background image

power switch, the power indicator light on the mount will glow
red and the power indicator light on the hand controller will
glow green. Your mount will now be moving at the sidereal
rate, which is the same rate as the sky’s apparent motion. If
the mount is properly polar aligned, it is now “tracking” the
motion of astronomical objects as the Earth rotates.

To move your telescope to a new object, loosen both the R.A.
and Dec. lock levers and move the telescope until it is pointed
in the general direction of the object you wish to view.
Retighten the R.A and Dec. lock levers. To center the object in
the eyepiece’s field of view, you will usually need to use the
hand controller.

There are four pushbuttons on the hand controller. If no but-
tons are pushed, the R.A. motor will turn the R.A. axis at side-
real rate to track the motion of the night sky. The left and right
buttons move the mount about its R.A. axis, and the up and
down buttons move the mount about its Dec. axis. The rate of
speed is determined by the rate switch at the top right of the
hand controller. If the switch is at the 2x position, the mount
will move at two times sidereal rate when the right hand but-
ton is pushed, which will cause objects to viewed in the eye-
piece to move slowly eastward. If the left button is pushed, the
drive will stop turning, which will cause objects in the eye-
piece to move slowly westward. The top and bottom bottoms
will cause the telescope to move north and south in declina-
tion at the 2x speed. Similarly, if the switch is at the 8x or 16x
position, the mount will move eight times or sixteen times
sidereal rate when a button is pushed.

The 2x sidereal rate is the best setting for making guiding cor-
rections during long-exposure astrophotography. The 8x and
16x rates are best for centering an object within the tele-
scope’s eyepiece.

Whenever any of the four buttons on the hand controller are
pressed, the LED in the center of the controller will shine red;
when the button is released, the LED will be green. Also,
when the LED starts to blink at a constant rate, its time to
change the batteries in the battery pack.

Using the R.A. and Dec. Reversal Switches

On the side of the hand controller, there are two reversal
switches, one for the R.A. axis, and one for the Dec. axis.
When these switches are flipped to the “REV” setting, the
function of the pushbuttons on the hand controller will be
reversed. The reversal switches allow you to orient the push-
buttons to the direction of the apparent movement of a guide
star in a guide scope for astrophotography.

Understanding the Setting Circles

The setting circles on an equatorial mount (Figure 12) enable
you to locate celestial objects by their “celestial coordinates”.
Every object resides in a specific location on the “celestial
sphere”. That location is denoted by two numbers: its right
ascension (R.A.) and declination (Dec.). In the same way,
every location on Earth can be described by its longitude and
latitude. Right ascension is similar to longitude on Earth, and
declination is similar to latitude. The R.A. and Dec. values for
celestial objects can be found in any star atlas or star catalog.

The R.A. setting circle is scaled in hours, from 1 through 24,
with small marks in between representing 10-minute incre-
ments (there are 60 minutes in 1 hour of right ascension). The
lower set of numbers apply to viewing in the Northern
Hemisphere, while the numbers above them apply to viewing
in the Southern Hemisphere.

The Dec. setting circle is scaled in degrees, with each mark
representing 2° increments. Values of declination coordinates
range from +90° to -90°. The 0° mark indicates the celestial
equator. When the telescope is pointed north of the celestial
equator, values of the declination setting circle are positive;
when the telescope is pointed south of the celestial equator,
values of the declination setting circle are negative.

So, the coordinates for the Orion Nebula listed in a star atlas
will look like this:

R.A. 5h 35.4m Dec. – 5° 27'

That’s 5 hours and 35.4 minutes in right ascension, and –5
degrees and 27 arc-minutes in declination (there are 60 arc-
minutes in 1 degree of declination).

Before you can use the setting circles to locate objects, the
mount must be accurately polar aligned, and the setting cir-
cles must be calibrated.

Calibrating the Declination Setting Circle

1. Loosen the Dec. lock lever and position the telescope as

accurately as possible in declination so it is parallel to the
R.A. axis as shown in Figure 7. Re-tighten the lock lever.

2. Loosen one of the thumbscrews on the Dec. setting circle,

this will allow the setting circle to rotate freely. Rotate the
Dec. setting circle until the pointer reads exactly 90°. Re-
tighten the setting circle thumbscrew.

10

Figure 12. 

The R.A. and Dec. setting circles.

Dec. setting circle

Dec. setting circle
thumbscrew (2)

Dec. indicator arrow

R.A. setting circle

R.A. indicator arrow

R.A. setting circle

thumbscrew

(2)

Summary of Contents for Atlas 10 EQ 9874

Page 1: ...onal Consumer Optical Products Since 1975 Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831 763 7000 P O Box 1815 Santa Cruz CA 95061 INSTRUCTION MANUAL Orion Atlas 10 EQ 9874 Equatorial Reflector Telescope ...

Page 2: ...shaft lock lever Counterweight shaft Counterweights Counterweight lock knobs Toe Saver Tripod leg Leg lock lever Finder scope Finder scope bracket Eyepiece Focus knob Tube rings Right ascension setting circle Right ascension lock lever Mirror cell Latitude scale Latitude adjustment L bolts Center support shaft not shown Hand controller Tripod support tray ...

Page 3: ... 1 9x50 Finder scope 1 Finder scope bracket with O ring 1 Collimation cap 1 Camera adapter 1 Dust cover 3 Assembly 1 Stand the tripod legs upright and spread the legs out as far as they will go Make certain that the leg lock levers are tightened Assembly should take no more than 30 min utes Refer to Figure 1 during assembly Assembling the telescope requires no tools other than the ones provided 2 ...

Page 4: ...plate with the tube rings attached in the dove tail slot on top of the equatorial mount Position the mount ing plate so that it is centered on the dovetail slot Re tight en the mounting plate securing knobs until the mounting plate is secure 8 Open the tube rings and lay the telescope optical tube in the rings at about the midpoint of the tube s length Rotate the tube so that the focuser is at a c...

Page 5: ...e to rotate freely about the right ascension axis Rotate it until the counter weight shaft is parallel to the ground i e horizontal 2 Now loosen the counterweight lock knobs and slide the weights along the shaft until they exactly counterbalance the telescope Figure 5a That s the point at which the shaft remains horizontal even when you let go with both hands Figure 5b 3 Retighten the counterweigh...

Page 6: ...ner moves in and out to keep the finder scope secure in the bracket The finder scope must be aligned accurately with the tele scope for proper use To align it first aim the main telescope in the general direction of an object at least a 1 4 mile away the top of a telephone pole a chimney etc Loosen the R A and Dec lock levers and move the telescope until it is point ing toward the desired object T...

Page 7: ...e the eyepiece with the new one by sliding it gently into the holder Re tighten the thumbscrew and refocus for your new magnification Using 2 eyepieces The Atlas 10 EQ s focuser is capable of accepting optional 2 eyepieces To use 2 eyepieces you must remove the 1 25 adapter from the focuser by loosening the two thumbscrews that hold it in place Figure 4 Once this adapter is removed insert a 2 eyep...

Page 8: ...ved only about its R A and Dec axes Using the Polar Axis Finder Scope The Atlas EQ mount comes with a polar axis finder scope Figure 9 housed inside the right ascension axis of the mount When properly aligned and used it makes accurate polar alignment quick and easy to do Alignment of the Polar Axis Finder Scope 1 Loosen the Dec lock lever and rotate the optical tube on the declination axis so tha...

Page 9: ...ion the star Polaris inside the tiny circle marked Polaris on the finder s reticle You must first loosen the knob underneath the equatorial mount on the center sup port shaft to use the azimuth adjustment knobs Once Polaris is properly positioned within the reticle you are precisely polar aligned If you do not have a clear view of Polaris from your observing site you will not be able to use the po...

Page 10: ...uttons on the hand controller will be reversed The reversal switches allow you to orient the push buttons to the direction of the apparent movement of a guide star in a guide scope for astrophotography Understanding the Setting Circles The setting circles on an equatorial mount Figure 12 enable you to locate celestial objects by their celestial coordinates Every object resides in a specific locati...

Page 11: ...scope overhead or in other directions In Figure 1 the telescope is pointed north as it would be during polar alignment The counterweight shaft is oriented down ward But it will not look like that when the telescope is point ed in other directions Let s say you want to view an object that is directly overhead at the zenith How do you do it DO NOT make any adjustment to the latitude adjustment L bol...

Page 12: ...n of the hole in the collimation cap is centered in the ring The center mark is also required for best results when using other collimating devices such as Orion s LaserMate Laser Collimator obviating the need to remove the primary mirror and mark it yourself Note The center ring sticker need not ever be removed from the primary mirror Because it lies directly in the shadow of the secondary mirror...

Page 13: ... cal tube bottom of the primary mirror cell these are the larg er thumbscrews The other three smaller thumbscrews lock the mirror s position in place these thumbscrews must be loosened before any collimation adjustments can be made to the primary mirror To start turn the smaller thumbscrews that lock the primary mirror in place a few turns each Figure 17 Use a screwdriv er in the slots if necessar...

Page 14: ...icantly distorting the incoming light and views at high magnifications will not appear sharp If the stars appear steady and do not twinkle seeing conditions are probably good and higher magnifica tions will be possible Also seeing conditions are typically poor during the day This is because the heat from the Sun warms the air and causes turbulence Good transparency is especially important for obse...

Page 15: ...sky objects however typically look better at medium or low magnifications This is because many of them are quite faint yet have some extent apparent width Deep sky objects will often disappear at higher magnifications since greater magnification inherently yields dimmer images This is not the case for all deep sky objects however Many galax ies are quite small yet are somewhat bright so higher pow...

Page 16: ...r enjoy the different colors of the stars and locate many pretty double and multiple stars The famous Double Double in the constellation Lyra and the gorgeous two color double star Albireo in Cygnus are favorites Defocusing a star slightly can help bring out its color E Deep Sky Objects Under dark skies you can observe a wealth of fascinating deep sky objects including gaseous nebulas open and glo...

Page 17: ...e focuser drawtube Figure 22a Then screw the camera adapter into the focuser drawtube Figure 22b Now attach the T Ring to your camera and thread it onto the camera adapter Figure 22c Use the camera s viewfinder to frame the picture Use the telescope s focuser to focus the image You may want to con sider using a remote shutter release instead of the shutter release on the camera touching the camera...

Page 18: ...quire expo sures on the order of 10 minutes To hold the camera s shut ter open this long you will need a lock shutter release cable Set the camera s shutter to the B bulb setting Depress the locking shutter release cable and lock it You are now expos ing your first deep sky object While exposing through the camera lens you will need to monitor the accuracy of the mount s tracking by looking throug...

Page 19: ...inized face up in the water and let it soak for a few minutes or hours if it s a very dirty mirror Wipe the mirror under water with clean cotton balls using extremely light pressure and stroking in straight line across the mirror Use one ball for each wipe across the mirror Then rinse the mirror under a stream of lukewarm water Any particles on the surface can be swabbed gently with a series of co...

Page 20: ...tsonville CA 95076 If the product is not registered proof of purchase such as a copy of the original invoice is required This warranty does not apply if in Orion s judgment the instrument has been abused mishandled or modified nor does it apply to normal wear and tear This warranty gives you specific legal rights and you may also have other rights which vary from state to state For further warrant...

Reviews: