APM SK P25012EQ6-2IN Instruction Manual Download Page 14

14

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.

Summary of Contents for SK P25012EQ6-2IN

Page 1: ...SK P25012EQ6 2IN...

Page 2: ...Newtonian reflector Cleaning Your Telescope 3 6 3 4 4 4 5 5 5 6 6 7 7 8 8 8 9 11 12 13 14 14 14 14 14 15 16 14 15 Before you begin Caution Read the entire instructions carefully before beginning Your...

Page 3: ...unterweight Rod Lock Knob Counterweight Thumbscrew Counterweight Counterweight Rod Hand Control Finderscope Bracket Alignment Screw Focus Locking Screw Piggyback Bracket Tube Rings Pirmary Mirror Posi...

Page 4: ...led knob underneath to secure mount to tripod Fig 3 Fig 4 Fig 5 TRIPOD SET UP Fig 2 Note Loosen the azimuth adjustment knobs if mount does not fit into tripod head completely Retighten knobs to secure...

Page 5: ...2 Find the center of balance of the telescope tube Place this in between the two tube rings Close the hinges around the telescope and fasten securely by tightening the thumb nuts TELESCOPE ASSEMBLY Fi...

Page 6: ...anced after all accessories eyepiece camera etc have been attached Before balancing your telescope make sure that your tripod is balanced and on a stable surface For photography point the telescope in...

Page 7: ...ontrol buttons R A control buttons N OFF S 2X 8X 16X Dec Dec R A R A R A The N Off S switch acts as a power switch as well as controlling the directions of the motors The N position allows R A motor t...

Page 8: ...n the sky you have to align your mount This means tilting the head over so that it points to the North or South celestial pole For people in the Northern Hemisphere this is rather easy as the bright s...

Page 9: ...e polar alignment This method of polar alignment is sufficient for virtually all visual use of the telescope To use the Polarscope with the EQ 6 mount the declination axis must be rotated such that th...

Page 10: ...ou should be able to align the reticle with the R A axis to within about 2 or 3 arc minutes You should never have to make this adjustment again unless the polar scope has been dropped disassembled or...

Page 11: ...the celestial pole Due to its proper motion Polaris can be seen to move with respect to the Pole from year to year The tick marks in the Polarscope can be used to compensate for this motion Fig h 5 c...

Page 12: ...DEC lock knobs to lock the mount in place Now rotate the R A setting circle until it reads 18h36m Your are now ready to use the setting circles to find objects in the sky Finding objects using the set...

Page 13: ...pe in mm by the magnification Exit Pupil Diameter of Primary mirror in mm Magnification For example a 200mm f 5 telescope with a 40mm eyepiece produces a magnification of 25x and an exit pupil of 8mm...

Page 14: ...lso 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 cond...

Page 15: ...p which covers the front of the telescope and look down the optical tube At the bottom you will see the primary mirror held in place by three clips 120 apart and at the top the small oval secondary mi...

Page 16: ...ew there If there is you will want to loosen it turn the screw to the left to bring the mirror away from that point If there isn t a adjusting screw there then go across to the other side and tighten...

Reviews: