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\noindent {\bf  Table 2.17.} Masses des principaux satellites. 
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{#\hfill&#\hfill&\hfill#&\hfill#&\hfill#\cr  
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\cc{$m$}&\cr
 Nom&\cc{N$^{\circ}$} &\multispan2\hfill\hbox to 52mm{\downbracefill}\hfill&$Gm\quad$\cr
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&&(masse solaire)&(masse plan\`ete)
&(m$^3$ s$^{-2}$)\cr
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{\medskip} 
\noalign{\hrule}
\noalign {\bigskip}
&&\multispan 2\hfill{\bf Terre}\hfill&\cr
\noalign{\medskip}
Lune&&3.694$\,$3024\x10$^{-8}$&1.230$\,$0034\x10$^{-2}$&4.902$\,$7989
\x10$^{12}$\cr 
\noalign{\bigskip\smallskip}
&&\multispan 2\hfill{\bf Mars}\hfill&\cr
\noalign{\medskip}
Phobos &&6.39\x10$^{-15}$&1.98\x10$^{-8}$&8.47\x10$^5$\cr
D\'eimos&&9.1\x10$^{-16}$& 2.8\x10$^{-9}$&1.20\x 10$^5$\cr
\noalign{\bigskip\smallskip}
&&\multispan 2\hfill{\bf Jupiter}\hfill&\cr
\noalign{\medskip}
M\'etis&XVI&4.8\x10$^{-14}$&5\x10$^{-11}$&6.3\x10$^6$\cr
Adrast\'eia&XV&9.5\x10$^{-15}$&1\x10$^{-11}$&1.3\x10$^6$\cr
Amalth\'ee&V&3.6\x10$^{-12}$&3.8\x10$^{-9}$&4.8\x10$^8$\cr
Th\'eb\'e&XIV&3.8\x10$^{-13}$&4\x10$^{-10}$&5.1\x10$^7$\cr
Io&I&4.49\x10$^{-8}$& 4.705\x10$^{-5}$&5.96\x10$^{12}$\cr 
Europe&II&2.41\x10$^{-8}$& 2.527\x10$^{-5}$&3.20\x10$^{12}$\cr 
Ganym\`ede&III&7.45\x10$^{-8}$& 7.804\x10$^{-5}$&9.89\x10$^{12}$\cr  
Callisto&IV&5.41\x10$^{-8}$&5.668\x10$^{-5}$&7.18\x10$^{12}$\cr
L\'eda&XIII&2.9\x10$^{-15}$&3\x10$^{-12}$&3.8\x10$^5$\cr
Himalia&VI&4.8\x10$^{-12}$& 5.0\x10$^{-9}$&6.3\x10$^8$\cr 
Lysith\'ea &X&3.8\x10$^{-14}$&  4\x10$^{-11}$&5.1\x10$^6$\cr
Elara&VII&3.8\x10$^{-13}$& 4\x10$^{-10}$&5.1\x10$^7$\cr
Anank\'e &XII&1.9\x10$^{-14}$&2\x10$^{-11}$&2.5\x10$^6$\cr
Carm\'e& XI&4.8\x10$^{-14}$&5\x10$^{-11}$&6.3\x10$^6$\cr            
Pasipha\'e&VIII&9.5\x10$^{-14}$&1\x10$^{-10}$&1.3\x10$^7$\cr
Sinop\'e&IX&3.8\x10$^{-14}$&4\x10$^{-11}$&5.1\x10$^6$\cr
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&&\multispan 2 \hfill{\bf Saturne}\hfill&\cr
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Anneau C&&4.9\x10$^{-13}$&1.7\x10$^{-9}$&6.4\x10$^7$\cr 
Anneau B&&1.2\x10$^{-11}$&4.2\x10$^{-8}$&1.6\x10$^9$\cr 
Anneau A&&3.1\x10$^{-12}$&1.1\x10$^{-8}$&4.2\x10$^8$\cr 
Mimas&I&2.29\x10$^{-11}$&8.00\x10$^{-8}$&3.04\x10$^9$\cr
Encelade&II&3.7\x10$^{-11}$&1.3\x10$^{-7}$&4.9\x10$^9$\cr
T\'ethys &III&3.4\x10$^{-10}$&1.2\x10$^{-6}$&4.5\x10$^{10}$\cr
Dion\'e&IV&5.29\x10$^{-10}$&1.85\x10$^{-6}$&7.0\x10$^{10}$\cr
Rh\'ea&V&1.16\x10$^{-9}$&4.06\x10$^{-6}$&1.54\x10$^{11}$\cr
Titan&VI&6.7652\x10$^{-8}$&2.3670\x10$^{-4}$&8.9782\x10$^{12}$\cr
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\noindent{ \bf Table 2.17.} (fin). 
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{#\hfill&\quad#\hfill&\hfill#&\hfill#&\quad\hfill#\cr 
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&&\multispan2 
\cc{$m$}\cr
 Nom&\cc{N$^{\circ}$} 
&\multispan2\hfill\hbox  to 52mm {\downbracefill}\hfill&$Gm\quad$\cr
\noalign{\smallskip}
&&(masse solaire)&(masse plan\`ete)
&(m$^3$ s$^{-2}$)\cr
\noalign{\bigskip} 
\noalign{\hrule}
\noalign{\bigskip}
&&\multispan 2\hfill{\bf Saturne}\hfill&\cr
\noalign{\medskip}
Hyp\'erion&VII&\phantom{3.694}8.6\x10$^{-12}$&\phantom{1.230$\,$003}3\x10$^{-8}$&
\phantom{4.902$\,$79}1.1\x10$^9$\cr 
Japet&VIII& 7.99\x10$^{-10}$&2.79\x10$^{-6}$&1.06\x10$^{11}$\cr
Ph\oe b\'e&IX&2\x10$^{-13}$&7\x10$^{-10}$&2.7\x10$^7$\cr
\noalign{\bigskip\smallskip}
&&\multispan 2\hfill{\bf Uranus}\hfill&\cr
\noalign{\medskip}
Cord\'elia&VI&7.0\x10$^{-15}$&1.6\x10$^{-10}$&9.3\x10$^5$\cr
Oph\'elie&VII&1.3\x10$^{-14}$&2.9\x10$^{-10}$&1.7\x10$^6$\cr
Miranda& V&0.33\x10$^{-10}$&0.76\x10$^{-6}$&4.4\x10$^9$\cr
Ariel&I&6.80\x10$^{-10}$&1.56\x10$^{-5}$&90.3\x10$^9$\cr
Umbriel&II&5.89\x10$^{-10}$&1.35\x10$^{-5}$&78.2\x10$^9$\cr 
Titania&III&17.73\x10$^{-10}$&4.061\x10$^{-5}$&235.3\x10$^9$\cr 
Ob\'eron&IV&15.15\x10$^{-10}$&3.471\x10$^{-5}$&201.1\x10$^9$\cr  
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&&\multispan 2\hfill{\bf Neptune}\hfill&\cr
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Na•\"\i ade&III&5.0\x10$^{-14}$&9.7\x10$^{-10}$&6.6\x10$^6$\cr
Thalassa&IV&1.6\x10$^{-13}$&3.1\x10$^{-9}$&2.1\x10$^7$\cr
Despina&V&1.1\x10$^{-12}$&2.1\x10$^{-8}$&1.4\x10$^8$\cr
Galat\'ee&VI&1.9\x10$^{-12}$&3.6\x10$^{-8}$&2.5\x10$^8$\cr
Larissa&VII&2.2\x10$^{-12}$&4.2\x10$^{-8}$&2.9\x10$^8$\cr
Prot\'ee&VIII&2.0\x10$^{-11}$&3.9\x10$^{-7}$&2.7\x10$^9$\cr
Triton&I&1.08\x10$^{-8}$&2.09\x10$^{-4}$&1.428\x10$^{12}$\cr 
N\'er\'eide&II&1\x10$^{-11}$&2\x10$^{-7}$&1.4\x10$^9$\cr     
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&&\multispan 2\hfill{\bf Pluton}\hfill&\cr 
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Charon&I&0.975\x10$^{-9}$&0.1567&12.9\x10$^{10}$\cr
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