Illustration of the dust ring surrounding HD 181327. Credit: Amanda Smith, University of Cambridge
Astronomers have found evidence of ice and comets orbiting a nearby sun-like star, which could give a glimpse into how our own solar system developed. Using Atacama Large Millimeter Array (ALMA), the researchers, led by the University of Cambridge, detected very low levels of CO around the star, in amounts that are consistent with the comets in our own solar system. The results are a first step in establishing the properties of comet clouds around sun-like stars just after the time of their birth.
Comets are essentially ‘dirty snowballs’ of ice and rock, sometimes with a tail of dust and evaporating ice trailing behind them, and are formed early in the development of stellar systems. They are typically found in the outer reaches of our solar system, but become most clearly visible when they visit the inner regions. Eg, Halley’s Comet visits the inner solar system every 75 years, some take as long as 100,000 years between visits, and others only visit once before being thrown out into interstellar space.
It’s believed that when our solar system was first formed, the Earth was a rocky wasteland, similar to how Mars is today, and that as comets collided with the young planet, they brought many elements and compounds, including water, along with them. The star in this study, HD 181327, has a mass ~30% greater than the sun and is 160 light years away in the Painter constellation. The system is about 23 million years old, whereas our solar system is 4.6 billion years old. “Young systems such as this one are very active, with comets and asteroids slamming into each other and into planets,” said Sebastián Marino. “The system has a similar ice composition to our own, so it’s a good one to study in order to learn what our solar system looked like early in its existence.”
Using ALMA, the astronomers observed the star, which is surrounded by a ring of dust caused by the collisions of comets, asteroids and other bodies. It’s likely that this star has planets in orbit around it, but they are impossible to detect using current telescopes.
To detect comets, ALMA was used to search for gas signatures, since the same collisions which caused the dust ring to form should also cause the release of gas. Until now, such gas has only been detected around a few stars, all more massive than the sun. Using simulations to model the composition of the system, they were able to increase the signal to noise ratio in the ALMA data, and detect very low levels of carbon monoxide gas. http://www.cam.ac.uk/research/news/first-evidence-of-icy-comets-orbiting-a-sun-like-star
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