Meade LX90 instruction manual Planets, Deep-Sky Objects

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Fig. 38: Jupiter and its four largest moons. The moons can be observed in a different position every night.

Fig. 39: Saturn has the most extensive ring structure in our Solar System.

Fig. 40: 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 planets 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 planets. 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 planet(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 LX90.

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. The plan- et appears as a disk with dark lines stretching across the surface. These lines are cloud bands in the atmosphere. Four of Jupiter’s 16 moons (Io, Europa, Ganymede, and Callisto) can be seen as “star-like” points of light when using even the lowest magnification (Fig. 38). 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. 39). 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 visible through the LX90. Titan, the largest of Saturn’s 18 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 pinpoints 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. 40). Through the LX90, 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 LX90 Schmidt-Cassegrain Telescope Meade Schmidt-Cassegrain Optical System Contents QUICK-START Guide ON/OFF Telescope Features E DPage To Attach the Handbox Holder Autostar Features Tour the Cosmos with Just the Push of a ButtonTopmost screen Select Item Object Page How to Attach the Tripod to the Telescope Assembly Getting StartedHow to Assemble Your Telescope Precautionary notes for the tripodUsing SmartFinder Choosing an EyepieceAligning SmartFinder Aligning the ViewfinderObserving Using AutoStars Arrow Keys ObservingObserving By Moving the Telescope Manually Terrestrial ObservingSlew Speeds Observe the MoonAstronomical Observing To Track an Object AutomaticallyMoving Through AutoStar’s Menus Initializing AutoStar for the First TimeObserve a Star using the Automatic Tracking Feature How to perform the Automatic Alignment procedureAutomatic Alignment While it does soUsing the Guided Tour Go To SaturnBasic Autostar Operation AutoStar Navigation ExerciseTo Calculate Sunset time Entering Data into AutoStarNavigating AutoStar AUTOSTAR’S Menus Select Item ObjectMenus and Menu Options Object MenuUtilities Menu Event MenuGlossary Menu Observing Considerations Setup Menu Time Zone Shift Menu Daylight SAVING, Advanced Autostar Features Adding Observing SitesTo Add a Site to the user-defined site list To Edit a SiteUsing AutoStar to Find Objects Not in the Database Observing Satellites To GO to a user-entered objectHow to Create Your Own Guided Tour Command LineWhat you will need Tour ModesWriting a Tour TitlePick END Landmarks Downloading ToursTo Add a landmark to the database To Select a landmark from the databaseIdentify Advanced Alt/Az AlignmentTo perform a Landmark Survey To check on the available amount of memory in AutoStarOne-Star Alt/Az Alignment BrowseTwo-Star Alt/Az Alignment Photography with a Digital Camera Photography with the LX90Few tips on photography with the LX90 Photography with Meade’s AutoStar Suite Meade Deep Sky ImagerOptional Accessories Eyepiece Power 2x Barlow Super Plössl 4-elementsSuper Wide Angle 6-elements Ultra Wide Angle 8-elements#62 T-Adapter Maintenance CollimationPage Gauging the Movement of the Telescope Meade Customer ServiceInspecting the Optics AutoStar Dimensions LX90 SpecificationsAutoStar Specifications Polar Alignment Celestial CoordinatesSetting Circles Locating the Celestial PoleAutoStar Polar Alignment Easy Polar AlignmentLining Up with the Celestial Pole Equatorial WedgePrecise Polar Alignment Star Charts Latitude Chart for Major Cities of the World City State/Prov./Country LatitudeCity Country Latitude City State/Country LatitudeAppendix C Training the Drive Appendix D Changing the LNT Module Battery To replace the batteryMoon AutoStar GlossaryObjects in Space Planets Deep-Sky ObjectsPage Page Page Meade Limited Warranty