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POLAR ALIGNMENT



Unless you are lucky enough to live in a dark location and have a permanent observatory, you will have to accurately polar align your telescope each and every time you go out.

Why?

An accurate polar alignment is required to eliminate "field rotation".  A perfectly guided astrophoto will still show error if the mount is not very accurately polar aligned.  Field rotation shows up in an image as curved stars at the outer edges of the image.  This is not to be mistaken for coma, usually seen in fast camera lenses, in which the stars are bloated little UFO-like things.  A well-aligned mount will not show field rotation.

How?

The following procedure for the drift method of polar alignment assumes the use of a Schmidt-Cassegrain (SCT) or refractor telescope.  If you are using a Newtonian for photography you will simply need to reverse the adjustment steps.  These steps are highlighted for you.

Once you have read through the following detailed procedure you may wish to print out the Quick Guide to Drift Alignment to have with you in the field.


Note:  The drift method of polar alignment requires the use of an illuminated crosshair eyepiece.  A simple double-crosshair (shown below) works perfectly, although a fancier eyepiece such a Celestron's Micro Guide eyepiece will work fine as well.

View through a double-crosshair illuminated reticle eyepiece

The telescope mount should already be roughly polar aligned, preferably using a polar alignment scope.

Reverse the following adjustments if you are using a Newtonian telescope

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