Terrestrial Ozone Depletion Due To A Milky Way Gamma-Ray Burst

dc.contributor.authorThomas, Brian C., Jackman, Charles H., Melott, Adrian L., Laird, Claude M., Stolarski, Richard S., Gehrels, Neil, Cannizzo, John K., and Hogan, Daniel P.en_US
dc.date.accessioned2014-09-29en_US
dc.date.accessioned2018-11-02T14:38:12Z
dc.date.available2014-09-29en_US
dc.date.available2018-11-02T14:38:12Z
dc.description.abstractBased on cosmological rates, it is probable that at least once in the last Gy the Earth has been irradiated by a gamma-ray burst in our Galaxy from within 2 kpc. Using a two-dimensional atmospheric model we have performed the first computation of the effects upon the Earth's atmosphere of one such impulsive event. A ten second burst delivering 100 kJ/m(2) to the Earth penetrates to the stratosphere and results in globally averaged ozone depletion of 35%, with depletion reaching 55% at some latitudes. Significant global deplation persists for over 5 years after the burst. This depletion would have dramatic implications for life since a 50% decrease in ozone column density results in approximately three times the normal UVB flux. Widespread extinctions are likely, based on extrapolation from UVB sensitivity of modern organisms. Additional effects include a shot of nitrate fertilizer and NO2 opacity in the visible providing a cooling perturbation to the climate over a similar timescale. these results lend support to the hypothesis that a GRB may have initiated the late Ordovician mass extinction (Melott et al. 2004).en_US
dc.format.medium.pdfen_US
dc.identifier.urihttps://hdl.handle.net/10425/217
dc.language.isoengen_US
dc.publisheren_US
dc.relationBrian C. Thomas is a Washburn University faculty member.en_US
dc.subjectAstrobiology, Gamma-ray burstsen_US
dc.titleTerrestrial Ozone Depletion Due To A Milky Way Gamma-Ray Bursten_US
washburn.identifier.cdm15en_US
washburn.identifier.oclcen_US
washburn.source.locationen_US
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