Orion XT8, XT6, XT10 instruction manual Moon, Sun, Planets, Stars, Deep-Sky Objects

Page 16

lower powers. It is quite common for an observer to own five or more eyepieces to access a wide range of magnifications. This allows the observer to choose the best eyepiece to use depending on the object being viewed. At least to begin with, the two supplied eyepieces will suffice nicely.

Whatever you choose to view, always start by inserting your lowest-power (longest focal length) eyepiece to locate and center the object. Low magnification yields a wide field of view, which shows a larger area of sky in the eyepiece. This makes acquiring and centering an object much easier. If you try to find and center objects with high power (narrow field of view), it’s like trying to find a needle in a haystack!

Once you’ve centered the object in the eyepiece, you can switch to higher magnification (shorter focal length eyepiece), if you wish. This is especially recommended for small and bright objects like planets and double stars. The Moon also takes higher magnifications well.

Deep-sky objects, however, typically look better at medium or low magnifications. This is because many of them are quite faint, yet have some extent (apparent width). Deep-sky objects will often disappear at higher magnifications, since greater magnification inherently yields dimmer images. This is not the case for all deep-sky objects, however. Many galax- ies are quite small, yet are somewhat bright, so higher power may show more detail.

The best rule of thumb with eyepiece selection is to start with a low power, wide field, and then work your way up in magnification. If the object looks better, try an even higher magnification. If the object looks worse, then back off the magnification a little by using a lower power eyepiece.

A. The Moon

With is rocky and cratered surface, the Moon is one of the most interesting and easy subjects to view with your scope. The best time to view it is during its partial phases when shadows fall on the craters and canyon walls to give them definition. While the full moon may look like a tempting target, it is not optimal for viewing! The light is too bright and surface definition is low.

Even at partial phases the Moon is very bright. Use of an optional Moon filter to helps to dim the glare. It simply threads onto the bottom of the eyepiece. You’ll find the Moon filter improves viewing comfort, and helps bring out the subtle fea- tures of the lunar surface.

B. The Sun

You can change your nighttime telescope into a daytime Sun viewer by installing an optional full-aperture solar filter over the front opening of the telescope. The primary attraction is sunspots, which change shape, appearance, and location daily. Sunspots are directly related to magnetic activity in the Sun. Many observers like to make drawings of sunspots to monitor how the Sun is changing from day to day.

Important Note: Do not look at the Sun with any optical instrument without a professionally made solar filter, or permanent eye damage could result. Also, be sure to cover the finder scope, or better yet, remove it altogether.

C. The Planets

The planets don’t stay put like the stars, so to find them you should refer to Sky Calendar at our website telescope.com, or to charts published monthly in Astronomy, Sky & Telescope, or other astronomy magazines. Venus, Mars, Jupiter, and Saturn are the brightest objects in the sky after the Sun and the Moon. Your SkyQuest IntelliScope is capable of showing you these planets in some detail. Other planets may be visible but will likely appear starlike. Because planets are quite small in apparent size, optional higher power eyepieces are recom- mended and often needed for detailed observations. Not all the planets are generally visible at any one time.

JUPITER The largest planet, Jupiter, is a great subject for observation. You can see the disk of the giant planet and watch the ever-changing positions of its four largest moon: Io, Callisto, Europa, and Ganymede. Higher power eyepieces should bring out the cloud bands on the planet’s disk and the Great Red Spot.

SATURN The ringed planet is a breathtaking sight. The tilt angle of the rings varies over a period of many years; some- times they are seen edge-on, while at other times they are broadside and look like giant “ears” on each side of Saturn’s disk. A steady atmosphere (good seeing) is necessary for a good view. Look closely and you should see the Cassini divi- sion, a thin, dark gap in the rings. You should also see one or more of Saturn’s moons, which look like faint stars. The brightest is the moon Titan.

VENUS At its brightest, Venus is the most luminous object in the sky, excluding the Sun and the Moon. It is so bright that sometimes it is visible to the naked eye during full daylight! Ironically, Venus appears as a thin crescent, not a full disk, when at its peak brightness. Because it is so close to the Sun, it never wanders too far from the morning or evening horizon. No surface markings can be seen on Venus, which is always shrouded in dense clouds.

MARS The Red Planet makes a close approach to Earth every two years. Observing Mars is most favorable at these times. You should see salmon-colored disk with some distinct dark patches, and you may be able to spot a whitish polar ice cap. To see surface detail on Mars, you will need a high power eyepiece and very steady air!

D. The Stars

Stars will appear as tiny points of light. Even powerful tele- scopes cannot magnify stars to appear as anything more than pinpoints. You can, however, enjoy the different colors of the stars and locate many pretty double and multiple stars. The famous “Double-Double” in the constellation Lyra and the gor- geous two-color double star Albireo in Cygnus are favorites. Defocusing a star slightly can help bring out its color.

E. Deep-Sky Objects

Under dark skies, you can observe a wealth of fascinating deep-sky objects; that is, objects that reside outside of our solar system. These include gaseous nebulas, open and globular star clusters, and a variety of different types of galax- ies. The large apertures of SkyQuest IntelliScope Dobsonians are particularly well suited to gathering light, which is critical

16

Image 16
Contents XT6, XT8, XT10 #9985, #9986, #9987SkyQuest XT8 IntelliScope Parts List Table of ContentsUnpacking Assembly Assembly of the Dobsonian BaseInstalling the Vertical Stop Correct Tension padsInstalling the CorrecTension Friction Optimization System Installing the Eyepiece RackPlacing the Optical Tube on the Dobsonian Base Installing the Finder Scope Does not require this bushingInserting an Eyepiece Using Your TelescopeAltitude and Azimuth Motion Setting the Altitude Tension Level Focusing the TelescopeViewing with Eyeglasses Aligning the Finder ScopeFocusing the Finder Scope Aiming/Pointing the TelescopeMagnification 1200 mm = 25 mmTube Balance Use of 2-Inch Eyepieces XT8 and XT10 onlyCarrying the Telescope Collimation Cap and Mirror Center Mark Alignment Collimation of the Optical SystemPreparing the Telescope for Collimation Adjusting the Primary Mirror Aligning the Secondary MirrorStar-Testing the Telescope Astronomical ObservingSelecting an Observing Site Seeing and TransparencyLet Your Eyes Dark-Adapt Eyepiece SelectionMoon SunPlanets StarsCare and Maintenance Optional IntelliScope Computerized Object LocationCleaning Eyepiece Lenses Cleaning MirrorsSpecifications SkyQuest XT6 IntelliScopeSkyQuest XT8 IntelliScope SkyQuest XT10 IntelliScopeOne-Year Limited Warranty
Related manuals
Manual 20 pages 35.54 Kb