Polar Alignment Using Imaging Camera

By Chris James

 


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Purpose

The purpose of this document is to describe a polar alignment method using your imaging camera that is already set up on your telescope ready for a imaging session.  This is an alternative to using the traditional reticle eye piece or one of the many software packages designed for this purpose.  The advantage of using this simple method is does not rely on any software yet at the same time provides a visual pleasing method that is both simple and quick.

 

Assumptions

1. The mount/wedge has been leveled with spirit level in all directions.

If the mount is NOT perfectly level, a polar alignment cannot be performed.

 

2. A basic Polar Alignment has been done.

Using a compass the mount has been aligned in the North/South direction allowing for magnetic deviation in the area.  The mount or wedge has had the latitude adjustment set for the latitude in use, preferably using a protractor.

 

3. The mounts tracking rate is set to twice the sidereal rate.

This allows the mount to be slewed at twice the sidereal rate when the left and right RA buttons are pressed.

 

4. All accessories have been fitted to the scope.

  All the normal accessories that will be fitted to your telescope for your imaging session have now been fitted.

 

 

Azimuth Adjustment

 

  1. Select a star that is close to the North/South meridian and position it in your camera's FOV so its on the RHS.  This can be any star close to the N/S meridian that you can see and the scope can slew too safely.

  2. Setup a timed exposure on your camera of two minutes and commence the exposure.

  3. Using the RA controls of your mounts hand controller, hold the RA button down to cause the start to move to the LHS for one minute.

  4. After the first minute has expired press the other RA button for a minute to return the star to the RHS of the cameras FOV.

  5. Save and view the two minute exposure. You should have a image that looks like the greater than or less than symbol "<", the angle of which will depend on the current Azimuth error of your mount.

  6. At this stage you have no idea which way you need to turn your mount/wedge azimuth control in order to correct the azimuth error.  Don't worry, pick a direction and turn it a nominated amount.  Just remember which direction and how much you turned it.

  7. Relocate the star on the RHS of the FOV of the camera and now repeat steps 2 to 5 above.

  8. Check the new image, if the angle produced in the image has now reduced you have turned the azimuth control in the correct direction and you now need to repeat steps 2 to 5 until you have a single straight line.  If the angle increased, you need to turn the azimuth control in the opposite direction.

Latitude Adjustment

 

  1. Select a star that is close to the either the eastern or western horizon and close to the east/west meridian and position it in your camera's FOV so its on the RHS.  This can be any star close to the E/W meridian but also close to either the east or west horizon that you can see and the scope can slew too safely.

  2. Setup a timed exposure on your camera of two minutes and commence the exposure.

  3. Using the RA controls of your mounts hand controller, hold the RA button down to cause the start to move to the LHS for one minute.

  4. After the first minute has expired press the other RA button for a minute to return the star to the RHS of the cameras FOV.

  5. Save and view the two minute exposure. You should have a image that looks like the greater than or less than symbol "<", the angle of which will depend on the current Latitude error of your mount.

  6. At this stage you have no idea which way you need to turn your mount/wedge latitude control in order to correct the latitude error.  Don't worry, pick a direction and turn it a nominated amount.  Just remember which direction and how much you turned it.

  7. Relocate the star on the RHS of the FOV of the camera and now repeat steps 2 to 5 above.

  8. Check the new image, if the angle produced in the image has now reduced you have turned the latitude control in the correct direction and you now need to repeat steps 2 to 5 until you have a single straight line.  If the angle increased, you need to turn the latitude control in the opposite direction.

 

Fine Adjustment

In our first pass of both the Azimuth and Latitude adjustments above we chose a period of two minutes to use as our timed exposure of both our images and the total period in which we move the mount in RA.  If your largest exposure times for your imaging session are not going exceed this time, in most cases they will, you will now need to redo both the Azimuth and Latitude adjustments above but this time increase the period for exposure and total RA movement to match your proposed exposure times.

 

For example if you plan on 5 minute exposures, then increase the camera exposure to 5 minutes and then you will have a 2.5 minute RA movement in each direction.

 

Refinements to Process

The above process can obviously be refined to suite your scope and individual setup.

 

For example my FOV of both my imaging camera on the LX200R and my guide camera on the ED80 are very similar.  As a result I synch their FOV so they are the same, resulting in the star being in the same place on both their images.  I then use the guide camera image, which is live, to monitor my movement when doing the timed RA movements above.  This makes it a lot easier !  It is also helps when re-positioning the star in the FOV of the camera to do the next exposure after each physical adjustment of the Azimuth or Latitude control of the mount.

 

Your environment will be different to mine so you will need to fine tune accordantly just to make things easier.

 

 

 

Related Documents

Polar Aligning The Mead LX200R - Full Document

Short Cuts For Polar Aligning Meade LX200R

 

 

                                 

 

 

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