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Polar Alignment of LX200R and Ultra Wedge

For The Southern Hemisphere by Chris James



This document goes thru the process required to Polar Align the LX200R using a Ultra Wedge in the Southern Hemisphere. It differs from that described in the manual for the Northern Hemisphere in that it takes measures to more accurately place the scope in the Polar Position as the star used by auto star for alignment Sigma Octanis cannot be seen with the naked eye under most circumstances, which is not the case for Polaris used in the northern hemisphere. As a result it uses methods to place the scope in the Polar position that are normally used during the day. This places the alignment star in the view scope at the end of this procedure to allow the normal process to be used to complete the polar alignment procedure.


You will need a Compass, Spirit Level and a Protractor to complete this process.


Setup Tripod


a) Orientate the tripod using a compass so that tangent arm on the tripod is pointing north. Dont forget to compensate for magnetic north in the area.


b) Using a spirit level, adjust the length of the three legs of the tripod to achieve level in all directions on the head of the tripod.





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Level Tripod Head

Orientate Tripod Using A Compass



Mount Ultra Wedge


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Mount the wedge on the tripod using the Manual Knob/Compass and the three Button Head bolts. Make the button head bolts firm but not tight to allow the wedge to rotate on the head of the tripod to perform adjustments.


Confirm the wedge is still aligned in the North/South direction with the compass mounted in the Manual Knob. You can correct any alignment with the Azimuth Control Knob on the wedge or by moving the tripod legs, depending on amount of the error you need to compensate for. Note: the wedge will now be orientated in such a manner so that when the scope is place on it, the control box of the scope will be facing south.


Using the bubble level in Ultra Wedge, confirm the wedge is still level in all directions. Adjust tripod legs if required to achieve level. If you have not already done so, confirm the bubble in the Ultra Wedge is reading true by using an alternative external spirit level before you solely depend on the inbuilt bubble level.


Adjust the Tilt Plate for your latitude. The latitude scale on the side of the wedge should be used as a guide only. Once you are close, use a protractor and the complementary angle for your latitude. Complementary Angle = 90 minus your Latitude. For latitude of 32 degrees, the complementary angle is, 90 minus 32 = 58 degrees. Placing the protractor on the tilt plate adjust the fine latitude control knob until the protractor reads the complementary angle of 58 degrees.







Setting Tilt Plate Complementary Angle





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Mount Scope


Before attempting to sit the scope base on the tilt panel, insert the single long bolt and washer into the scope base using the hole at the opposite end to the auto star interface panel. Use just enough thread to ensure it can hold the scope on its own but not too much to allow you to slip it through the mounting slot on the tilt plane. To make this easier, you can lay the bolt in the tilt panel slot and mark the depth of the tilt panel on the bolt using a pen, before inserting it into the scope base.


Release the RA clutch and turn the forks so that one arm of the fork is opposite the interface panel, then lock the RA clutch again.


You can now lift the scope onto the tilt plane sliding the one bolt on the telescope base through the mounting slot on the tilt plane of the wedge.


Align the telescope base so that all three remaining holes in the telescope base and the tilt plane align.


Now use the T-Bar to take some of the weight for safety reasons, dont tighten it too much yet until you have insert and started the thread on the remaining two bolts through the tilt plane to the scope base.


Now tighten all four bolts and ensure the scope base is flush with the tilt panel.


The proceeding section will assume that the view scope has been mounted and calibrated so mount all hardware including, focusing unit, diagonal prism, 9mm Illuminated Reticle eyepiece and view scope.


Release the RA clutch and place the place the fork arms in the middle of its RA movement. Checking its travel between the RA stops should show it has about two turns between stops, so lock the RA clutch about one turn from one of these stops.



Set Polar Home Position


At this stage auto star has been turned on and the following has been completed:


Smart drive init has completed.

GPS fix has completed.

Polar mount has been selected in the telescope setup menu.

You have selected Align scope and chosen the Easy Polar Alignment option.


Auto Star is now prompting you to place the scope in the Polar Home Position.

Adjusting the RA Zero Position

As you have centered the RA movement before hand, use the Auto Star controller to rotate the fork arms to the 00 position so that the center tick on the arms and base align.



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Setting RA To Zero





Place the sprit level across the fork arms and fine tune the RA position so that the spirit level reads true, you can reduce the RA speed to make this adjustment real easy when using the sprit level.


Alternatively you can point the telescope vertically up and place the spirit level across the telescope cover and fine tune the RA position so that the spirit level reads true.


Adjusting the DEC 90 degree Position

Release the Dec clutch and rotate the OTA so the DEC dial reads 90 degrees. Now place the protractor on the OTA and fine tune the Dec position with the Auto Star controls using a slow speed, so that the protractor reads your latitude in degrees, 32 degrees for example.



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Adjust Dec To Your Latitude




Now quickly recheck the following:


1) Is the Bubble on the Wedge still true?

2) Is the RA indicator roughly on the tick marks at the base and fork arms and the spirit level across the fork arms showing level?

3) Is the Dec indicator showing approx 90 Degrees and the protractor indicating your latitude when placed along the OAT?

4) Is the scope pointing at the point in the sky where you imagine the South Celestial Pole to be?









Polar Position Facing SCP




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Press ENTER to AutoStar


If you where able to answer yes to all of the above, then we are now ready to proceed by pressing ENTER to allow AutoStar to continue now that you have placed the scope in the Polar Home Position.


If its not dark enough yet to see Sigma Octanis in your view scope, you may consider using this time while you wait, to Train your drives (RA & DEC) on a distant terrestrial object and then come back to this point. Training the drives is not covered in this document.



AutoStar now slews to the Star Sigma Octanis


AutoStar now slews to Sigma Octanis, dont be surprised if what seems a small movement in the sky may result in a relatively long slew in RA for the scope to arrive at Sigma Octanis. The length of the RA slew will depend on the Local Sidereal Time and date you are doing this alignment. In other words Sigma Octanis is quite close to the South Celestial Pole but the scope may take a while to slew to it depending on the date and time.


A word of caution, this possible long RA slew may leave the scope in such a position that you cannot reach the viewfinder / eyepiece in some orientations. More importantly, if you are not expecting this movement, depending on your setup, you may damage some expensive accessories that you may have attached to the scope, such as SLR cameras, as it attempts to slew through positions these attachments cant go. Dont get a nasty surprise in the dark, know your setup limitations, if any in advance!


Sigma Octanis, is quite dim and under most conditions you will need binoculars or the view scope to see it. I have exaggerated its size in the chart below. Check Sigma Octanis location on your sky map to ensure you are happy where it should appear in the sky. RA = 21h 15.515m DEC = 88 deg 55.663m


To find it in the sky, start at the Southern Cross, trace out four times the length of the cross heading towards the SCP. Using the binoculars look in that area and pan around to find three faint stars that form an isosceles triangle that fit within the field of view of the binoculars. Now the two stars that form the side of the triangle that are 90 degrees to the line that you have just drawn from the Southern Cross are Chi Octantis and Sigma Octantis, the third star of the triangle is Tau Octantis.


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Once AutoStar has completed its slew to the Star Sigma Octanis,


With the assistance of the view scope, centre Sigma Octanis in the 9mm Illuminated Reticle eyepiece using the Wedges Azimuth and Latitude controls, do not use the arrow keys on AutoStar. The view scope will display all three stars (Chi, Sigma & Tau Octanis) whilst the field of view of the eyepiece will only display the one. If you have taken care with the setup to this point, Sigma Octanis should be in your eyepiece. If its not, try moving the Azimuth control on the wedge first to find it as its more likely you have made an error aligning North/South with your compass then the Latitude on the tilt plate with the protractor


When you have Sigma Octanis in the center of the eye piece press ENTER on AutoStar.


AutoStar will now select a star from its database and slew to it. Once it has completed slewing, use the arrow keys on AutoStar to center the selected star in the eyepiece then press ENTER.


AutoStar will now select a second star from its database and slew to it. Once it has completed slewing, use the arrow keys on AutoStar to center the selected star in the eyepiece then press ENTER.


This should complete the rough Polar alignment of the wedge and the alignment of AutoStar to to-nights sky.



Drift Polar Alignment ( Precise Polar Alignment )


If you have done the proceeding Polar Alignment correctly, this section should only be a fine tune of the polar alignment required for astrophotography.


If you where unable to complete the proceeding Polar Alignment because for example Sigma Octanis was not visible, then the Polar Alignment can still be completed using the drift method. It just means your starting point may be more off alignment and this step may take a little longer then would otherwise be the case.


Fine Adjustment of Wedges Azimuth


Place the 9mm Illuminated Reticle Eyepiece into the eyepiece holder of the telescope. With the telescope now tracking, slew the telescope to a bright star near the meridian close to zenith. Youll find that nearing straight up brings the Dec close to your latitude in degrees.


Using the arrow keys on the remote key pad of autostar, move the scope back and forth in RA. Adjust the cross line pattern to align the star movement to the RA plane.

Ignoring any RA drift, compensate for any North/South drift by adjusting the wedges Azimuth Control Knob. Keep doing this until no noticeable drift occurring over 15 minutes.

In Short:

1.    If the start drifts south in the eyepiece adjust the Azimuth knob to move the start east in the eyepiece then re-centre it by using the autostar controls.


2.    If the star drifts north, adjust the Azimuth knob on the polar mount to move the start west in the eyepiece then re-centre it by using the auto star controls.











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Fine Adjustment of Wedges Latitude


Slew the telescope to a bright star near the Eastern or Western Horizon but still near the celestial equator.

Ignoring any RA drift, compensate for North/South drift by adjusting the wedges Latitude Control Knob. Keep doing this until no noticeable drift occurs over 15 minutes.

In Short:

      1. Use the Tilt Knob on the Polar Mount to move the star in the eyepiece in the opposite direction to the North/South drift.









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Keep repeating the Azimuth and Latitude adjustments above until the changes in one have little effect on the other.


Once you are confident with this process, you may consider a short cut process that makes better use of the setup time for a astro imaging session.


The url of the short cut process can be found @


The url of the process using your imaging camera can be found @






Written by:

Chris James

55 Blackthorn Road

Greenwood WA 6024










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