As faraway stars die, they generate massive solar winds that eject up to half the star’s mass into space, where it becomes accessible for building Earth-like planets.
Such stars are called red giants and their death throes create these superwinds that last 10,000 years and are 100 million times stronger than the wind from our sun.
Until now, superwinds were thought to be driven by tiny dust grains or silicates in a dying star’s halo that are pushed away by starlight. However, based on this theory, dust grains would overheat and evaporate.
Led by Barnaby Norris at Australia’s University of Sydney, an international team of astronomers used the European Southern Observatory’s (ESO) Very Large Telescope in Chile to observe the dust shells around three red giant stars.
They found that silicate grains can reach unexpectedly large sizes of 300 nanometers (1 nanometer is one-billionth of a meter), giving them much stronger reflective abilities. Hence they act like mirrors, staying cool despite the star’s intense radiation, and can be pushed out without disintegrating.
The scientists believe these large wind-driving grains are accelerated by scattered, not absorbed, light, traveling at the speed of a rocket—20,000 miles per hour (10 km per second). Although they are tiny in comparison to sand grains, a superwind is similar in effect to a sandstorm.
This discovery is a breakthrough in our understanding of superwinds and how sun-like stars die, said Albert Zijilstra at the UK’s University of Manchester in a press release.
“The dust and sand in the superwind will survive the star, and later become part of the clouds in space from which new stars form,” he explained. “The sand grains at that time become the building blocks of planets.”
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