Bedoukian   RussellIPM   RussellIPM   Piezoelectric Micro-Sprayer


Home
Animal Taxa
Plant Taxa
Semiochemicals
Floral Compounds
Semiochemical Detail
Semiochemicals & Taxa
Synthesis
Control
Invasive spp.
References

Abstract

Guide

Alphascents
Pherobio
InsectScience
E-Econex
Counterpart-Semiochemicals
Print
Email to a Friend
Kindly Donate for The Pherobase

« Previous AbstractChemometric tools to highlight non-intentionally added substances (NIAS) in polyethylene terephthalate (PET)    Next AbstractEffect of pH and temperature on the kinetics of odor oxidation using chlorine dioxide »

Orig Life Evol Biosph


Title:Bolide impacts and the oxidation state of carbon in the Earth's early atmosphere
Author(s):Kasting JF;
Address:"Department of Geosciences, The Pennsylvania State University, University Park 16802"
Journal Title:Orig Life Evol Biosph
Year:1992
Volume:20
Issue:
Page Number:199 - 231
DOI: 10.1007/BF01808105
ISSN/ISBN:0169-6149 (Print) 0169-6149 (Linking)
Abstract:"A one-dimensional photochemical model was used to examine the effect of bolide impacts on the oxidation state of Earth's primitive atmosphere. The impact rate should have been high prior to 3.8 Ga before present, based on evidence derived from the Moon. Impacts of comets or carbonaceous asteroids should have enhanced the atmospheric CO/CO2 ratio by bringing in CO ice and/or organic carbon that can be oxidized to CO in the impact plume. Ordinary chondritic impactors would contain elemental iron that could have reacted with ambient CO2 to give CO. Nitric oxide (NO) should also have been produced by reaction between ambient CO2 and N2 in the hot impact plumes. High NO concentrations increase the atmospheric CO/CO2 ratio by increasing the rainout rate of oxidized gases. According to the model, atmospheric CO/CO2 ratios of unity or greater are possible during the first several hundred million years of Earth's history, provided that dissolved CO was not rapidly oxidized to bicarbonate in the ocean. Specifically, high atmospheric CO/CO2 ratios are possible if either: (1) the climate was cool (like today's climate), so that hydration of dissolved CO to formate was slow, or (2) the formate formed from CO was efficiently converted into volatile, reduced carbon compounds, such as methane. A high atmospheric CO/CO2 ratio may have helped to facilitate prebiotic synthesis by enhancing the production rates of hydrogen cyanide and formaldehyde. Formaldehyde may have been produced even more efficiently by photochemical reduction of bicarbonate and formate in Fe(++)-rich surface waters"
Keywords:"*Atmosphere Carbon Dioxide/*chemistry Carbon Monoxide/*chemistry *Earth, Planet Formaldehyde/chemical synthesis/chemistry Hydrogen Cyanide/chemical synthesis/chemistry Minor Planets *Models, Chemical Nitric Oxide/chemistry Oceans and Seas Oxidation-Reduct;"
Notes:"MedlineKasting, J F eng Netherlands 1992/01/01 Orig Life Evol Biosph. 1992; 20:199-231. doi: 10.1007/BF01808105"

 
Back to top
 
Citation: El-Sayed AM 2024. The Pherobase: Database of Pheromones and Semiochemicals. <http://www.pherobase.com>.
© 2003-2024 The Pherobase - Extensive Database of Pheromones and Semiochemicals. Ashraf M. El-Sayed.
Page created on 22-11-2024