Kazumi Ozaki

ORCID: 0000-0003-1121-8921
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About
Contact & Profiles
Research Areas
  • Paleontology and Stratigraphy of Fossils
  • Geology and Paleoclimatology Research
  • Astro and Planetary Science
  • Methane Hydrates and Related Phenomena
  • Marine and coastal ecosystems
  • Geochemistry and Elemental Analysis
  • Isotope Analysis in Ecology
  • Atmospheric and Environmental Gas Dynamics
  • Ocean Acidification Effects and Responses
  • Marine Biology and Ecology Research
  • Geological and Geophysical Studies
  • Marine and environmental studies
  • Geological Studies and Exploration
  • Hydrocarbon exploration and reservoir analysis
  • Geological and Geochemical Analysis
  • Atmospheric Ozone and Climate
  • Planetary Science and Exploration
  • Stellar, planetary, and galactic studies
  • Space Science and Extraterrestrial Life
  • Astronomy and Astrophysical Research
  • Microbial Community Ecology and Physiology
  • Pacific and Southeast Asian Studies
  • Groundwater and Isotope Geochemistry
  • Advanced Image and Video Retrieval Techniques
  • Shape Memory Alloy Transformations

The University of Tokyo
2011-2024

NASA Astrobiology Institute
2018-2024

NASA Exoplanet Science Institute
2022-2024

National Aeronautics and Space Administration
2022-2024

Tokyo Institute of Technology
1988-2024

Japan Meteorological Agency
2023-2024

Life Science Institute
2023-2024

Meteorological Research Institute
2024

Toho University
2019-2023

Georgia Institute of Technology
2016-2022

The progressive oxygenation of the Earth's atmosphere was pivotal to evolution life, but puzzle when and how atmospheric oxygen (O2) first approached modern levels (∼21%) remains unresolved. Redox proxy data indicate deep oceans were oxygenated during 435-392 Ma, appearance fossil charcoal indicates O2 >15-17% by 420-400 Ma. However, existing models have failed predict at this time. Here we show that earliest plants, which colonized land surface from ∼470 Ma onward, responsible for...

10.1073/pnas.1604787113 article EN Proceedings of the National Academy of Sciences 2016-08-15

Abstract The emergence of oxygenic photosynthesis created a new niche with dramatic potential to transform energy flow through Earth’s biosphere. However, more primitive forms that fix CO 2 into biomass using electrons from reduced species like Fe(II) and H instead water would have competed early biosphere for essential nutrients. Here, we combine experimental microbiology, genomic analyses, Earth system modeling demonstrate competition light nutrients in the surface ocean between...

10.1038/s41467-019-10872-z article EN cc-by Nature Communications 2019-07-09

Abstract The possibility of low but nontrivial atmospheric oxygen (O 2 ) levels during the mid‐Proterozoic (between 1.8 and 0.8 billion years ago, Ga) has important ramifications for understanding Earth's O cycle, evolution complex life evolving climate stability. However, regulatory mechanisms redox fluxes required to stabilize these in face continued biological production remain uncertain. Here, we develop a biogeochemical model C‐N‐P‐O ‐S cycles use it constrain global balance...

10.1111/gbi.12317 article EN cc-by-nc-nd Geobiology 2018-10-03

Abstract The global silica cycle is an important component of the long-term climate system, yet its controlling factors are largely uncertain due to poorly constrained proxy records. Here we present a ∼70 Myr-long record early Mesozoic biogenic (BSi) flux from radiolarian chert in Japan. Average low-mid-latitude BSi burial superocean Panthalassa ∼90% that modern ocean and relative amplitude varied by ∼20–50% over 100 kyr 30 Myr orbital cycles during Mesozoic. We hypothesize was major sink...

10.1038/ncomms15532 article EN cc-by Nature Communications 2017-06-07

Abstract Carbon is an essential element for life on Earth, and the relative abundances of major carbon species (CO 2 , CO, CH 4 ) in atmosphere exert fundamental controls planetary climate biogeochemistry. Here we employed a theoretical model atmospheric chemistry to investigate diversity CO Earth-like lifeless planets orbiting Sun-like (F-, G-, K-type) stars. We focused conditions formation CO-rich atmosphere, which would be favorable origin life. Results demonstrated that elevated levels...

10.3847/1538-4357/ad10a2 article EN cc-by The Astrophysical Journal 2024-01-01

[1] Wind and wave records obtained from the Kvitebjorn platform (2.3°E, 61.0°N, 190 m deep) in northern North Sea 2003 to 2005 were analyzed. Among 2723 20-min taken during storm conditions, 57 cases included freak waves exceeding twice significant height. Comparisons between various parameters occurrence index did not show any correlation. Thus, situ record was used select days when relatively more or less observed. The classified into freakish non-freakish days, respectively. On Icelandic...

10.1029/2011gl047779 article EN Geophysical Research Letters 2011-07-01

Some atmospheric gases have been proposed as counter indicators to the presence of life on an exoplanet if remotely detectable at sufficient abundance (i.e., antibiosignatures), informing search for biosignatures and potentially fingerprinting uninhabited habitats. However, quantitative extent which putative antibiosignatures could exist in atmospheres inhabited planets is not well understood. The most commonly referenced potential antibiosignature CO, because it represents a source free...

10.3847/1538-4357/ab05e1 article EN cc-by The Astrophysical Journal 2019-03-15

Abstract The advent of oxygenic photosynthesis represents the most prominent biological innovation in evolutionary history Earth. exact timing evolution photoautotrophic bacteria remains elusive, yet these profoundly altered redox state ocean–atmosphere–biosphere system, ultimately causing first major rise atmospheric oxygen (O 2 )—the so‐called Great Oxidation Event (GOE)—during Paleoproterozoic (~2.5–2.2 Ga). However, it unclear how coupled atmosphere–marine biosphere system behaved after...

10.1111/gbi.12554 article EN Geobiology 2023-03-24

Iron (Fe) is an essential element for life, and its geochemical cycle intimately linked to the coupled history of life Earth's environment. The accumulated geologic records indicate that ferruginous waters existed in Precambrian oceans not only before first major rise atmospheric O2 levels (Great Oxidation Event; GOE) during Paleoproterozoic, but also rest Proterozoic. However, interactive evolution biogeochemical cycles Fe Archean-Proterozoic remains ambiguous. Here, we develop a model...

10.1111/gbi.12571 article EN publisher-specific-oa Geobiology 2023-08-25

Earth's ocean-atmosphere system has undergone a dramatic but protracted increase in oxygen (O2) abundance. This environmental transition ultimately paved the way for rise of multicellular life and provides blueprint how biosphere can transform planetary surface. However, estimates atmospheric levels large intervals history still vary by orders magnitude—foremost middle history. Historically, mid-Proterozoic (1.9–0.8 Ga) are inferred based on kinetics reactions occurring soils or oceans,...

10.1089/ast.2019.2060 article EN Astrobiology 2020-03-31

Abstract Earth’s orbital variations on timescales of 10 4 –10 5 years, known as Milankovitch cycles, have played a critical role in pacing climate change and ecosystem dynamics, through glacial and/or monsoon dynamics. However, the climatic biotic consequences these cycles much longer (~ 7 years) remain unclear, due to lack long proxy records with precise age constraints. Here, we show ~ 10-Myr scale early Mesozoic (250–180 Ma) lake-level, desert distribution, biogenic-silica burial flux,...

10.1038/s41598-020-68542-w article EN cc-by Scientific Reports 2020-07-23

Abstract The global‐scale oxygenation of Earth's surface represents one the most fundamental chemical transformations in our planet's history. There is empirical and theoretical evidence for at least two distinct stable regimes Earth oxygenation—a “low‐O 2 world” characterized by pervasively anoxic deep ocean waters, a “high‐O with dominantly well‐oxygenated waters represented modern environment. Numerous biogeochemical processes feedbacks control redox state marine system, particularly when...

10.1029/2021gb007052 article EN Global Biogeochemical Cycles 2022-01-01

Abstract The evolution and expansion of land plants brought about one the most dramatic shifts in history Earth system — birth modern soils likely stimulated massive changes marine biogeochemistry climate. Multiple extinctions characterized by widespread anoxia, including Late Devonian mass extinction around 372 million years ago, may have been linked to terrestrial release nutrient phosphorus driven newly-rooted landscapes. Here we use recently published lake records as variable inputs an...

10.1038/s43247-023-01087-8 article EN cc-by Communications Earth & Environment 2023-11-29

Abstract. A new Earth system model of intermediate complexity – CANOPS-GRB v1.0 is presented for use in quantitatively assessing the dynamics and stability atmospheric oceanic chemistry on Earth-like planets over geologic timescales. The release designed to represent coupled major element cycles C, N, P, O, S, as well global redox budget (GRB) Earth's exogenic (ocean–atmosphere–crust) system, using a process-based approach. This framework provides mechanistic evolution O2 levels timescales...

10.5194/gmd-15-7593-2022 article EN cc-by Geoscientific model development 2022-10-20

Abstract Understanding the oceanic phosphate concentration is critical for understanding marine productivity and oxygen evolution throughout Earth history. During Archean, estimates of levels range from scarce to enriched conditions. However, biogeochemical conditions required sustaining high concentrations while retaining an anoxic atmosphere during Archean remain ambiguous. Here, we employ a model cycle determine under which could have been higher than present‐day values after emergence...

10.1029/2023gl108077 article EN cc-by Geophysical Research Letters 2024-04-08

Understanding the oceanic phosphate concentration is critical for understanding marine productivity and oxygen evolutions throughout Earth history. During Archean, estimates of levels range from depleted to enriched conditions. However, biogeochemical conditions required sustaining high concentrations while retaining an anoxic atmosphere during Archean remain ambiguous. Here, we employ a model cycle determine under which could have been higher than present-day values after emergence oxygenic...

10.22541/essoar.170561632.22376910/v1 preprint EN cc-by-nc-nd Authorea (Authorea) 2024-01-18

Abstract The Capitanian stage is characterized by marine anoxia possibly related to the extinction, although global redox structure of ocean has not been constrained. We newly report a nitrogen isotope (δ 15 N) record from paleo‐atoll limestone at top mid‐Panthalassan seamount constrain spatial extent and duration anoxia. δ N value after acid treatment substantially high for ∼5‐Myr up +28‰, highest through Phanerozoic oceans, suggesting that source (nitrate) was enriched in via...

10.1029/2022pa004573 article EN cc-by-nc-nd Paleoceanography and Paleoclimatology 2023-05-22
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