Two satellites \( A \) and \( B \), having masses in the ratio \( 4:3 \), are revolving in circular orbits of radii \( 3r \) and \( 4r \) respectively around the earth. The ratio of total mechanical energy of \( A \) to \( B \) is:
\( 9:16 \)
\( 16:9 \)
\( 1:1 \)
\( 4:3 \)