Specific effects of large asteroids on the orbits of terrestrial planets and the ASETEP database

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Table 5

Comparisons of the sinusoids found in this paper with those in Mouret et al. (2009) of the effects of Ceres, Pallas and Vesta on λ_Mars.

Our analysis		Mouret et al. (2009)
Period	Amplitude	Period	Amplitude	Argument
(y)	× 10^-3 ′′	(y)	× 10^-3 ′′	i λ_M	+	j λ_c
				i		j

Ceres
10.280	0.573	10.25	0.571	1		–2
44.330	1.768	45.77	1.914	2		–5
76.553	0.205
1.590	0.108	1.59	0.127	2		–4
2.429	0.108	2.43	0.109	2		–2
5.139	0.126	5.12	0.108	2		–3
8.342	0.058	8.37	0.060	1		–3
3.180	0.080	3.18	0.039	3		–4
13.378	0.069	13.20	0.025	3		–6

Pallas
49.058	2.521	48.65	2.537	2		–5
59.790	0.333
24.517	0.209	24.32	0.227	4		–10
12.855	0.148	12.89	0.153	3		–7
17.424	0.088	17.54	0.099	5		–12

Vesta
51.657	4.372
25.854	0.679	25.93	0.668	2		–4
4.223	0.112	4.22	0.110	2		–3
40.162	0.107
17.237	0.104	17.29	0.103	3		–6
1.118	0.096
15.779	0.083
1.952	0.078	1.95	0.078	2		–2
32.816	0.078
2.029	0.036	2.03	0.035	3		–4
1.301	0.032	1.30	0.031	3		–3

Notes. Coefficients are ranged in decreasing order of amplitude.

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