Peculiar planetary system architecture around three Orion stars explained

New observations of GW Orionis, a triple star system with a peculiar inner region, revealed that this object has a warped planet-forming disk with a misaligned ring.
New observations of GW Orionis, a triple star system with a peculiar inner region, revealed that this object has a warped planet-forming disk with a misaligned ring. The image on the right is from the SPHERE instrument on the European Southern Observatory’s Very Large Telescope, which allowed astronomers to see, for the first time, the shows this ring casts on the rest of the disk. This helped the researchers figure out the 3D shape of the ring and the overall disk. The left panel shows an artistic impression of the disk’s inner region, including the ring, which is based on the 3D shape reconstructed by the team. Credit: ESO/L. Calçada, Exeter/Kraus et al.
Thursday, September 03, 2020 


Washington, DC— The discovery that our galaxy is teeming with exoplanets has also revealed the vast diversity of planetary systems out there and raised questions about the processes that shaped them. New work published in Science by an international team including Carnegie’s Jaehan Bae could explain the architecture of multi-star systems in which planets are separated by wide gaps and do not orbit on the same plane as their host star’s equatorial center.

“In our Solar System, the eight planets and many other minor objects orbit in a flat plane around the Sun; but in some distant systems, planets orbit on an incline—sometimes a very steep one,” Bae explained. “Understanding the origins of extremely oblique orbital angles such as these could help reveal details about the planetary formation process.”

Stars are born in nurseries of gas and dust called molecular clouds—often forming in small groups of two or three. These young stars are surrounded by rotating disks of leftover material, which accretes to form baby planets. The disk’s structure will determine the distribution of the planets that form from it, but much about this process remains unknown.

This computer simulation shows the evolution of the GW Orionis system. The scientists believe the disc around the three stars in the system was initially flat, much like the planet-forming disc we see around many stars. Their simulation shows that the misalignment in the orbits of the three stars caused the disc around them to break into distinct rings, which is exactly what they see in the observations of the system. Credit: Exeter/Kraus et al.

Led by University of Exeter’s Stefan Kraus, the team found the first direct evidence confirming the theoretical prediction that gravitational interactions between the members of multi-star systems can warp or break their disks, resulting in misaligned rings surrounding the stellar hosts.

Over a period of 11 years, the researchers made observations of the GW Orionis triple-star system, located just over 1,300 light-years away in the Orion constellation. Their work was accomplished using the European Southern Observatory’s Very Large Telescope and the Atacama Large Millimeter/submillimeter Array—a radio telescope made up of 66 antennas.

Our images reveal an extreme case where the disk is not flat at all, but is warped and has a misaligned ring that has broken away from the disk,” Kraus said.

Their findings were tested by simulations, which demonstrated that the observed disorder in the orbits of the three stars could have caused the disk to fracture into the distinct rings.

We predict that many planets on oblique, wide-separation orbits will be discovered in future planet imaging campaigns,” said co-author Alexander Kreplin, also of the University of Exeter.

Bae concluded: “This system is a great example of how theory and observing can inform each other. I’m excited to see what we learn about this system and others like it with additional study.”

A team of astronomers using ESO’s Very Large Telescope (VLT), the VLT Interferometer and ALMA, in which ESO is a partner, have studied GW Orionis, a triple star system with a peculiar inner region. Unlike the flat planet-forming discs we see around many stars, GW Orionis features a warped disc, deformed by the movements of the three stars at its centre. This animation allows the viewer to see the warped disc and the tilted ring that was torned apart from it in spectacular detail. The animation is based on a computer model of the inner region of GW Orionis, provided by the team; they were able to reconstruct the 3D orbits of the stars and the 3D shape of the disc from the observational data. Credit: ESO/Exeter/Kraus et al./L. Calçada


Support for this research was provided by the European Research Council under the European Commission’s Horizon 2020 program Seventh Framework program; the Science Technology and Facilities Council; the U.S. NSF; NASA; the research council of the KU Leuven; and the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy.

The Carnegie Institution for Science (carnegiescience.edu) is a private, nonprofit organization headquartered in Washington, D.C., with six research departments throughout the U.S. Since its founding in 1902, the Carnegie Institution has been a pioneering force in basic scientific research. Carnegie scientists are leaders in plant biology, developmental biology, astronomy, materials science, global ecology, and Earth and planetary science.


Contact: Jaehan Bae at  jbae@carnegiescience.edu

For copies of the paper contact scipak@aaas.org

EOS Press Release




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