Table 2: Gravitomagnetic and classical nodal precession coefficients, in '' cy^-1. The coefficients $\dot\Omega_{.\ell}$ are $\partial\dot\Omega^{J_{\ell}}_{\rm class}/\partial J_{\ell}$ and refer to the classical precessions induced by the oblateness of the central mass. The numerical values of Table 1 have been used in Eqs. (1) and (5) (see below). $\dot\Omega_{\rm class}$ are the nominal centennial rates released at http://ssd.jpl.nasa.gov/elem_planets.html. They mainly include the N-body secular precessions.
Precessions Mercury Venus Earth Mars

$\dot\Omega_{\rm LT}$ $1.008\times 10^{-3}$ $1.44\times 10^{-4}$ $5.4\times 10^{-5}$ $1.5\times 10^{-5}$

$\dot\Omega_{.2}$ $-1.26878626476\times 10^5$ $-1.3068273031\times 10^{4}$ $-4.210107706\times 10^3$ $-9.80609460\times 10^2$

$\dot\Omega_{.4}$ $5.2774935\times 10^1$ 1.349709 $2.28040\times 10^{-1}$ $2.3554\times 10^{-2}$

$\dot\Omega_{\rm class}$ $-4.4630\times 10^2$ $-9.9689\times 10^2$ $-1.822825\times 10^4$ $-1.02019\times 10^3$

**Table 2:** Gravitomagnetic and classical nodal precession coefficients, in '' cy^-1. The coefficients $\dot\Omega_{.\ell}$ are $\partial\dot\Omega^{J_{\ell}}_{\rm class}/\partial J_{\ell}$ and refer to the classical precessions induced by the oblateness of the central mass. The numerical values of Table 1 have been used in Eqs. (1) and (5) (see below). $\dot\Omega_{\rm class}$ are the nominal centennial rates released at http://ssd.jpl.nasa.gov/elem_planets.html. They mainly include the N-body secular precessions.
Precessions	Mercury	Venus	Earth	Mars
$\dot\Omega_{\rm LT}$	$1.008\times 10^{-3}$	$1.44\times 10^{-4}$	$5.4\times 10^{-5}$	$1.5\times 10^{-5}$
$\dot\Omega_{.2}$	$-1.26878626476\times 10^5$	$-1.3068273031\times 10^{4}$	$-4.210107706\times 10^3$	$-9.80609460\times 10^2$
$\dot\Omega_{.4}$	$5.2774935\times 10^1$	1.349709	$2.28040\times 10^{-1}$	$2.3554\times 10^{-2}$
$\dot\Omega_{\rm class}$	$-4.4630\times 10^2$	$-9.9689\times 10^2$	$-1.822825\times 10^4$	$-1.02019\times 10^3$

Source LaTeX | All tables | In the text

	1 Introduction
	2 The gravitomagnetic field of the Sun
	3 The linear combination approach
	4 Conclusions
	References