Does nitrate deposition following astrophysical ionizing radiation events pose an additional threat to amphibians?
arXiv:0804.3604 · doi:10.1089/ast.2007.0262
Abstract
It is known that amphibians are especially susceptible to the combination of heightened UVB radiation and increased nitrate concentrations. Various astrophysical events have been suggested as sources of ionizing radiation that could pose a threat to life on Earth, through destruction of the ozone layer and subsequent increase in UVB, followed by deposition of nitrate. In this study, we investigate whether the nitrate deposition following an ionizing event is sufficiently large to cause an additional stress beyond that of the heightened UVB previously considered. We have converted predicted nitrate depositions to concentration values, utilizing data from the New York State Department of Environmental Conservation Acid Rain Monitoring Network web site. Our results show that the increase in nitrate concentration in bodies of water following the most intense ionization event likely in the last billion years would not be sufficient to cause a serious additional stress on amphibian populations and may actually provide some benefit by acting as fertilizer.
This version is a longer, more detailed draft of an article submitted to the journal Astrobiology
References in corpus (4)
- Gamma-Ray Bursts and the Earth: Exploration of Atmospheric, Biological, Climatic and Biogeochemical Effects
- Terrestrial Consequences of Spectral and Temporal Variability in Ionizing Photon Events
- Superluminous supernovae: No threat from Eta Carinae
- Gamma-ray bursts and terrestrial planetary atmospheres
Cited by in corpus (7)
- Cosmic Rays and Terrestrial Life: A Brief Review
- A supernova at 50 pc: Effects on the Earth's atmosphere and biota
- Ground-level ozone following astrophysical ionizing radiation events: an additional biological hazard?
- Atmospheric Consequences of Cosmic Ray Variability in the Extragalactic Shock Model II: Revised ionization levels and their consequences
- Terrestrial effects of moderately nearby supernovae
- Ozone depletion-induced climate change following a 50 pc supernova
- Climate change via co2 drawdown from astrophysically initiated atmospheric ionization?