Mounting Slot

Track

Thumb- screws

Fig. 11: Viewfinder Assembly.

Collimation Viewfinder

ScrewsEyepiece

GPS

Receiver

Fig. 12: Viewfinder collimation screws and eyepiece.

Tip:

Because the space between the GPS receiver and the viewfinder is a bit tight, it is helpful if you tighten the front, bottom viewfinder collimation thumbscrew first and use the other screws to set the alignment. However, if you determine you need to adjust the front thumb- screw, choose an alignment object that allows you to slightly elevate or rotate the telescope to a convenient position for adjustment of this thumbscrew.

Fig. 13a & 13b: Jupiter; examples of the right amount of magnification and too much magnification.

with a lower power eyepiece such as the 26mm Plössl. When the object is located and centered in the eyepiece, you may wish to switch to a higher power eyepiece to enlarge the image as much as practical for prevailing seeing conditions. For informa- tion about optional eyepieces for the your telescope, see OPTIONAL ACCESSORIES, page 43.

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). To calculate eyepiece power, divide the tele- scope's focal length by the eyepiece's focal length. For example: A 26mm eyepiece is supplied with LX200R models. The focal length of the 8" f/10 LX200R is 2000mm (see SPECIFICATIONS, pages 46 through 48).

Eyepiece Power = Telescope focal length ÷ Eyepiece focal length Eyepiece Power = 2000mm ÷ 26mm

Eyepiece Power = 77

The eyepiece power, or magnification is therefore 77X.

Note: For a list of magnification ratings of the eyepieces available for the LX200R telescopes, see OPTIONAL ACCESSORIES, page 43.

Mounting and Adjusting the Viewfinder

To align the viewfinder, perform steps 1 through 5 during the daytime; perform step 6 at night.

1.Slide the track on the bottom of the viewfinder into the slot in the viewfinder mounting assembly. See Fig. 11. To secure the viewfinder to the mounting assembly, tighten the two thumbscrews (Fig. 11) to a firm feel only.

2.If you have not already done so, insert the Super Plössl 26mm eyepiece into the diagonal prism.

3.Unlock the R.A. (12, Fig. 1) and Dec. (17, Fig. 1) locks so that the telescope moves freely on both axes.

4.Point the telescope at some well-defined and stationary land object at least 200 yards distant, such as the top of a telephone pole or street sign. Center the object in the telescope eyepiece. Re-tighten the R.A. and Dec. locks.

5.Look through the viewfinder eyepiece (Fig. 12) and loosen or tighten, as appro- priate, one or more of the viewfinder collimation screws (Fig. 12) until the viewfinder crosshairs are precisely centered on the object you previously cen- tered in the telescope eyepiece.

6.Check this alignment on a celestial object, such as the Moon or a bright star, and make any necessary refinements, using the method outlined in steps 3 through 5.

Note: Seeing conditions vary widely from night-to-night and site-to-site. Turbulence in the air, even on an apparently clear night, can distort images. If an image appears fuzzy and ill-defined, back off to a lower power eyepiece for a more well-resolved image (see Fig. 13a and 13b).

LX200R TIPS

Too Much Power?

Can you ever have too much power? If the type of power you’re referring to is eyepiece magnification, yes, you can! The most common mistake of the begin- ning observer is to “overpower” a telescope by using high magnifications which the telescope’s aperture and atmospheric conditions cannot reasonably support. Keep in mind that a smaller, but bright and well-resolved image is far superior to one that is larger, but dim and poorly resolved (see Figs. 13a and 13b). Powers above 400X should be employed only under the steadiest atmospheric condi- tions.

AutoStar II can calculate the best eyepiece for you to use. Try out the “Eyepiece Calc” feature in the Utilities menu.

Most observers should have three or four additional eyepieces to achieve the full range of reasonable magnifications possible with the LX200R telescopes. See OPTIONAL ACCESSORIES, page 43.

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

 

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

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Meade LX200 R instruction manual Mounting and Adjusting the Viewfinder, Too Much Power?

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.