Meade LX200GPS instruction manual Planets, Deep-Sky Objects

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Tip:

Enter a date in the Date menu and you can deter- mine if a planet(s) will be visible during the night of the entered date by check- ing its rise and set times.

Fig. 60: A favorite winter sight—the great nebula in Orion.

Fig. 61: The Pleiades is one of the most beautiful open clusters.

Fig. 62: The Andromeda Galaxy, the largest galaxy of our local group.

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 II 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. Listed below are the best planets for viewing through the LX200GPS.

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 11 times the diameter of Earth. Jupiter (Fig. 58) appears as a disk with dark lines stretching across the surface. 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 vis- ible 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. 59). 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 LX200GPS. 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 just some of the deep-sky objects you'll be able to observe with your LX200GPS 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) (Fig. 60), 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. 61). Through the LX200GPS, 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) (Fig. 62) 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 Meade Maksutov-Cassegrain Optical System Meade Schmidt-Cassegrain Optical SystemContents QUICK-START Guide Important Note Autostar Telescope FeaturesTelescope? See pages 17 See Optional ACCESSORIES, pages 41, 42,Ascension Declination setting # Computer Control Panel see insetAscension, DefinitionsShift Microfocuser? Tour the Cosmos with Just the Push of a Button Autostar II FeaturesLibrary # of Objects Want to learn more about changing slew speeds? See LX200GPS Tips How to Attach the Tripod to the Telescope Assembly Parts ListingGetting Started To install batteries How to Assemble Your TelescopeTip Choosing an Eyepiece Attach Diagonal or accessoriesToo Much Power? Mounting and Adjusting the ViewfinderTerrestrial Observing Observing Using Autostar IIs Arrow KeysObserving Observing by Moving the Telescope ManuallyKey # Speed Focusing the Eyepiece Using the MicrofocuserSlew Speeds To use the microfocuserMoving Through Autostar II’s Menus Observe the MoonAstronomical Observing To Track an Object AutomaticallyImportant Notes Which One’s the Alignment Star?Using the Guided Tour Observe a Star using the Automatic Tracking FeatureGo To Saturn Detecting True Level Global Positioning SystemFinding True North Autostar II Navigation Exercise Basic AutostarTo Calculate Sunset time Look into the Future Navigating AutostarSelect Item Object MenusTo slew the telescope to catalog objects Object MenuWant to learn more about Observing Satellites? See Event Menu Want to learn more about using the Browse menu? SeeUtilities Menu Glossary MenuWant to learn more about Landmarks? See Timing is Everything Setup MenuRECTION, Adding and editing sites? Setup Menu Daylight SAVING,Mirror, Mirror Hot Button MenusTo Add a Site to the user-defined site list Adding Observing SitesTo Edit a Site To GO to a user-entered object Creating User ObjectsTips Observing SatellitesLandmarks To Add a landmark to the databaseTo check on the available amount of memory in Autostar IdentifyTo Select a landmark from the database To perform a Landmark SurveyDisplayed information Example BrowseEasy Two-Star Alignment How to perform the Easy Align ProcedureAlternate Alt/Az Alignments Initialize AutostarTo Set the Home Position Manually One-Star Alt/Az AlignmentTip Try a Spiral Search Star Charts Periodic Error CorrectionFew tips on photography with the LX200GPS telescopes PhotographyMeade Series 4000 Eyepieces Optional AccessoriesSeries 4000 8 24mm Zoom Eyepiece Illuminated Reticle Eyepiece Collimation MaintenanceDefocused star images. Misaligned 1, 2, Aligned Gauging the Movement of the Telescope Meade Customer ServiceWhat is Smart Drive? Inspecting the Optics15 LX200GPS Specifications SpecificationsMaksutov Fan 10 f/10 LX200GPS Specifications 10 LX200GPS Specifications12 f/10 LX200GPS Specifications Autostar II System Specifications 16 f/10 LX200GPS SpecificationsAutostar II Handbox Specifications Equatorial Alignment Setting CirclesCelestial Coordinates Equatorial Wedge Declination Setting CircleLocating Polaris Lining Up with the Celestial PoleLX200GPS mounted on an equatorial wedge Precise Polar AlignmentTwo-Star Polar Alignment Autostar II Polar AlignmentEasy Polar Alignment One-Star Polar AlignmentCity Country Latitude Appendix B Latitude ChartLatitude Chart for Major Cities of the World City State/Prov./Country LatitudeComment Line Command LineWhat you will need Tour ModesTitle Writing a TourPick ONE / Pick END Further Study Appendix D Training the DriveAppendix E the Moon Menu To observe the Apollo 15 landing site using the Moon optionControl Panel Features 16 LX200GPS Unique FeaturesCommercial Shipping To Assemble the 16 Super Field Tripod Telescope AssemblyAttaching the Fork Mounting the Optical Tube Assembly OTAAttaching the Power and Data Cords Attaching the 16 Drive BaseObserving Considerations Tighten the fork arm assem- bly using the provided hex keyTo attach the microfocuser to the de-rotater Appendix GMoon Basic AstronomyAutostar II Glossary Objects in SpaceDeep-Sky Objects PlanetsPage Meade Instruments Corporation
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