ephem.git - Astronomical ephemerides (unfinished)

	Commit message (Collapse)	Author	Age	Files	Lines
*	Use J2000 ecliptic (rather than equatorial) coordinates as starting point ↵	David A. Madore	2012-04-17	1	-2/+4
\| \| \| \| \| \|	for precession. We will assume that these are the coordinates returned by VSOP87.
*	Use quaternions instead of 3*3 matrices to represent rotations.	David A. Madore	2012-04-03	1	-5/+5
\|
*	Equation of the origins/equinoxes.	David A. Madore	2012-03-27	1	-0/+2
\|
*	Nutation.	David A. Madore	2012-03-27	1	-3/+5
\|
*	Simple matrix library + formula for precession.	David A. Madore	2012-03-27	1	-0/+22