Proc. Neutrino Astrophysics - MPP Theory Group
Proc. Neutrino Astrophysics - MPP Theory Group
Proc. Neutrino Astrophysics - MPP Theory Group
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6<br />
What Killed The Dinosaurs?<br />
Arnon Dar 1,2<br />
1 Max-Planck-Institut für Physik (Werner-Heisenberg-Institut)<br />
Föhringer Ring 6, 80805 München, Germany.<br />
2 Department of Physics and Space Research Institute,<br />
Technion, Israel Institute of Technology, Haifa 32000, Israel.<br />
The early history of life during the Precambrian until its end 570 million years (My) ago<br />
is poorly known. Since then the diversity of both marine and continental life has increased<br />
exponentially. Analysis of fossil records shows that this diversification was interrupted by five<br />
massive extinctions and some smaller extinction peaks [1]. The largest extinction occurred<br />
about 251 My ago at the end of the Permian period. The global species extinction ranged then<br />
between 80% to 95%, much more than, for instance, the Cretaceous-Tertiary extinction 64 My<br />
ago which killed the dinosaurs and claimed ∼ 47% of existing genera [2]. In spite of intensive<br />
studies it is still not known what caused the mass extinctions. Many extinction mechanisms<br />
have been proposed but no single mechanism seems to provide a satisfactory explanation of<br />
the complex geological records on mass extinctions [3]. These include terrestrial mechanisms<br />
such as intense volcanism, which coincided only with two major extinctions [4] or drastic<br />
changes in sea level, climate and environment that occurred too often, and astrophysical<br />
mechanisms, such as a meteoritic impact that explains the iridium anomaly which was found at<br />
the Cretaceous/Tertiary boundary [5] but has not been found in any of the other extinctions,<br />
supernova explosions [6] and gamma ray bursts [7] which do not occur close enough at a<br />
sufficiently high rate to explain the observed rate of mass extinctions.<br />
The geological records, however, seem to indicate that an accidental combination of drastic<br />
events [3] occurred around the times of the major extinctions. For instance, the dinosaur<br />
extinction coincides in time with a large meteoritic impact, with a most intensive volcanic<br />
eruption and with a drastic change in sea level and climate. The origin of these correlations is<br />
still unclear. Meteoritic impacts alone or volcano eruptions alone or sea regression alone could<br />
not have caused all the major mass extinctions. An impact of a 10 km wide meteorite with<br />
a typical velocity of 30 km s −1 was invoked [5] in order to explain the Cretaceous-Tertiary<br />
(K/T) mass extinction 64 My ago, which killed the dinosaurs, and the iridium anomaly<br />
observed at the K/T boundary. But neither an iridium anomaly nor a large meteoritic<br />
crater have been dated back to 251 My ago, the time of the Permian/Triassic (P/T) mass<br />
extinction, which was the largest known extinction in the history of life [3] where the global<br />
species extinction ranged between 80% to 95%. The gigantic Deccan volcanism in India that<br />
occurred around the K/T boundary [4] and the gigantic Siberian basalts flood that occurred<br />
around the P/T boundary have ejected approximately 2×10 6 km 3 of lava [4]. They were more<br />
than a thousand times larger than any other known eruption on Earth, making it unlikely<br />
that the other major mass extinctions, which are of a similar magnitude, were produced<br />
by volcanic eruptions. Although there is no one-to-one correspondence between major mass<br />
extinctions, large volcanic eruptions, large meteoritic impacts, and drastic environmental<br />
changes, there are clear time correlations between them. We propose that near encounters<br />
of Earth with “visiting planets” from the outer solar system are responsible for most of the<br />
mass extinctions on planet Earth and can explain both the above correlations and the detailed<br />
geological records on mass extinctions [8].