Astronomers discover micronovae, a new kind of stellar explosion
Tuesday 10 May 2022
Artist’s impression of a micronova - Credit: ESO/M. Kornmesser, L. Calçada ESO, 20th April 2022. A team of astronomers, with the help of
the European Southern Observatory’s Very Large Telescope (ESO’s VLT),
have observed a new type of stellar explosion — a micronova. These
outbursts happen on the surface of certain stars, and can each burn
through around 3.5 billion Great Pyramids of Giza of stellar material in
only a few hours. “We have discovered and identified for the first time what we are calling a micronova,”
explains Simone Scaringi, an astronomer at Durham University in the UK
who led the study on these explosions published today in Nature.
“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,” he adds. Micronovae are extremely powerful events, but are small on
astronomical scales; they are much less energetic than the stellar
explosions known as novae, which astronomers have known about for
centuries. Both types of explosions occur on white dwarfs, dead stars
with a mass about that of our Sun, but as small as Earth. A white dwarf in a two-star system can steal material,
mostly hydrogen, from its companion star if they are close enough
together. As this gas falls onto the very hot surface of the white dwarf
star, it triggers the hydrogen atoms to fuse into helium explosively.
In novae, these thermonuclear explosions occur over the entire stellar
surface. “Such detonations make the entire surface of the white dwarf burn and shine brightly for several weeks,” explains co-author Nathalie Degenaar, an astronomer at the University of Amsterdam, the Netherlands. Micronovae are similar explosions that are smaller in scale
and faster, lasting just several hours. They occur on some white dwarfs
with strong magnetic fields, which funnel material towards the star’s
magnetic poles. “For the first time, we have now seen that hydrogen
fusion can also happen in a localised 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,” says Paul Groot, an astronomer at Radboud University in the Netherlands and co-author of the study. “This leads to micro-fusion bombs going off, which have
about one millionth of the strength of a nova explosion, hence the name
micronova,” Groot continues. Although ‘micro’ may imply these
events are small, do not be mistaken: just one of these outbursts can
burn through about 20 000 000 trillion kg, or about 3.5 billion Great
Pyramids of Giza, of material [1]. These new micronovae challenge astronomers’ understanding
of stellar explosions and may be more abundant than previously thought. “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,” Scaringi explains. The team first came across these mysterious
micro-explosions when analysing data from NASA’s Transiting Exoplanet
Survey Satellite (TESS). “Looking through astronomical data
collected by NASA’s TESS, we discovered something unusual: a bright
flash of optical light lasting for a few hours. Searching further, we
found several similar signals,” says Degenaar. The team observed three micronovae with TESS: two were from
known white dwarfs, but the third required further observations with
the X-shooter instrument on ESO’s VLT to confirm its white dwarf status. “With help from ESO’s Very Large Telescope, we found that all these optical flashes were produced by white dwarfs,” says Degenaar. “This observation was crucial in interpreting our result and for the discovery of micronovae,” Scaringi adds. The discovery of micronovae adds to the repertoire of known
stellar explosions. The team now want to capture more of these elusive
events, requiring large scale surveys and quick follow-up measurements. “Rapid response from telescopes such as the VLT or ESO’s New Technology Telescope and the suite of available instruments will allow us to unravel in more detail what these mysterious micronovae are,” Scaringi concludes. Notes[1] We use trillion to mean a million million (1,000,000,000,000 or 1012) and billion to mean a thousand million (1,000,000,000 or 109).
The weight of the Great Pyramid of Giza in Cairo, Egypt (also known as
the Pyramid of Khufu or Pyramid of Cheops) is about 5,900,000,000 kg. More informationThis research was presented in a paper title
"Localised thermonuclear bursts from accreting magnetic white dwarfs"
(doi: 10.1038/s41586-022-04495-6) to appear in Nature. A
follow-up letter, titled "Triggering micronovae through magnetically
confined accretion flows in accreting white dwarfs" has been accepted
for publication in Monthly Notices of the Royal Astronomical Society. The team on the Nature paper is composed of S.
Scaringi (Centre for Extragalactic Astronomy, Department of Physics,
Durham University, UK [CEA]), P. J. Groot (Department of Astrophysics,
Radboud University, Nijmegen,the Netherlands [IMAPP] and South African
Astronomical Observatory, Cape Town, South Africa [SAAO] and Department
of Astronomy, University of Cape Town, South Africa [Cape Town]), C.
Knigge (School of Physics and Astronomy, University of Southampton,
Southampton, UK [Southampton]), A.J. Bird (Southampton) , E. Breedt
(Institute of Astronomy, University of Cambridge, UK), D. A. H. Buckley
(SAAO, Cape Town, Department of Physics, University of the Free State,
Bloemfontein, South Africa), Y. Cavecchi (Instituto de Astronomía,
Universidad Nacional Autónoma de México, Ciudad de México, México), N.
D. Degenaar (Anton Pannekoek Institute for Astronomy, University of
Amsterdam, Amsterdam, the Netherlands), D. de Martino (INAF-Osservatorio
Astronomico di Capodimonte, Naples, Italy), C. Done (CEA), M. Fratta
(CEA), K. Iłkiewicz (CEA), E. Koerding (IMAPP), J.-P. Lasota (Nicolaus
Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw,
Poland and Institut d’Astrophysique de Paris, CNRS et Sorbonne
Universités, Paris, France), C. Littlefield (Department of Physics,
University of Notre Dame, USA and Department of Astronomy, University of
Washington, Seattle, USA [UW]), C. F. Manara (European Southern
Observatory, Garching, Germany [ESO]), M. O’Brien (CEA), P. Szkody (UW),
F. X. Timmes (School of Earth and Space Exploration, Arizona State
University, Arizona, USA, Joint Institute for Nuclear Astrophysics -
Center for the Evolution of the Elements, USA). The European Southern Observatory (ESO) enables scientists
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