era.obl06.md

eraObl06

rv = ERFA.obl06(date1, date2)

Mean obliquity of the ecliptic, IAU 2006 precession model.

Given:

   date1,date2  double   TT as a 2-part Julian Date (Note 1)

Returned (function value):

                double   obliquity of the ecliptic (radians, Note 2)

Notes:

1. The TT date date1+date2 is a Julian Date, apportioned in any convenient way between the two arguments. For example, JD(TT)=2450123.7 could be expressed in any of these ways, among others:

          date1          date2

       2450123.7           0.0       (JD method)
       2451545.0       -1421.3       (J2000 method)
       2400000.5       50123.2       (MJD method)
       2450123.5           0.2       (date & time method)

The JD method is the most natural and convenient to use in cases where the loss of several decimal digits of resolution is acceptable. The J2000 method is best matched to the way the argument is handled internally and will deliver the optimum resolution. The MJD method and the date & time methods are both good compromises between resolution and convenience.

2. The result is the angle between the ecliptic and mean equator of date date1+date2.

Reference:

Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351

This revision: 2021 May 11

Copyright (C) 2013-2021, NumFOCUS Foundation. Derived, with permission, from the SOFA library.