Thank exploding stars for our galaxy’s gold
All the elements on Earth, from those that create us humans to the air we breathe and even the jewellery we wear, all come from cosmological phenomena like exploding stars. Scientists have now discovered a new type of cosmic explosion that is likely to have created elements, such as oxygen, iron and gold, in our galaxy’s earliest stars.
Meaning, the gold jewellery you own may be made of star dust as old as the earliest era of the Milky Way.
Science worth its weight in gold
The study found evidence that one of the most powerful explosive events in our universe produced heavy elements in the earliest era of the Milky Way. The discovery was made using the SkyMapper Telescope in Australia.
The event, called a magnetorotational hypernova, is a spinning, super-energetic supernova created by the collapse of a massive star.
Dr Chiaki Kobayashi, co-author and Reader in Astrophysics at the University of Hertfordshire, said:
“We would like to understand where we come from. The elements which compose our human bodies come from stars. But what about mobile phones, which contains previous metals such as copper, silver, and gold?
“Ancient stars we can observe only with big telescopes are amazing as they have recorded the history of the Universe like fossils in archaeology. The discovery of this star is proof that these elements come from an explosion of a massive star, probably 25 times more massive than the Sun, about 13 billion years ago.”
The discovery of the precious star, known as SMSS J200322.54-114203.3, was the made using the SkyMapper Telescope in Australia* led by David Yong and Gary Da Costa from Australia’s ARC Centre of Excellence in All Sky Astrophysics in 3 Dimensions (ASTRO 3D) based at the Australian National University (ANU).
Jewellers should thank their lucky (dead) stars
The research conducted by Dr Kobayashi was supported by the Science and Technology Facilities Council (STFC), part of UK Research and Innovation, through a nuclear astrophysics consortium BRIDGCE. The STFC-supported study follows on from pioneering analysis by an international team of female astrophysicists in 2020.
The all-female team led by Dr Kobayashi analysed the origins of all the elements in the periodic table. Their research concluded that spinning supernovae are most likely to be responsible for creating the abundance very heavy elements such as gold in the cosmos, rather than neutron star collisions as previously believed.
This type of hypernovae also produced the light elements formed during massive star evolution and the iron-peak elements generated by explosive nuclear burning.
The research paper, ’r-Process elements from magnetorotational hypernovae’, is now available to view in Nature.
*The star was discovered by the SkyMapper Telescope (in Australia), but the elements were measured by the 6.5-m Magellan telescope at the Las Campanas Observatory in Chile and ESO’s Very Large Telescope.
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