  We describe the fall of Annama meteorite occurred in the remote Kola
Peninsula (Russia) close to Finnish border on April 19, 2014 (local time). The
fireball was instrumentally observed by the Finnish Fireball Network. From
these observations the strewnfield was computed and two first meteorites were
found only a few hundred meters from the predicted landing site on May 29th and
May 30th 2014, so that the meteorite (an H4-5 chondrite) experienced only
minimal terrestrial alteration. The accuracy of the observations allowed a
precise geocentric radiant to be obtained, and the heliocentric orbit for the
progenitor meteoroid to be calculated. Backward integrations of the orbits of
selected near-Earth asteroids and the Annama meteoroid showed that they rapidly
diverged so that the Annama meteorites are unlikely related to them. The only
exception seems to be the recently discovered 2014UR116 that shows a plausible
dynamic relationship. Instead, analysis of the heliocentric orbit of the
meteoroid suggests that the delivery of Annama onto an Earth-crossing Apollo
type orbit occurred via the 4:1 mean motion resonance with Jupiter or the nu6
secular resonance, dynamic mechanisms that are responsible for delivering to
Earth most meteorites studied so far.
