You can determine the 3D position for a star, pp, by using the distance from Earth, RR, as well as the right ascension, OmegaOmega, and declination, deltadelta, within the following formula.
p=RbeginbmatrixcosOmegacosdelta sinOmegacosdelta sindelta endbmatrixp=RbeginbmatrixcosOmegacosdelta sinOmegacosdelta sindelta endbmatrix
Note this will yield positions within the Earth-centered inertial reference frame.
No comments:
Post a Comment