Celestron 21035 User Manual
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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. 
 
 
 
 
 
 
 
