What’s a safe distance from a supernova?
A supernova is a spectacular explosion of a massive star. If our sun exploded as a supernova, the resulting shock wave probably wouldn’t incinerate the entire Earth, but the side of Earth facing the sun would boil away. Scientists estimate that the planet as a whole would increase in temperature to roughly 15 times hotter than our sun’s normal surface temperature.
What’s more, Earth wouldn’t stay put in orbit. The sudden decrease in the sun’s mass might free the planet to wander off into space. Clearly, the sun’s distance – 8 light-minutes away – isn’t safe if it were to explode in a supernova. Fortunately, our sun isn’t the sort of star destined to explode as a supernova. But other stars, beyond our solar system, will.
What is the closest safe distance? According to a recent study based on data from the Chandra X-Ray Observatory , a supernova would have to be within 160 light-years of Earth before we would feel its damaging effects. Formerly, it was believed a supernova would have to be within 50 light-years of Earth to impact our planet. Another study found evidence a supernova within 300 light-years reached Earth millions of years ago, but it wouldn’t cause an extinction event. So, the answer varies and the research continues.
What would happen if a supernova exploded near Earth?
Let’s consider the explosion of a star that’s at an unsafe distance to Earth. Say, the supernova is 30 light-years away. Mark Reid, a senior astronomer at the Harvard-Smithsonian Center for Astrophysics, said:
… were a supernova to go off within about 30 light-years of us, that would lead to major effects on the Earth, possibly mass extinctions. X-rays and more energetic gamma rays from the supernova could destroy the ozone layer that protects us from solar ultraviolet rays. It also could ionize nitrogen and oxygen in the atmosphere, leading to the formation of large amounts of smog-like nitrous oxide.
What’s more, if a supernova exploded within 30 light-years, phytoplankton and reef communities would be particularly affected. Such an event would severely deplete the base of the ocean food chain.
Suppose the explosion were slightly more distant. An explosion of a nearby star might leave Earth and its surface and ocean life relatively intact. But any relatively nearby explosion would still shower us with gamma rays and other high-energy radiation. This radiation could cause mutations in earthly life. Also, the radiation from a nearby supernova could change our climate.
Fortunately, there are no stars within 30 light-years of Earth poised to go supernova.
Close supernovas in the not-so-distant past
No supernova has been known to erupt within 100’s of light-years in the known history of humankind. The most recent supernova visible to the eye was Supernova 1987A, in the year 1987. It was approximately 168,000 light-years away.
Before that, the last supernova visible to the eye was was documented by Johannes Kepler in 1604. At about 20,000 light-years, it shone more brightly than any star in the night sky. It was even visible in daylight! But it didn’t cause earthly effects, as far as we know.
How far away are the closest supernova candidates?
First, there are two different kinds of supernovas. A Type II supernova is an aging massive star that collapses. There are no stars massive enough to do this located within 160 light-years of Earth. A Type I supernova happens when a small, faint white dwarf star collapses due to infalling material of a companion. These stars are dim and hard to find, so we can’t be sure just how many are around. There are probably a few hundred of these stars within 160 light-years, but we don’t know of any ready to explode.
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The star IK Pegasi B is the nearest known supernova progenitor candidate. It’s part of a binary star system, located about 150 light-years from our sun and solar system.
The main star in the system – IK Pegasi A – is an ordinary main sequence star, not unlike our sun. The potential Type I supernova is the other star – IK Pegasi B – a massive white dwarf that’s extremely small and dense, orbiting closer to IK Pegasi A than Mercury is to our sun. When the A star begins to evolve into a red giant, it’s expected to grow to a radius where the white dwarf can accrete, or take on, matter from A’s expanded gaseous envelope. When the B star gets massive enough, it might collapse on itself, in the process exploding as a supernova.
