use crateD2PI;
use Rem;
/// Fundamental argument, IERS Conventions (2003):
/// mean longitude of Jupiter.
///
/// Status: canonical model.
///
/// Given:
/// t f64 TDB, Julian centuries since J2000.0 (Note 1)
///
/// Returned (function value):
/// f64 mean longitude of Jupiter, radians (Note 2)
///
/// Notes:
///
/// 1) Though t is strictly TDB, it is usually more convenient to use
/// TT, which makes no significant difference.
///
/// 2) The expression used is as adopted in IERS Conventions (2003) and
/// comes from Souchay et al. (1999) after Simon et al. (1994).
///
/// References:
///
/// McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
/// IERS Technical Note No. 32, BKG (2004)
///
/// Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
/// Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
///
/// Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
/// Astron.Astrophys.Supp.Ser. 135, 111