Unit vector to Right Ascension/Declination

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Discussion Overview

The discussion revolves around the conversion of a unit vector to right ascension and declination, which are spherical coordinates used in astronomy. Participants explore the relevant formulas and seek clarification on the concepts involved.

Discussion Character

  • Exploratory, Technical explanation, Conceptual clarification

Main Points Raised

  • One participant expresses uncertainty about the conversion process and mentions having a unit vector with a radius of 1.
  • Another participant requests resources to better understand right ascension and declination.
  • A participant explains that right ascension and declination correspond to spherical coordinates, with declination analogous to latitude and right ascension to longitude.
  • Further resources are shared, including a link to a document discussing common transformations in positional astronomy and the concept of the metric tensor related to coordinate transformations.
  • One participant acknowledges a mistake regarding the formulas used for the conversion.

Areas of Agreement / Disagreement

The discussion contains multiple viewpoints and resources shared, but there is no consensus on the correct formulas or methods for the conversion process.

Contextual Notes

Participants have not fully resolved the mathematical steps involved in the conversion, and there may be missing assumptions regarding the definitions of the coordinate systems.

Scott S
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OK, I'm really rusty on this.

I need to convert a unit vector to right ascension and declination.
I believe I recall the formulae correctly, as I seem to have gotten 1 as my radius.
So, that's good.

In the pic I have my unit vector (P2), my actual answer below, my expected answer in red and the formulae I (believe) I need in blue shaded cells.

Any help greatly appreciated.
 

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  • UNIT VECTOR.jpg
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Hey Scott S.

Can you point out a wiki or some other resource that outlines the concept you are talking about for ascension and declination?
 
A quick google search gave me this which discusses a lot of common transformations.

http://www2.astro.psu.edu/users/rbc/a501/positional_astronomy.pdf

If you wanted to derive the results yourself you should derive the metric tensor that goes between two systems and check if the tensor you derive gives the same results.

The metric tensor is related to the Jacobian transformation between the two systems and you can learn it by reading about tensor mathematics or differential geometry.
 
Last edited by a moderator:
Got it, thanks.

Wrong formulae.
 

Attachments

  • UNIT VECTOR 2.jpg
    UNIT VECTOR 2.jpg
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