Accurate free and forced rotational motions of rigid Venus

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Table 8:

Oppolzer terms in obliquity depending on triaxiality.
		Oppolzer	A.M
Argument	Period	$\cos(\omega t)$	CS $\cos(\omega t)$
	d	arcsec	arcsec
		10^-7	10^-7
$2\Phi$	-121.51	555 905	-275 453
$2l_{\rm S}-2\Phi$	58.37	-173 668	132 365
$M+2\Phi$	-264.6	-68 544	-6093
$M-2\Phi+2L_{\rm S}$	46.34	3074	2491
$2l_{\rm S}+2\Phi$	1490.35	-250	1786
$M-2\Phi$	78.86	2686	1816
$-M-2\Phi+2L_{\rm S}$	78.86	896	-606
$2M+2\Phi$	1490.35	-49	348
$2M-2\Phi+2L_{\rm S}$	38.41	-40	35
$2M-2\Phi$	58.37	18	14
$M +2\Phi+2L_{\rm S}$	195.26	-3	6
$-M+2\Phi+2L_{\rm S}$	-264.6	12	1
$2M+2\Phi+2L_{\rm S}$	104.47	0	0

Notes. Comparison with the corresponding nutation coefficients of the AMA in the tables of Cottereau & Souchay (2009).

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