Euler rotations in galactic plane to change to equatorial

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SUMMARY

The discussion focuses on converting coordinates from the galactic coordinate system to the equatorial coordinate system using Euler rotations. The user seeks to establish rotation angles, specifically alpha and beta, where alpha ranges from -π to π and beta from -π/2 to π/2. The galactic north pole is defined by coordinates (L=any value, B=90), highlighting the singularity at the poles. Online conversion tools are recommended for users seeking quick answers.

PREREQUISITES
  • Understanding of Euler rotations in three-dimensional space
  • Familiarity with the galactic coordinate system
  • Knowledge of equatorial coordinate system concepts
  • Basic trigonometry for angle calculations
NEXT STEPS
  • Research the mathematical principles behind Euler rotations
  • Explore online tools for converting between galactic and equatorial coordinates
  • Study the implications of singularities in spherical coordinate systems
  • Learn about the relationship between latitude and longitude at the poles
USEFUL FOR

Astronomers, astrophysicists, and anyone involved in celestial navigation or coordinate transformations will benefit from this discussion.

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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