Japan Geoscience Union Meeting 2019

Presentation information

[J] Oral

B (Biogeosciences ) » B-CG Complex & General

[B-CG08] Phanerozoic biodiversity change: Extinction and diversification

Tue. May 28, 2019 1:45 PM - 3:15 PM 105 (1F)

convener:Yukio Isozaki(Department of Earth Science and Astronomy, Multi-disciplinary Sciences - General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo), Yusuke Sawaki(The University of Tokyo), Chairperson:Wataru Fujisaki(Japan Agency for Marine-Earth Science and Technology)

3:00 PM - 3:15 PM

[BCG08-10] Mass extinctions: hierarchy of causes and cosmoclimatological perspective

*Yukio Isozaki1 (1.Department of Earth Science and Astronomy, Multi-disciplinary Sciences - General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo)

Keywords:mass extinction, global cooling, GCR, extinction cause

This paper reviews possible causes proposed for the double-stepped extinction in regard of the current status of mass extinction studies. Causes of extinction can be grouped into four categories; from small to large scale, Caterogry 1 to Category 4. Category 1 – direct kill mechanism, Category 2 – global environmental change, Category 3 – trigger on the planet’s surface, and Category 4 – ultimate cause. Among the Big-5 mass extinctions of the Phanerozic, two events in the Paleozoic, i.e.,the Hirnantian (Ordovician) and end-Guadalupian (Permian) events, show significant similarities in various aspects. Biological and non-biological aspects unique to these two distinct events include changes in biodiversity, isotope ratios (C, Sr etc.) of seawater, sea level, ocean redox state, episodic volcanism, and geomagnetism. In particular, the similar appearance of global cooling (Category 2) suggests the same cause and processes were likely responsible for the biodiversity drop. In addition to the most prevalent scenario of mantle plume-generated large igneous provinces (LIPs) (Category 3) for the end-Permian extinction, an emerging perspective of cosmoclimatology is introduced with respect to astrobiology. Galactic cosmic radiation (GCR) and solar/terrestrial responses in magnetism (Category 4) could have had a profound impact on Earth’s climate, in particular, on extensive cloud coverage (irradiance shutdown). Furthermore, the star-burst events detected in the Milky Way Galaxy apparently coincide in timing with the cooling-associated major extinctions of the Phanerozoic and also with the Proterozoic snowball Earth episode. As an ultimate cause (Category 4) for major extinction, the episodic increase in GCR flux from the source (dark clouds derived from star-burst) against the geomagnetic shield likely determined the major climate changes, particularly global cooling in the past. The study of mass extinctions on Earth is entering a new stage with a new astrobiological perspective.