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\centerline{\tit Table 5.2}
 
\vskip 5mm 
    
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 & & & & & & & New & calc. & KS & calc. & \cr
$\lambda_{Ve}$&$\lambda_{Ea}$ &$\lambda_{Ma}$ & $\lambda_{Ju}$ &
$\lambda_{Sa}$&$p_{A}$ & P(yr.) & Sin & Cos & Sin & Cos & \cr
 & & & & & & & (0.01&mas) & (0.01&mas) & \cr
 & & & & & & & & & & & \cr
0 &0 &0 &0 &2 &1 &14.72 &0.6 &-0.3 &0.0 &0.0 &**\cr
3 &-5 &0 &0 &0 &-1 &8.10 &-2.0 &0.5 &0.0 &0.0 &***\cr
0 &0&0 &2 &0 &1 &5.93 &1.2 &-0.2 &0.0 &0.0 &***\cr
0 &0&0 &2 &0 &2 &5.93 &0.0 &0.5 &0.0 &0.0 &**\cr
2 &-4 &0 &0 &0 &-2 &1.34 &0.0 &0.5 &0.0 &0.5 &\cr
0 &1 &0 &1 &0 &2 &0.92 &0.0 &1.1 &0.0 &1.1 &\cr
1 &-3 &0 &0 &0 &-2 &0.73 &0.0 &-1.2 &0.0 &-1.2 &\cr
2 &-5 &0 &0 &0 &-2 &0.57 &0.6 &0.0 &0.6 &0.0 &\cr
0 &2 &0 &-1 &0 &2 &0.52 &-0.1 &0.7 &0.0 &0.7 &*\cr
0 &2 &-8 &3 &0 &-2 &0.50 &1.8 &0.5 &1.8 &0.5 &\cr
0 &6 &-8 &3 &0 &2 &0.50 &-1.8 &-0.5 &-1.8 &-0.5 &\cr
0 &2 &0 &1 &0 &2 &0.48 &0.0 &-0.7 &0.0 &-0.7 &\cr
2 &-1 &0 &0 &0 &2 &0.44 &-0.8 &0.0 &-0.8 &0.0 &\cr
1 &1 &0 &0 &0 &2 &0.38 &0.0 &1.3 &0.0 &1.3 &\cr
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0 &3 &0 &-1 &0 &2 &0.34 &0.0 &-2.2 &0.0 &-2.2 &\cr
0 &4 &-2 &0 &0 &2 &0.34 &0.0 &-0.6 &0.0 &-0.6 &\cr
2 &0 &0 &0 &0 &2 &0.31 &0.0 &-1.7 &0.0 &-1.7 &\cr
0 &4 &0 &-2 &0 &2 &0.26 &0.0 &0.8 &0.0 &0.8 &\cr
& & & & & & & & & & &\cr
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Table 5. Coefficients of rigid Earth nutation coming from the 
indirect planetary contribution, solar part, up to 0.005 mas,
in longitude (5.1) and obliquity (5.2). Comparison with the
respective value in the tables of Kinoshita and Souchay(1990).
The symbol "*" indicates that the absolute difference is between
0.1 and 0.5 mas,"**" between 0.5 and 1.0 mas, and "***" bigger
than 1.0 mas.

\end