Two nearby supernovae that exploded about 2.5 and eight million years ago could have resulted in a staggered depletion of Earth's ozone layer, leading to a variety of repercussions for life on Earth.
In particular, 2.5 million years ago, the Earth was changing dramatically. The Pliocene, which was a hot and balmy epoch, was ending and the Pleistocene, an era of repeated glaciation known as the Ice Age, was beginning. Natural variations in Earth's orbit and wobble likely accounted for the change in climate, but the simultaneous event of a supernova could provide insight on the diversification of life during this epoch.
This supernova is thought to have occurred between 163 and 326 light-years away (50–100 parsecs) from Earth. For perspective, our closest stellar neighbor, Proxima Centauri, is 4.2 light-years away. [Proxima b: Closest Earth-Like Planet Discovery in Pictures]
Consequences for Earth
Supernovae can sterilize any nearby inhabited planets that happen to be in the path of their harmful ionizing radiation. Could nearby supernovae wreak havoc on the existing biology of our planet? One researcher wanted to find out. Brian Thomas, an astrophysicist at Washburn University in Kansas, modeled the biological impacts at the Earth's surface, based on geologic evidence (opens in new tab) of nearby supernovae 2.5 million and 8 million years ago.
In his latest paper, which was published in the journal Astrobiology, Thomas investigated cosmic rays from the supernovae as they propagated through our atmosphere to the surface, to understand their effect on living organisms.
Looking at the fossil record during the Pliocene-Pleistocene boundary (2.5 million years ago), we see a dramatic change in the fossil record and in land cover globally. Thomas told Astrobiology Magazine that "there were changes, especially in Africa, which went from being more forested to more grassland." During this time, the geologic record shows an elevated global concentration of iron-60 (60Fe), which is a radioactive isotope produced during a supernova.
"We are interested in how exploding stars affect life on Earth, and it turns out a few million years ago there were changes in the things that were living at the time," Thomas said. "It might have been connected to this supernova."
For example, there was a change in the abundance of species during the Pliocene-Pleistocene boundary. Although no major mass extinctions happened, there was a higher rate of extinction in general, more speciation and a change in vegetation. [Supernova Photos: Great Images of Star Explosions]
Not quite so deadly
How would a nearby supernova affect life on Earth? Thomas laments that supernovae often are exemplified as "supernova goes off and everything dies," but that is not quite the case. The answer lies in Earth's atmosphere. The ozone layer protects all biology from harmful, genetically altering ultraviolet (UV) radiation. Thomas used global climate models, recent atmospheric chemistry models and radiative transfer (the propagation of radiation through the layers of the atmosphere) to better understand how the flux of cosmic rays from supernovae would alter Earth's atmosphere, specifically the ozone layer.
One thing to note is that cosmic rays from supernovae would not blast everything in their paths all at once. The intergalactic medium acts as a kind of sieve, slowing down the arrival of cosmic rays and "radioactive iron rain" (60Fe) over hundreds of thousands of years, Thomas told Astrobiology Magazine. Higher-energy particles will reach Earth first and interact with our atmosphere differently than lower-energy particles arriving later. Thomas's study modeled the depletion in ozone 100, 300, and 1,000 years after the initial particles from a supernova began penetrating our atmosphere. Interestingly, depletion peaked (at roughly 26 percent) for the 300-year case, beating out the 100-year case.
The high-energy cosmic rays in the 100-year case would zip right through the stratosphere and deposit their energy below the ozone layer, depleting it less, while the less energetic cosmic rays arriving during the 300-year interval would deposit more energy in the stratosphere, depleting ozone significantly.
A decrease in ozone could be a concern for life on the surface.
"This work is an important step towards understanding the impact of nearby supernovae on our biosphere," said Dimitra Atri, a computational physicist at the Blue Marble Space Institute of Science in Seattle, who was not involved in the new study.
Thomas examined several possible biologically damaging effects (erythema, skin cancer, cataracts, marine phytoplankton photosynthesis inhibition and plant damage) at different latitudes as a result of increased UV radiation resulting from a depleted ozone layer. They showed heightened damage across the board, generally increasing with latitude, which makes sense given the changes we see in the fossil record. However, the effects aren't equally detrimental to all organisms. Plankton, the primary producers of oxygen, seemed to be minimally affected. The results also suggested a small increase in the risk of sunburn and skin cancer among humans.
So, do nearby supernovae result in mass extinctions? It depends, Thomas said.
"There is a subtler shift; instead of a 'wipe-out everything,' some [organisms] are better off and some are worse off," he said.
For example some plants showed increase yield, like soybean and wheat, while other plants showed reduced productivity. "It fits," Thomas stated, referring to the change in species in the fossil record.
In the future, Thomas hopes to expand on this work and examine possible linkages between human evolution and supernovae.
The work was supported by NASA Astrobiology through the Exobiology & Evolutionary Biology Program.