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Viewing conditions affect what you can see through your telescope during an observing session.  Conditions include transparency, sky illumination, and seeing.  
Understanding viewing conditions and the effect they have on observing will help you get the most out of your telescope. 

 

Transparency 

 

Transparency is the clarity of the atmosphere which is affected by clouds, moisture, and other airborne particles.  Thick cumulus clouds are completely opaque while 
cirrus can be thin, allowing the light from the brightest stars through.  Hazy skies absorb more light than clear skies making fainter objects harder to see and reducing 
contrast on brighter objects.  Aerosols ejected into the upper atmosphere from volcanic eruptions also affect transparency.  Ideal conditions are when the night sky is 
inky black. 
 

Sky Illumination 

 

General sky brightening caused by the Moon, aurorae, natural airglow, and light pollution greatly affect transparency.  While not a problem for the brighter stars and 
planets, bright skies reduce the contrast of extended nebulae making them difficult, if not impossible to see.  To maximize your observing, limit deep sky viewing to 
moonless nights far from the light polluted skies found around major urban areas.  LPR filters enhance deep sky viewing from light polluted areas by blocking 
unwanted light while transmitting light from certain deep sky objects.  You can, on the other hand, observe planets and stars from light polluted areas or when the Moon 
is out. 

 

Seeing 

 

Seeing conditions refers to the stability of the atmosphere and directly affects the amount of fine detail seen in extended objects.  The air in our atmosphere acts as a 
lens which bends and distorts incoming light rays.  The amount of bending depends on air density.  Varying temperature layers have different densities and, therefore, 
bend light differently.  Light rays from the same object arrive slightly displaced creating an imperfect or smeared image.  These atmospheric disturbances vary from 
time-to-time and place-to-place.  The size of the air parcels compared to your aperture determines the "seeing" quality.  Under good seeing conditions, fine detail is 
visible on the brighter planets like Jupiter and Mars, and stars are pinpoint images.  Under poor seeing conditions, images are blurred and stars appear as blobs.   
 
The conditions described here apply to both visual and photographic observations. 

 
 
 
 
 
 

Figure 5-3 

Seeing conditions directly affect image quality.  These drawings represent a point source (i.e., star) under bad 
seeing conditions (left) to excellent conditions (right).  Most often, seeing conditions produce images that lie 
somewhere between these two extremes. 

ASTROPHOTOGRAPHY

 

The PowerSeeker series of telescopes was designed for visual observing.  After looking at the night sky for a while you may want to try your hand at photography of it. 
There are a few simple forms of photography possible with your telescope for celestial pursuits although celestial photography is best done using an equatorial mount or 
computerized altazimuth mount.  Below is just a very brief discussion of some of the methods of photography available and suggest you search out various books for 
detailed information on the subject matter. 

 

As a minimum you will need a digital camera or 35mm (D)SLR camera.  Attach your camera to the telescope with: 

 

Digital camera – you will need the Universal Digital Camera Adapter (# 93626).  The adapter allows the camera to be mounted rigidly prime focus 
astrophotography. 

 

35mm (D)SLR camera – you will need to remove your lens from the camera and attach a T-Ring for your specific camera brand.  Then, you will need a T-Adapter 
(# 93625) to attach on one end to the T-Ring and the other end to the telescope focus tube. Your telescope is now the camera lens. 

 

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Short exposure prime focus photography is the best way to begin imaging celestial objects.  It is done by attaching your camera to the telescope as described in the 
paragraph above.  A couple of points to keep in mind: 

 

You can image the Moon as well as the brighter planets with very short exposures.  You will have to experiment with various settings and exposure times.  Much 
information can be obtained from your camera instruction manual which can supplement what you can find in detailed books on the subject matter. 

 

Do your photography from a dark sky observing site if possible. 

 

Remember, this is just very simple photography.  For more detailed and serious astrophotography you need an equatorial mount or a computerized altazimuth 
mount. 

 

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During the last few years a new technology has evolved which makes taking superb images of the planets and moon relatively easy and the results are truly amazing.  
Celestron offers the NexImage (# 93712) which is a special camera and included is software for image processing.  You can capture planetary images your first night 
out which rivals what professionals were doing with large telescopes just a few short years ago. 

 

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Special cameras have been developed for taking images of deep sky images.  These have evolved over the last several years to become much more economical and 
amateurs can take fantastic images.  Several books have been written on how to get the best images possible.  The technology continues to evolve with better and easier 
to use products on the market. 
 

Summary of Contents for 21056-K

Page 1: ...P Po ow we er rS Se ee ek ke er r 1 11 14 4A AZ Z T Te el le es sc co op pe e INSTRUCTION MANUAL Model 21056 K ENGLISH ...

Page 2: ...y The PowerSeeker 114AZ carries a two year limited warranty For details see our website at www celestron com Some of the many standard features of the PowerSeeker include All coated glass optical elements for clear crisp images Smooth functioning rigid altazimuth mount with easy pointing to located objects Preassembled aluminum tripod ensures a stable platform Quick and easy no tool set up CD ROM ...

Page 3: ...pright and pull the tripod legs apart until each leg is fully extended and then push down slightly on the tripod leg brace Figure 2 2 The very top of the tripod is called the tripod head AZ mount 3 Next we will install the tripod accessory tray Figure 2 3 onto the tripod leg brace center of Figure 2 2 4 On the bottom of the tripod tray is a screw attached to the center The screw attaches into a th...

Page 4: ...d and into the mechanism and tighten it 3 Thread the altitude locking knob out so the hole is clear in the eyebolt see Figure 2 8 4 Put the rod of the assembly through the eyebolt and then tighten the altitude locking knob Figure 2 9 5 Thread the two knobs one on either side of the mount through the top of the mount into the threaded holes in the optical tube and tighten Figure 2 7 Figure 2 7 Figu...

Page 5: ...be easier to focus Figure 2 12 I In ns st ta al ll li in ng g t th he e S St ta ar rP Po oi in nt te er r F Fi in nd de er rs sc co op pe e The Star Pointer is the quickest and easiest way to point your telescope exactly at a desired object in the sky It s like having a laser pointer that you can shine directly onto the night sky The Star Pointer is a zero magnification pointing tool that uses a c...

Page 6: ...e back end There light is bent forward in the tube to a single point its focal point Since putting your head in front of the telescope to look at the image with an eyepiece would keep the reflector from working a flat mirror called a diagonal intercepts the light and points it out the side of the tube at right angles to the tube The eyepiece is placed there for easy viewing Newtonian Reflector tel...

Page 7: ... G Ge en ne er ra al l O Ob bs se er rv vi in ng g H Hi in nt ts s When using any optical instrument there are a few things to remember to ensure you get the best possible image Never look through window glass Glass found in household windows is optically imperfect and as a result may vary in thickness from one part of a window to the next This inconsistency can and will affect the ability to focu...

Page 8: ...e sky Stars near the celestial equator form the largest circles rising in the east and setting in the west Moving toward the north celestial pole the point around which the stars in the northern hemisphere appear to rotate these circles become smaller Stars in the mid celestial latitudes rise in the northeast and set in the northwest Stars at high celestial latitudes are always above the horizon a...

Page 9: ...elescope For safe solar viewing use a proper solar filter that reduces the intensity of the Sun s light making it safe to view With a filter you can see sunspots as they move across the solar disk and faculae which are bright patches seen near the Sun s edge The best time to observe the Sun is in the early morning or late afternoon when the air is cooler To center the Sun without looking into the ...

Page 10: ...ine connecting the two stars 6 Look through the telescope and the Ring Nebula should be in your field of view The Ring Nebula s angular size is quite small and difficult to see 7 Because the Ring Nebula is rather faint you may need to use averted vision to see it Averted vision is a technique of looking slightly away from the object you re observing So if you are observing the Ring Nebula center i...

Page 11: ...owerSeeker series of telescopes was designed for visual observing After looking at the night sky for a while you may want to try your hand at photography of it There are a few simple forms of photography possible with your telescope for celestial pursuits although celestial photography is best done using an equatorial mount or computerized altazimuth mount Below is just a very brief discussion of ...

Page 12: ...stortions Before collimating your telescope take time to familiarize yourself with all its components The primary mirror is the large mirror at the back end of the telescope tube This mirror is adjusted by loosening and tightening the three screws placed 120 degrees apart at the end of the telescope tube The secondary mirror the small elliptical mirror under the focuser in the front of the tube al...

Page 13: ...to use a longer focal length ocular with a Barlow lens When a star is in focus it should look like a sharp pinpoint of light If when focusing on the star it is irregular in shape or appears to have a flare of light at its edge this means your mirrors aren t in alignment If you notice the appearance of a flare of light from the star that remains stable in location just as you go in and out of exact...

Page 14: ...o preserve night vision better than red filters or other devices Brightness is adjustable Operates on a single 9 volt included battery Collimation Tool 94183 Collimating your Newtonian telescope is easily accomplished with this handy accessory which includes detailed instructions Collimation Eyepiece 1 25 94182 The collimation eyepiece is ideal for precise collimation of Newtonian telescopes Digit...

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