Some classic expansions of the elliptic motion - cos m E and sin m E -
in powers of the eccentricity are extended to highly eccentric orbits
, 0.6627... < e < 1. The new expansions are developed in powers of (e
- e), where e* is a fixed value of the eccentricity. The coefficients
are given in terms of the derivatives of Bessel functions with respec
t to the eccentricity. The expansions have the same radius of converge
nce rho(e) of the extended solution of Kepler's equation, previously
derived by the author. Some other simple expansions - (a/r), (r/a), (r
/a) sin v,..., - derived straightforward from the expansions of E, cos
E and sin E are also presented.