An astronomer from the University of Warwick has recently captured a double star system that has flipped its surrounding disc to a position that leaps over the orbital plane of those stars. The system composed of a thick hoop of gas and dust circling at right angles to the binary star orbit.
An international team of astronomers used Atacama Large Millimeter/submillimeter Array (ALMA) to obtain high-resolution images of the Asteroid belt-sized disc. Their observations prove that polar discs of this type exist, and may even be relatively common.
Dr Grant M. Kennedy of the University of Warwick said, “Discs rich in gas and dust are seen around nearly all young stars, and we know that at least a third of the ones orbiting single stars form planets. Some of these planets end up being misaligned with the spin of the star, so we’ve been wondering whether a similar thing might be possible for circumbinary planets. A quirk of the dynamics means that a so-called polar misalignment should be possible, but until now we had no evidence of misaligned discs in which these planets might form.”
Using ALMA, astronomers pinned down the orientation of the ring of gas and dust in the system. The orbit of the binary was previously known, from observations that quantified how the stars move in relation to each other. They then combined these two pieces of information to establish that the dust ring was consistent with a perfectly polar orbit.
It means, the stellar orbits orbit each other in one plane, like two horses going around on a carousel, the disc surrounds these stars at right angles to their orbits, like a giant Ferris wheel with the carousel at the center.
Dr Grant M. Kennedy of the University of Warwick added: “Perhaps the most exciting thing about this discovery is that the disc shows some of the same signatures that we attribute to dust growth in discs around single stars. We take this to mean planet formation can at least get started in these polar circumbinary discs. If the rest of the planet formation process can happen, there might be a whole population of misaligned circumbinary planets that we have yet to discover, and things like weird seasonal variations to consider.”
“If there were a planet or planetoid present at the inner edge of the dust ring, the ring itself would appear from the surface as a broad band rising almost perpendicularly from the horizon. The polar configuration means that the stars would appear to move in and out of the disc plane, giving objects two shadows at times.”
“Seasons on planets in such systems would also be different. On Earth, they vary throughout the year as we orbit the Sun. A polar circumbinary planet would have seasons that also vary at different latitudes receive more or less illumination throughout the binary orbit.”
Co-author Dr. Daniel Price of Monash University’s Centre for Astrophysics (MoCA) and School of Physics and Astronomy added:
“We used to think other solar systems would form just like ours, with the planets all orbiting in the same direction around a single sun. But with the new images, we see a swirling disc of gas and dust orbiting around two stars. It was quite surprising to also find that that disc orbits at right angles to the orbit of the two stars.”
“Incredibly, two more stars were seen orbiting that disc. So if planets were born here there would be four suns in the sky!”
“ALMA is just a fantastic telescope, it is teaching us so much about how planets in other solar systems are born.”
The study is presented in the journal Nature Astronomy.