A renovated knowledge of the lunar librations is exposed in the present pap
er: This updating derives both from progress of observational techniques of
the Moon's motions and fi om theoretical methods of celestial dynamics. Fi
rst is presented a summary of classical libration families such as the appa
rent librations, the physical librations, ol the called fr ee librations. A
mbiguities and redundancies of this cutting out are discussed On the one ha
nd lunar librations ala strongly overlapped and datum of their branching is
not immediate. On the other hand, new librations have been made into evide
nce. Starting from a causal analysis of libration nature, the necessary arr
angement of the lunar librations is first based on the modern knowledge of
dynamical systems. It takes then into account the post-Newtonian gravitatio
n acquisitions in use of reference systems required for dealing with rotati
on motions combined with translation ones. By the way of the new families o
f lunar librations, namely the potential and kinetical librations, the pape
r gives the libration amplitudes discovered at the joint epoch of the LLR e
xperiment and elaborated methods of numerical integrations of the coupled s
pin-or-bit motion of the Moon The paper presents also a description of the
lunar. rides If takes stock on the I-elation between the accurate study of
the Moon's librations and the knowledge of its internal structure. Finally,
it takes into account the lunar spin-or-bit interaction whereby the mechan
ism of the secular acceleration of the Moon is marched by a secular slowing
-down of its rotation. (C) 2000 Academie des sciences/Editions scientifique
s Pt medicales Elsevier SAS.