Euler rotations in galactic plane to change to equatorial

AI Thread Summary
To rotate an axis from the galactic north pole to the equatorial north pole using Euler rotations, one must determine the appropriate rotation angles alpha and beta, where alpha ranges from -pi to pi and beta from -pi/2 to pi/2. The galactic north pole is represented by coordinates l=0, b=90, indicating a singularity at the pole where longitude is irrelevant. This singularity is analogous to Earth's coordinate system, where latitude of 90 degrees means longitude is inconsequential. The discussion highlights the confusion surrounding the conversion and the nature of coordinate systems at the poles. Understanding these concepts is crucial for accurately performing the rotation.
birdhen
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HI there,

I am having problems understanding something.
If I have an axis pointing towards the galactic north pole, and I rotate it using an Euler rotations how can I can I establish the rotation angles needed so that it will be pointing to the equatorial North pole.
I am looking for values alpha and beta where alpha can run from -pi-->pi and beta can run from -pi/2-->pi/2.

Many thanks
 
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Thank you for your reply. I am getting confused still. Would the galactic north pole just have l=0 b=90 in galactic coordinates? I am imagining the surface of a sphere, if b=90 is the top point of the sphere, then there can be no l value as the horizontal plane through the sphere would just be a point.
 
These types of coordinates systems have a singularity at the poles, so the north galactic pole has coordinates (L=anything, B=90). The same is true on the Earth. If the latitude is 90 degrees, it doesn't matter what the longitude is, you are at the pole.
 
OK , of course, thanks !
 
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