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Jiang HJ, Underwood TC, Bell JG, Lei J, Gonzales JC, Emge L, Tadese LG, Abd El-Rahman MK, Wilmouth DM, Brazaca LC, Ni G, Belding L, Dey S, Ashkarran AA, Nagarkar A, Nemitz MP, Cafferty BJ, Sayres DS, Ranjan S, Crocker DR, Anderson JG, Sasselov DD, Whitesides GM. Mimicking lightning-induced electrochemistry on the early Earth. Proc Natl Acad Sci U S A 2024; 121:e2400819121. [PMID: 39074283 PMCID: PMC11317556 DOI: 10.1073/pnas.2400819121] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/16/2024] [Accepted: 06/10/2024] [Indexed: 07/31/2024] Open
Abstract
To test the hypothesis that an abiotic Earth and its inert atmosphere could form chemically reactive carbon- and nitrogen-containing compounds, we designed a plasma electrochemical setup to mimic lightning-induced electrochemistry under steady-state conditions of the early Earth. Air-gap electrochemical reactions at air-water-ground interfaces lead to remarkable yields, with up to 40 moles of carbon dioxide being reduced into carbon monoxide and formic acid, and 3 moles of gaseous nitrogen being fixed into nitrate, nitrite, and ammonium ions, per mole of transmitted electrons. Interfaces enable reactants (e.g., minerals) that may have been on land, in lakes, and in oceans to participate in radical and redox reactions, leading to higher yields compared to gas-phase-only reactions. Cloud-to-ground lightning strikes could have generated high concentrations of reactive molecules locally, establishing diverse feedstocks for early life to emerge and survive globally.
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Affiliation(s)
- Haihui Joy Jiang
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
- Department of Astronomy, Harvard University, Cambridge, MA02138
| | - Thomas C. Underwood
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
- Department of Aerospace Engineering and Engineering Mechanics, The University of Texas at Austin, Austin, TX78705
| | - Jeffrey G. Bell
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Jonathan Lei
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Joe C. Gonzales
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Lukas Emge
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Leah G. Tadese
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | | | - David M. Wilmouth
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
- Harvard John A. Paulson School of Engineering and Applied Sciences, Harvard University, Cambridge, MA02138
| | - Lais C. Brazaca
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Gigi Ni
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Lee Belding
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Supriya Dey
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Ali Akbar Ashkarran
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Amit Nagarkar
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Markus P. Nemitz
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - Brian J. Cafferty
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
| | - David S. Sayres
- Harvard John A. Paulson School of Engineering and Applied Sciences, Harvard University, Cambridge, MA02138
| | - Sukrit Ranjan
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ85721
- Department of Planetary Sciences, University of Arizona, Tucson, AZ85721
| | - Daniel R. Crocker
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA02138
| | - James G. Anderson
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
- Harvard John A. Paulson School of Engineering and Applied Sciences, Harvard University, Cambridge, MA02138
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA02138
| | | | - George M. Whitesides
- Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA02138
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Chowdhuri I, Pal SC, Saha A, Chakrabortty R, Ghosh M, Roy P. Significant decrease of lightning activities during COVID-19 lockdown period over Kolkata megacity in India. THE SCIENCE OF THE TOTAL ENVIRONMENT 2020; 747:141321. [PMID: 32771791 PMCID: PMC7385625 DOI: 10.1016/j.scitotenv.2020.141321] [Citation(s) in RCA: 27] [Impact Index Per Article: 6.8] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/25/2020] [Revised: 07/19/2020] [Accepted: 07/27/2020] [Indexed: 04/14/2023]
Abstract
The outbreak of COVID-19 has now created the largest pandemic and the World health organization (WHO) has declared social distancing as the key precaution to confront such type of infections. Most of the countries have taken protective measures by the nationwide lockdown. The purpose of this study is to understand the effect of lockdown on air pollutants and to analyze pre-monsoon (April and May) cloud-to-ground and inter-cloud lightning activity in relation to air pollutants i.e. suspended Particulate matter (PM10), Nitrogen dioxides (NO2) Sulfur dioxide (SO2), Ozone (O3) and Aerosol concentration (AC) in a polluted tropical urban megacities like Kolkata. After the strict lockdown the pollutants rate has reduced by more than 40% from the pre-lockdown period in the Kolkata megacity. So, decreases of PM10, NO2, SO2, O3 and AC have a greater effect on cloud lightning flashes in the pre-monsoon period. In the previous year (2019), the pre-monsoon average result shows a strong positive relation between the lightning and air pollutants; PM10 (R2 = 0.63), NO2 (R2 = 0.63), SO2 (R2 = 0.76), O3 (R2 = 0.68) and AC (R2 = 0.83). The association was relatively low during the lock-down period (pre-monsoon 2020) and the R2 values were 0.62, 0.60, 0.71, 0.64 and 0.80 respectively. Another thing is that the pre-monsoon (2020) lightning strikes decreased by 49.16% compared to the average of previous years (2010 to 2019). The overall study shows that the reduction of surface pollution in the thunderstorm environment is strongly related to the reduction of lightning activity where PM10 and AC are the key pollutants in the Kolkata megacity.
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Affiliation(s)
| | | | - Asish Saha
- Department of Geography, The University of Burdwan, West Bengal, India
| | | | - Manoranjan Ghosh
- Rural Development Centre, Indian Institute of Technology Kharagpur, West Bengal, India
| | - Paramita Roy
- Department of Geography, The University of Burdwan, West Bengal, India
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Pasek MA, Hurst M. A Fossilized Energy Distribution of Lightning. Sci Rep 2016; 6:30586. [PMID: 27466230 PMCID: PMC4964350 DOI: 10.1038/srep30586] [Citation(s) in RCA: 17] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/28/2016] [Accepted: 07/04/2016] [Indexed: 11/27/2022] Open
Abstract
When lightning strikes soil, it may generate a cylindrical tube of glass known as a fulgurite. The morphology of a fulgurite is ultimately a consequence of the energy of the lightning strike that formed it, and hence fulgurites may be useful in elucidating the energy distribution frequency of cloud-to-ground lightning. Fulgurites from sand mines in Polk County, Florida, USA were collected and analyzed to determine morphologic properties. Here we show that the energy per unit length of lightning strikes within quartz sand has a geometric mean of ~1.0 MJ/m, and that the distribution is lognormal with respect to energy per length and frequency. Energy per length is determined from fulgurites as a function of diameter, and frequency is determined both by cumulative number and by cumulative length. This distribution parallels those determined for a number of lightning parameters measured in actual atmospheric discharge events, such as charge transferred, voltage, and action integral. This methodology suggests a potential useful pathway for elucidating lightning energy and damage potential of strikes.
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Affiliation(s)
- Matthew A Pasek
- School of Geoscience, NES 204, University of South Florida, 4202 E Fowler Ave Tampa FL 33620, USA
| | - Marc Hurst
- Independent Geological Services, Inc. 4432 Burlington Drive, Winter Haven, FL 33880, USA
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