Celestron Advanced Series GT, C6-RGT manual Finding the North Celestial Pole

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Remember, while Polar aligning, do NOT move the telescope in R.A. or DEC. You do not want to move the telescope itself, but the polar axis. The telescope is used simply to see where the polar axis is pointing.

Like the previous method, this gets you close to the pole but not directly on it. The following methods help improve your accuracy for more serious observations and photography.

Finding the North Celestial Pole

In each hemisphere, there is a point in the sky around which all the other stars appear to rotate. These points are called the celestial poles and are named for the hemisphere in which they reside. For example, in the northern hemisphere all stars move around the north celestial pole. When the telescope's polar axis is pointed at the celestial pole, it is parallel to the Earth's rotational axis.

 

Many methods of polar alignment require that you know how to find the celestial pole by

 

identifying stars in the area. For those in the northern hemisphere, finding the celestial pole is

 

not too difficult. Fortunately, we have a naked eye star less than a degree away. This star,

 

Polaris, is the end star in the handle of the Little Dipper. Since the Little Dipper (technically

 

called Ursa Minor) is not one of the brightest constellations in the sky, it may be difficult to

 

locate from urban areas. If this is the case, use the two end stars in the bowl of the Big Dipper

 

(the pointer stars). Draw an imaginary line through them toward the Little Dipper. They point

 

to Polaris (see Figure 5-5). The position of the Big Dipper changes during the year and

 

throughout the course of the night (see Figure 5-4). When the Big Dipper is low in the sky

 

(i.e., near the horizon), it may be difficult to locate. During these times, look for Cassiopeia

 

(see Figure 5-5). Observers in the southern hemisphere are not as fortunate as those in the

 

northern hemisphere. The stars around the south celestial pole are not nearly as bright as those

 

around the north. The closest star that is relatively bright is Sigma Octantis. This star is just

Definition

within naked eye limit (magnitude 5.5) and lies about 59 arc minutes from the pole.

 

The north celestial pole is the point in the northern hemisphere around which all

 

stars appear to rotate. The counterpart in the southern hemisphere is referred to as

 

the south celestial pole.

Figure 5-4 The position of the

Big Dipper changes

throughout the year and the

night.

Figure 5-5

The two stars in the front of the bowl of the Big Dipper point to Polaris which is less than one degree from the true (north) celestial pole. Cassiopeia, the “W” shaped constellation, is on the opposite side of the pole from the Big Dipper. The North Celestial Pole (N.C.P.) is marked by the “+” sign.

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Contents Advanced Series Advanced Series GT Assembly Version Get Alt-Az Goto Alt-Az Hibernate Turn On/Off GPS Page C8-N Shown Advanced Series C6-RAdvanced Series C6-RGT Attaching the Equatorial Mount Setting up the TripodAttaching the Center Leg Brace Installing the Counterweight BarAttaching the Hand Control Holder Advanced GT Models Only Installing the CounterweightAttaching the Telescope Tube to the Mount Installing the Finderscope Telescope Tube Completely Balancing the Tube in R.AAdjusting the Mount in Altitude Adjusting the MountAttaching the Declination Cable For GT Models Only Adjusting the Mount in AzimuthPowering the Telescope Advanced GT Hand Control Double Stars Hand Control OperationStartup Procedure Alignment ProceduresAuto Three-Star Align Auto AlignRe-Alignment Quick-AlignLast Alignment Finding Planets Object CatalogSelecting an Object Slewing to an ObjectRate Button Tour ModeConstellation Tour Direction ButtonsSetup Procedures Identify Precise GoTo Scope Setup FeaturesObserving Tip Helpful Hint Utility Features Helpful Hint Advanced GT Image Orientation Calculating Magnification FocusingAligning the Finderscope General Observing Hints Determining Field of View Celestial Coordinate System Motion of the Stars Pointing at Polaris Finding the North Celestial Pole Declination Drift Method of Polar Alignment Observing the Sun Observing the MoonLunar Observing Hints Observing the PlanetsTransparency Solar Observing HintsObserving Deep Sky Objects Seeing ConditionsUsing the Lens Cap Aperture Stop Piggyback Short Exposure Prime Focus Photography Reducing Vibration Terrestrial PhotographyMetering Auto Guiding Collimation Care and Cleaning of the OpticsCollimated telescope Should appear as a Page Page Page Appendix a Technical Specifications Appendix B Glossary of Terms Page Eclipsing or obscuring the brightness of the star Appendix C Longitudes Latitudes Georgia Minnesota Rhode Island Canada Appendix D RS-232 Connection Additional RS232 Commands Appendix E Maps of Time Zones Page Page Page Page Page Page Page Celestron TWO Year Warranty
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