  High entry speed (> 25 km/s) and low density (< 2500 kg/m3) are two factors
that lower the chance of a meteoroid to drop meteorites. The 26 g carbonaceous
(CM2) meteorite Maribo recovered in Denmark in 2009 was delivered by a
superbolide observed by several instruments across northern and central Europe.
By reanalyzing the available data, we confirmed the previously reported high
entry speed of (28.3 +/- 0.3) km/s and trajectory with slope of 31 degrees to
horizontal. In order to understand how such a fragile material survived, we
applied three different models of meteoroid atmospheric fragmentation to the
detailed bolide light curve obtained by radiometers located in Czech Republic.
The Maribo meteoroid was found to be quite inhomogeneous with different parts
fragmenting at different dynamic pressures. While 30 - 40% of the (2000 +/-
1000) kg entry mass was destroyed already at 0.02 MPa, another 25 - 40%,
according to different models, survived without fragmentation until relatively
large dynamic pressures of 3 - 5 MPa. These pressures are only slightly lower
than the measured tensile strengths of hydrated carbonaceous chondrite (CC)
meteorites and are comparable with usual atmospheric fragmentation pressures of
ordinary chondritic (OC) meteoroids. While internal cracks weaken OC meteoroids
in comparison with meteorites, this effects seems to be absent in CC, enabling
meteorite delivery even at high speeds, though in the form of only small
fragments.
