Astronomers have discovered a new kind of stellar explosion that could be commonplace in the universe and may change our understanding of how eruptions in stars occur.
A micronova is a thermonuclear blast that lasts for just a few hours making them extremely difficult to observe.
These outbursts happen on the surface of certain stars and can each rapidly burn through a huge amount of stellar material equivalent to around 3.5 billion Great Pyramids of Giza.
An international team of researchers, led by Durham University, UK, saw the phenomenon in three white dwarfs—the remnants of dead stars—as they fed in each case on a companion star.
They say their discovery could lead to more micronovae being found and challenge what we know about how thermonuclear explosions occur in stars.
The research is published in the journal Nature.
The team first came across the unusual micronovae when they noticed a bright flash of light lasting for a short time while analyzing data from NASA’s Transiting Exoplanet Survey Satellite (TESS).
In total they have since observed three micronovae using TESS—normally used to look for planets outside of our solar system.
Two micronovae were from already known white dwarfs, but the third needed more observations with the X-Shooter instrument on the European Southern Observatory’s (ESO) Very Large Telescope (VLT) for its white dwarf status to be confirmed.
Lead author Dr. Simone Scaringi, in the Centre for Extragalactic Astronomy, Durham University, said: “We have discovered and identified for the first time what we are calling a micronova. The phenomenon challenges our understanding of how thermonuclear explosions in stars occur. We thought we knew this, but this discovery proposes a totally new way to achieve them. It just goes to show how dynamic the Universe is. These events may actually be quite common, but because they are so fast they are difficult to catch in action.”
Micronovae are extremely powerful, but are small on astronomical scales compared to novae and supernovae, which are extremely bright and have been known about for centuries. There are numerous accounts across history of “new stars” being seen by astronomers that we now call novae.
In novae this thermonuclear explosion occurs over the entire surface of the star and the intensely bright light from this blast can be seen for weeks. Some supernova, on the other hand, are so energetic they burn the entire white dwarf.
Both types of explosions occur on white dwarfs, dead stars with a mass similar to that of our Sun, but as small as the Earth in size.
White dwarfs can steal material, mostly hydrogen, from their companion stars if they are close enough to them.
As the hydrogen falls on to the very hot surface of the dwarf star its atoms fuse into helium in explosive fashion.
In novae this thermonuclear explosion occurs over the entire surface of the star and the intensely bright light from this blast can be seen for weeks.
Micronovae are similar explosions that are smaller in scale and faster, lasting several hours.
The researchers say that they occur on some white dwarfs with strong magnetic fields, which funnel material towards the star’s magnetic poles.
Study co-author Professor Paul Groot, of Radboud University, the Netherlands, said: “For the first time, we have now seen that hydrogen fusion can also happen in a localized way.
“The hydrogen fuel can be contained at the base of the magnetic poles of some white dwarfs, so that fusion only happens at these magnetic poles.
“This leads to micro-fusion-bombs going off, which have the strength of about one millionth of a nova explosion, hence the name ‘micronova.’”
The team now wants to capture more of these elusive events, which will require large-scale surveys and quick follow-up measurements.
Scaringi added: “Rapid response from telescopes such as the VLT or ESO’s New Technology Telescope and the suite of available instruments will allow us to truly unravel what these mysterious micronovae are.”
The research was funded in the UK by the Science and Technology Facilities Council.
- This press release was originally published on the Durham University website