Table 2: Numerical values used in this study. H, $\psi _1$ and $\omega _1$ are integration constants.
Initial values at J2000.0

H $H_{\mbox{\scriptsize MHB}}=3.27379492 \times 10^{-3}$

$\psi _1$ $5038\hbox{$.\!\!^{\prime\prime}$ }481507$ /cy

$\omega _1$ $-0\hbox{$.\!\!^{\prime\prime}$ }02575$ /cy

p₁ $5028\hbox{$.\!\!^{\prime\prime}$ }796195$ /cy

$\chi_1$ $10\hbox{$.\!\!^{\prime\prime}$ }556403$ /cy

$\epsilon _0$ $84~381\hbox{$.\!\!^{\prime\prime}$ }406 = 23^{\circ} 26' 21\hbox{$.\!\!^{\prime\prime}$ }406$

Contributions to the precession rate in longitude (in ''/cy)

Lunisolar first order $~~5494.062986 \times \cos \epsilon_0 \simeq 5040.7047$

Planetary first order 0.031

Geodesic precession -1.919882

**Table 2:** Numerical values used in this study. H, $\psi _1$ and $\omega _1$ are integration constants.
Initial values at J2000.0
H	$H_{\mbox{\scriptsize MHB}}=3.27379492 \times 10^{-3}$
$\psi _1$	$5038\hbox{$.\!\!^{\prime\prime}$ }481507$ /cy
$\omega _1$	$-0\hbox{$.\!\!^{\prime\prime}$ }02575$ /cy
p₁	$5028\hbox{$.\!\!^{\prime\prime}$ }796195$ /cy
$\chi_1$	$10\hbox{$.\!\!^{\prime\prime}$ }556403$ /cy
$\epsilon _0$	$84~381\hbox{$.\!\!^{\prime\prime}$ }406 = 23^{\circ} 26' 21\hbox{$.\!\!^{\prime\prime}$ }406$

Contributions to the precession rate in longitude (in ''/cy)
Lunisolar first order	$~~5494.062986 \times \cos \epsilon_0 \simeq 5040.7047$
Planetary first order	0.031
Geodesic precession	-1.919882

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