Meade LXD55 instruction manual Planets, Deep-Sky Objects

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Fig. 51: The giant planet, Jupiter. The four largest moons can be observed in a different position every night.

Fig. 52: Saturn has the most extensive ring struc- ture in our Solar System.

Fig. 53: The Pleiades is one of the most beautiful open clusters.

Planets

Planets change positions in the sky as they orbit around the Sun. To locate the plan- ets on a given day or month, consult a monthly astronomy magazine, such as Sky and Telescope or Astronomy. You can also consult Autostar for information about planets. Scroll to the "Object: Solar System" menu and scroll through the lists of plan- ets. When a planet you are interested in displays, press ENTER. Use the Scroll keys to display information about the planet, such as the planet's coordinates, and the rise and set times (Tip: enter a date in the Date menu and you can determine if a plan- et(s) will be visible during the night of the entered date by checking its rise and set times). Listed below are the best planets for viewing through the LXD55-Series.

Venus is about nine-tenths the diameter of Earth. As Venus orbits the Sun, observers can see it go through phases (crescent, half, and full) much like those of the Moon. 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. Approximately every two years, when Mars is closest to Earth in its orbit, additional detail and coloring on the planet's surface may be visible.

Jupiter is the largest planet in our solar system and is eleven times the diameter of Earth. The planet appears as a disk with dark lines stretching across the surface (Fig. 51). These lines are cloud bands in the atmosphere. Four of Jupiter’s moons (Io, Europa, Ganymede, and Callisto) can be seen as “star-like” points of light when using even the lowest magnification. These moons orbit Jupiter so that the number of moons visible on any given night changes as they circle around the giant planet.

Saturn is nine times the diameter of Earth and appears as a small, round disk with rings extending out from either side (Fig. 52). In 1610, Galileo, the first person to observe Saturn through a telescope, did not understand that what he was seeing were rings. Instead, he believed that Saturn had “ears.” Saturn’s rings are composed of billions of ice particles ranging in size from a speck of dust to the size of a house.

The major division in Saturn's rings, called the Cassini Division, is occasionally visi- ble through the LXD55-Series. Titan, the largest of Saturn’s moons can also be seen as a bright, star-like object near the planet.

Deep-Sky Objects

Star charts can be used to locate constellations, individual stars and deep-sky objects. Examples of various deep-sky objects are given below:

Stars are large gaseous objects that are self-illuminated by nuclear fusion in their core. Because of their vast distances from our solar system, all stars appear as pin- points of light, irrespective of the size of the telescope used.

Nebulae are vast interstellar clouds of gas and dust where stars are formed. Most impressive of these is the Great Nebula in Orion (M42), a diffuse nebula that appears as a faint wispy gray cloud. M42 is 1600 light years from Earth.

Open Clusters are loose groupings of young stars, all recently formed from the same diffuse nebula. The Pleiades is an open cluster 410 light years away (Fig. 53). Through the LXD55-Series, numerous stars are visible.

Constellations are large, imaginary patterns of stars believed by ancient civilizations to be the celestial equivalent of objects, animals, people, or gods. These patterns are too large to be seen through a telescope. To learn the constellations, start with an easy grouping of stars, such as the Big Dipper in Ursa Major. Then, use a star chart to explore across the sky.

Galaxies are large assemblies of stars, nebulae, and star clusters that are bound by gravity. The most common shape is spiral (such as our own Milky Way), but galaxies can also be elliptical, or even irregular blobs. The Andromeda Galaxy (M31) is the closest spiral-type galaxy to our own. This galaxy appears fuzzy and cigar-shaped. It is 2.2 million light years away in the constellation Andromeda, located between the large “W” of Cassiopeia and the great square of Pegasus.

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Contents Meade Instruments Corporation Page Contents 1 1% g f e Telescope Features$2% LXD55-SeriesYour Personal Window to the Universe Computer Control Panel see e LXD55 Tips Features Autostar FeaturesTour the Cosmos with Just the Push of a Button Tip Telescope Assembly How to Assemble Your TelescopeAccessories Getting StartedViewfinder assembly Schmidt-Newtonian models Insert eyepiece into holder and tighten thumbscrews Balancing the TelescopeChoosing an Eyepiece Aligning the ViewfinderObserving by Moving the Telescope Manually Too Much Power?Slew Speeds Autostar Models Only Activate the Arrow Keys Autostar Models OnlyObserve the Moon Setting the Polar Home PositionTracking Objects 16bUsing Autostars GO to Capabilities Autostar Models Only Observe a Star using the Automatic Tracking FeatureInitializing Autostar Autostar Models Only Moving Through Autostar’s Menus Autostar Models OnlyTraining the Drive Autostar Models Only Go To Saturn Autostar Models Only Easy Alignment Autostar Models OnlyPlanet Saturn is over 800 million miles from the Earth Using the Guided Tour Autostar Models OnlyTo Calculate Sunset time Autostar Navigation ExerciseNavigating Autostar Entering Data into AutostarSelect Item Object Autostars MenusObject Menu MenusGlossary Menu Event MenuUtilities Menu LXD55-SeriesEnter Setup MenuObserving Considerations Setup Menu Daylight SAVING, Surf the Web To Add a Site to the user-defined site list Adding Observing SitesTo Edit a Site To GO to a user-entered object Using Autostar to Find Objects Not in the LibrariesLandmarks Observing SatellitesTo Add a landmark to the database To Select a landmark from the database To Check on the Available MemoryTo perform a Landmark Survey Few tips on photography with the LXD55-Seriestelescopes Photography10 f/4 Optional AccessoriesSeries 4000 Photo-Visual Page General Maintenance MaintenanceD e f g Page Defocused star images. Misaligned 1, 2, Aligned Inspecting the Optics Meade Customer Service5 Model SN-6, SN-6EC Specifications Specifications4 Model SN-8, SN-8EC Specifications 9.3 Model AR-5, AR-5EC Specifications 10 f/4 Model SN-10 Specifications8 Model AR-6 Specifications Autostar Specifications 10 Model SC-8 SpecificationsAutostar Dimensions Appendix a Celestial Coordinates Setting CirclesOne- and Two-Star Polar Alignment Locating the Celestial PoleOne-Star Polar Alignment Two-Star Polar AlignmentProcedure #1 To correct for attitude misalignment Axis Alignment ProcedurePolar Alignment Viewfinder Method 1 Manual AlignmentPosition a Procedure #2 To correct for elevation misalignmentTips Star ChartsMethod 2 Axis Alignment Using Autostar Latitude Chart for Major Cities of the World Appendix C Latitude ChartCity State/Prov./Country Latitude City Country LatitudeAppendix D EC Handbox Modes of Operation To move the telescope using the Electronic ControllerSlew Speeds Tracking Rates Optional Autostar Computer Controller for LXD55 EC Users Changing the Polar ModeMounting the SC bracket and optical tube to the mount How to Attach the Optical Tube to the MountAutostar Glossary Appendix F Basic AstronomyObjects in Space MoonDeep-Sky Objects PlanetsFurther Study Page Meade Instruments Corporation