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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.

 

 
 

 

 

 
 

Summary of Contents for FirstScope 21024

Page 1: ...F Fi ir rs st tS Sc co op pe e I In ns st tr ru uc ct ti io on n M Ma an nu ua al l M Mo od de el l 2 21 10 02 24 4...

Page 2: ...General Observing Hints 7 The Celestial Coordinate System 8 Motion of the Stars 9 CELESTIAL OBSERVING 10 Observing the Moon 10 Lunar Observing Hints 10 Observing the Planets 10 Observing Deep Sky Obje...

Page 3: ...and easy set up Take time to read through this manual before embarking on your journey through the Universe It may take a few observing sessions to become familiar with your telescope so you should ke...

Page 4: ...4 Figure 1 1 1 Focuser 6 Arm 2 Secondary Diagonal Mirror inside 7 Tube End 3 Optical Tube 8 Primary Mirror inside 4 Lock Nut 9 Focus Knob 5 Base 10 Eyepiece 10 9 8 7 6 5 4 3 2 1...

Page 5: ...er see the section on Calculating Magnification The eyepiece fits directly into the focuser To attach the eyepieces 1 Make sure the thumbscrews are not protruding into the focuser tube Then insert the...

Page 6: ...ll enjoy a telescope that is relatively compact and portable A Newtonian Reflector telescope offers such impressive light gathering characteristics you can take a serious interest in deep space astron...

Page 7: ...t you are observing To calculate the actual field of view divide the apparent field of the eyepiece supplied by the eyepiece manufacturer by the magnification In equation format the formula looks like...

Page 8: ...rth and separates the northern celestial hemisphere from the southern Like the Earth s equator it bears a reading of zero degrees On Earth this would be latitude However in the sky this is referred to...

Page 9: ...use the sunlight during the day washes out the starlight However part of this circular motion of stars in this region of the sky can be seen by setting up a camera on a tripod and opening the shutter...

Page 10: ...see the moons of Jupiter as they orbit the giant planet Saturn with its beautiful rings is easily visible at moderate power Planetary Observing Hints y Remember that atmospheric conditions are usually...

Page 11: ...than you can with the naked eye y Binoculars a helpful tool in locating bright stars and searching an area you are looking for objects in Can be a substitute or supplement to a finderscope y Books sev...

Page 12: ...necting 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 r...

Page 13: ...ound 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...

Page 14: ...ted If moisture condenses on the inside of the optics remove the accessories from the telescope Place the telescope in a dust free environment and point it down This will remove the moisture from the...

Page 15: ...osed on the primary mirror Figure 6 2 If the primary mirror is not centered in the secondary mirror adjust the secondary mirror screws by alternately tightening and loosening them until the mirror is...

Page 16: ...Length 300mm Focal Ratio f 4 Optical Coatings Coated Eyepieces 1 25 Barrel 20mm 15x 4mm 75x Apparent FOV 20mm 25 and 4mm 33 Angular Field of View w 20mm eyepiece 1 7 Linear FOV w 20mm ft 1000yds m 10...

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