Five thousand light-years away in the Monoceros constellation, strange materials are swirling around a young star known as V960 Mon.
Astronomers were baffled when the star’s brightness rapidly increased by over 20 times back in 2014. Now, observations published in The Astrophysical Journal Letters have helped to explain the secrets behind these events in fascinating detail.
New images reveal large, dusty ‘clumps’ as large as planets gathering around the star. If these collapse, they could form giant planets as massive as Jupiter.
“This discovery is truly captivating,” said Dr Alice Zurlo of the Universidad Diego Portales, Chile, a researcher involved in the observations.
The images, released by the European Southern Observatory (ESO), show that the material orbiting the star is assembling into spiral ‘arms’ that extend over distances bigger than our entire Solar System.
These formations were detected using the creatively named Very Large Telescope (VLT) and the Atacama Large Millimeter/submillimeter Array (ALMA), which probe around the surface of the spiral arms as well as deep into their intricate structures.
The observations could help astronomers learn more about the secrets behind the formation of large planets. Currently there are two theories as to how this happens.
The first is called core accretion, which is essentially when dust grains join together. The second is gravitational instability, which involves large material around a star contracting and collapsing into a planet. The clumps around V960 Mon could provide evidence of this second theory, which so far has had limited support.
“Our group has been searching for signs of how planets form for over ten years, and we couldn't be more thrilled about this incredible discovery,” said Sebastián Pérez, one of the researchers from the University of Santiago, Chile.
As if the Very Large Telescope wasn’t enough, the ESO is currently building an Extremely Large Telescope (ELT) in the Atacama Desert in Chile. This will allow the astronomers to observe the system in even greater detail, including the chemical compositions of the forming planets.
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