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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].

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