Show simple item record

Rates of fixation by lightning of carbon and nitrogen in possible primitive atmospheres

dc.contributor.authorChameides, W. L.en_US
dc.contributor.authorWalker, James C. G.en_US
dc.date.accessioned2006-09-08T21:20:26Z
dc.date.available2006-09-08T21:20:26Z
dc.date.issued1981-12en_US
dc.identifier.citationChameides, W. L.; Walker, J. C. G.; (1981). "Rates of fixation by lightning of carbon and nitrogen in possible primitive atmospheres." Origins of Life 11(4): 291-302. <http://hdl.handle.net/2027.42/43346>en_US
dc.identifier.issn0302-1688en_US
dc.identifier.issn1573-0875en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43346
dc.identifier.urihttp://www.ncbi.nlm.nih.gov/sites/entrez?cmd=retrieve&db=pubmed&list_uids=6276836&dopt=citationen_US
dc.description.abstractA thermochemical-hydrodynamic model of the production of trace species by electrical discharges has been used to estimate the rates of fixation of C and N by lightning in the primitive atmosphere. Calculations for various possible mixtures of CH 4 , CO 2 , N 2 , H 2 , and H 2 O reveal that the prime species produced were probably HCN and NO and that the key parameter determining the rates of fixation was the ratio of C atoms to O atoms in the atmosphere. Atmospheres with C more abundant than O have large HCN fixation rates, in excess of 10 17 molecules J −1 , but small NO yields. However, when O is more abundant than C, the NO fixation rate approaches 10 17 molecules J −1 while the HCN yield is small. The implications for the evolution of life are discussed.en_US
dc.format.extent657114 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; D. Reidel Publishing ; Springer Science+Business Mediaen_US
dc.subject.otherLife Sciencesen_US
dc.subject.otherOrganic Chemistryen_US
dc.subject.otherGeochemistryen_US
dc.subject.otherBiochemistry, Generalen_US
dc.titleRates of fixation by lightning of carbon and nitrogen in possible primitive atmospheresen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelNatural Resources and Environmenten_US
dc.subject.hlbsecondlevelEcology and Evolutionary Biologyen_US
dc.subject.hlbsecondlevelBiological Chemistryen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelHealth Sciencesen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumSpace Physics Research Laboratory, University of Michigan, Ann Arbor, Michigan, USAen_US
dc.contributor.affiliationotherSchool of Geophysical Sciences, Georgia Institute of Technology, Atlanta, Georgia, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.identifier.pmid6276836en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43346/1/11084_2004_Article_BF00931483.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00931483en_US
dc.identifier.sourceOrigins of Lifeen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.