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\centerline{\tit Table 6.2}
 
\vskip 5mm 
    
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 & & & & & & &  & & & New & calc. & KS & calc. &\cr
$\lambda_{Ve}$&$\lambda_{Ea}$ &$\lambda_{Ma}$ & $\lambda_{Ju}$ &
$\lambda_{Sa}$&D &F &l &$\Omega$ & P(yr.) & Sin & Cos & Sin & Cos \cr
 & & & & & & &  & & & (0.01&mas) & (0.01&mas) &\cr
 & & & & & & &  & & & & & & &\cr
0 &2 &0 &-2 &0 &2 &0 &-2 &1 &274.21 &0.0 &-1.5 &0.0 &-1.6 &\cr
8 &-12 &0 &0 &0 &1 &-1 &0 &-1 &241.06 &-3.2 &-6.4 &-3.1 &-6.3 &* \cr
0 &1 &-2 &0 &0 &0 &0 &0 &-1 &103.72 &2.3 &2.5 &2.3 &2.4 & \cr
0 &2 &0 &-3 &0 &2 &0 &-2 &-1 &37.32 &0.0 &-0.5 &0.0 &-0.5 & \cr
0 &1 &0 &0 &1 &1 &-1 &0 &-1 &29.49 &-0.4 &-0.9 &0.0 &-0.9 & \cr
0 &4 &-8 &3 &0 &0 &0 &0 &-1 &18.81 &-1.6 &-0.4 &-1.6 &-0.4 & \cr
0 &4 &-8 &3 &0 &0 &0 &0 &1 &18.42 &1.6 &0.4 &1.6 &0.4 & \cr
0 &0 &2 &0 &0 &1 &-1 &0 &-1 &15.79 &-0.4 &-1.5 &0.0 &-1.5 & *\cr
0 &1 &0 &0 &-2 &1 &-1 &0 &-1 &14.72 &0.6 &0.3 &0.6 &0.0 & *\cr
5 &-6 &0 &0 &0 &2 &-2 &0 &-1 &13.55 &2.3 &0.0 &2.3 &0.0 & \cr
0 &1 &0 &1 &0 &1 &-1 &0 &-1 &11.87 &-1.0 &0.3 &-1.0 &0.0 & *\cr
5 &-7 &0 &0 &0 &1 &-1 &0 &-1 &7.84 &-0.1 &-0.7 &0.0 &-0.7 \cr
0 &1 &0 &-2 &0 &1 &-1 &0 &-1 &5.93 &0.8 &0.1 &0.8 &0.0 & \cr
3 &-3 &0 &0 &0 &2 &-2 &0 &-1 &5.64 &0.0 &-0.6 &0.0 &-0.6 & \cr
18 &-16 &0 &0 &0 &0 &-2 &-1 &-2 &0.04 &0.3 &-0.5 &-0.6 &-1.3 &*** \cr
18 &-16 &0 &0 &0 &0 &2 &-1 &2 &0.04 &-0.3 &0.5 &-0.5 &1.1 &** \cr
 & & & & & & &  & & & & & & &\cr
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\vskip 50mm

Table 6. Coefficients of rigid Earth nutation coming from the
indirect planetary contribution, lunar part, up to 0.005 mas, in
longitude (6.1) and obliquity (6.2). Comparison with the respective
value 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.

\bye
\end