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11

OBSERVING THE  SKY

Sky conditions are usually defined by two atmospheric characteristics, seeing, or the steadiness of the air, 
and transparency, light scattering due to the amount of water vapour and particulate material in the air. When 
you observe the Moon and the planets, and they appear as though water is running over them, you probably 
have bad "seeing" because you are observing through turbulent air. In conditions of good "seeing", the stars 
appear steady, without twinkling, when you look at them with unassisted eyes (without a telescope). Ideal 
"transparency" is when the sky is inky black and the air is unpolluted.

S

ky conditions

S

electing an observing site

C

hoosing the best time to observe

C

ooling the telescope

Travel to the best site that is reasonably accessible. It should be away from city lights, and upwind from any 
source of air pollution. Always choose as high an elevation as possible; this will get you above some of the 
lights and pollution and will ensure that you aren't in any ground fog. Sometimes low fog banks help to block 
light pollution if you get above them. Try to have a dark, unobstructed view of the horizon, especially the 
southern horizon if you are in the Northern Hemisphere and vice versa. However, remember that the darkest 
sky is usually at the "Zenith", directly above your head. It is the shortest path through the atmosphere. Do not 
try to observe any object when the light path passes near any protrusion on the ground. Even extremely light 
winds can cause major air turbulence as they flow over the top of a building or wall. 

Observing through a window is not recommended because the window glass will distort images considerably. 
And an open window can be even worse, because warmer indoor air will escape out the window, causing 
turbulence which also affects images. Astronomy is an outdoor activity.

The best conditions will have still air, and obviously, a clear view of the sky. It is not necessary that the sky be 
cloud-free. Often broken cloud conditions provide excellent seeing. Do not view immediately after sunset. After 
the sun goes down, the Earth is still cooling, causing air turbulence. As the night goes on, not only will seeing 
improve, but air pollution and ground lights will often diminish. Some of the best observing time is often in the 
early morning hours. Objects are best observed as they cross the meridian, which is an imaginary line that runs 
through the Zenith, due North-South. This is the point at which objects reach their highest points in the sky. 
Observing at this time reduces bad atmospheric effects. When observing near the horizon, you look through 
lots of atmosphere, complete with turbulence, dust particles and increased light pollution.

Telescopes require at least 10 to 30 minutes to cool down to outside air temperature. This may take longer if 
there is a big difference between the temperature of the telescope and the outside air. This minimizes heat 
wave distortion inside telescope tube (tube currents). Allow a longer cooling time for larger optics. If you are 
using an equatorial mount, use this time for polar alignment.

A

dapting your eyes

Do not expose your eyes to anything except red light for 30 minutes prior to observing. This allows your pupils 
to expand to their maximum diameter and build up the levels of optical pigments, which are rapidly lost if 
exposed to bright light. It is important to observe with both eyes open. This avoids fatigue at the eyepiece. If 
you find this too distracting, cover the non-used eye with your hand or an eye patch. Use averted vision on 
faint objects: The center of your eye is the least sensitive to low light levels. When viewing a faint object, don't 
look directly at it. Instead, look slightly to the side, and the object will appear brighter.

Содержание SK 763 EQ/TA

Страница 1: ...SK 763 EQ TA SK 804 EQ TA SK MAK90 EQ TA SK 8035 EQ TA TABLETOP TELESCOPES...

Страница 2: ...ope Main Tube Focuser Knob Focuser Tube Finderscope adjustment screw Dust cap mask remove before viewing SK 80 400 EQ TA Dust Cap Mask Remove before Viewing Dew Cap Sun Shade Dec Scale R A Axis Scale...

Страница 3: ...ONTENTS Caution Before you begin This instruction manual is applicable to all the models listed on the cover Take a moment to find the model number of your telescope on page 2 Follow the instructions...

Страница 4: ...hole on the end of the declination shaft 2 Unscrew the threaded cap from the end of the counterweight rod INSTALLING THE COUNTER WEIGHT Fig 8 1 Slide the counterweight halfway along counterweight rod...

Страница 5: ...he desired eyepiece and re tighten thumb screws to hold eyepieces in place Fig 12 Fig 10 ATTACHING THE TELESCOPE MAIN TUBE TO THE MOUNT Fig 10 1 Place the telescope tube on the mount secure with the 2...

Страница 6: ...the variable brightness control clockwise until you hear a click Continue rotating the control knob to increase the brightness level Insert a low power eyepiece into the telescope s focuser Locate a...

Страница 7: ...is very near the North Celestial Pole For casual observing rough polar alignment is adequate Make sure your equatorial mount is level and the red dot finder is aligned with the telescope before beginn...

Страница 8: ...magnitude star Vega in the Constellation Lyra From a star chart we know the R A coordinate of Vega is 18h 36m Loosen the R A and DEC lock knobs on the mount and adjust the telescope so that Vega is c...

Страница 9: ...to the object you wish to observe but are not accurate enough to put it in the centre of your Red Dot Finder s finderscope s field of view The accuracy of your setting circles also depends on how accu...

Страница 10: ...l length of the eyepieces you are going to use For example a 10mm focal length eyepiece will give 80X magnification with an 800mm focal length telescope To put this in perspective the moon is about 0...

Страница 11: ...e which also affects images Astronomy is an outdoor activity The best conditions will have still air and obviously a clear view of the sky It is not necessary that the sky be cloud free Often broken c...

Страница 12: ...cm x 23cm Super 25mm Super 10mm 90 2X The sky is mapped out in a spherical coordinate system similar to the system of Latitude and Longitude on the surface of the Earth On the imaginary celestial sphe...

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