.

Note: If you have an obstruction, such as a tree or a building blocking your view of the alignment star, or if you have any doubts at all about the star that has been cho- sen, no problem. Just press the Scroll Down key and AutoStar will find another star to align upon.

LX200R TIPS

Which One’s the Alignment Star?

If AutoStar II has chosen an alignment star with which you are unfamiliar, 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 GO TO 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 dra- matically from the rest of the stars in that portion of the sky. The viewfinder will help you locate a star more quickly than the eyepiece, because it has a much wider field of view than the eyepiece. Using AutoStar II, set the slew speed to 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 20.

- 19 -

Looking at or near the Sun will cause irreversible damage to your eye. Do not point this telescope

 

at or near the Sun. Do not look through the telescope as it is moving.

Page 19
Image 19
Meade LX200 R Which One’s the Alignment Star?, It is recommended that you do not attempt a GPS fix indoors

LX200 R specifications

The Meade LX200 R is a renowned telescope that has captivated astronomers and enthusiasts alike with its impressive blend of advanced technology, user-friendly features, and excellent optical performance. Launched as part of Meade's line of enjoyable yet high-performing telescopes, the LX200 R remains a top choice for both amateur stargazers and serious astrophotographers.

At the heart of the LX200 R is its advanced telescope design. It features a robust, 8-inch primary mirror, which provides exceptional light-gathering capability. This larger aperture allows users to observe faint celestial objects, including distant galaxies, nebulae, and star clusters, with stunning clarity and detail. The telescope's reflective optics are coated with high-quality, anti-reflective coatings that enhance contrast and minimize light loss, ensuring crisp, clear images even in challenging viewing conditions.

One of the standout features of the LX200 R series is its sophisticated computer-controlled GoTo mount. This feature allows users to locate over 30,000 celestial objects with remarkable precision using a simple one-button operation. The dual-axis motor drives enable smooth tracking of objects across the night sky, making it easier to follow their movements. The mount also includes an integrated GPS system, which automatically adjusts the telescope's location and time settings for accurate alignment without requiring complex manual adjustments.

The LX200 R is configured for both visual observations and astrophotography, accommodating a wide range of accessories like cameras and focal reducers. Its sturdy construction minimizes vibrations, which is crucial for capturing sharp images during extended exposures. Additionally, the telescope's optical tube is designed to be both lightweight and durable, making it convenient for transport and setup in various observing locations.

The ergonomic design of the LX200 R also enhances user experience, featuring a comfortable eyepiece height and an intuitive control panel. The display is user-friendly, allowing even novice astronomers to navigate settings and options quickly. With its combination of high-quality optics, advanced tracking capabilities, and versatile design, the Meade LX200 R continues to be a preferred choice for anyone looking to explore the wonders of the universe with sophistication and ease.