Gamma-ray Bursts and Terrestrial Planetary Atmospheres

dc.contributor.authorThomas, Brian C. and Melott, Adrian L.en_US
dc.date.accessioned2014-09-29en_US
dc.date.accessioned2018-11-02T14:38:43Z
dc.date.available2014-09-29en_US
dc.date.available2018-11-02T14:38:43Z
dc.description.abstractWe describe results of modelling the effects on Earth-like planets of long-duration gamma-ray bursts (GRBs) within a few kiloparsecs. A primary effect is generation of nitrogen oxide compounds which deplete ozone. Ozone depletion leads to an increase in solar UVB radiation at the surface, enhancing DNA damage, particularly in marine microorganisms such as phytoplankton. In addition, we expect increased atmospheric opacity due to build-up of nitrogen dioxide produced by the burst and enhanced precipitation of nitric acid. We review here previous work on this subject and discuss recent developments, including further discussion of our estimates of the rates of impacting GRBs and the possible role of short-duration bursts.en_US
dc.format.medium.pdfen_US
dc.identifier.urihttps://hdl.handle.net/10425/350
dc.language.isoengen_US
dc.publisheren_US
dc.relationBrian C. Thomas ia a Washburn University faculty member.en_US
dc.subjectAstrophysics, Atmospheric and oceanic physics, Geophysics, Populations and evolutionen_US
dc.titleGamma-ray Bursts and Terrestrial Planetary Atmospheresen_US
washburn.identifier.cdm6en_US
washburn.identifier.oclcen_US
washburn.source.locationen_US
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