Astronomers image dusty disks, uncover companions to distant stars

Dusty disks imaged from NSF's NOIRLab
A survey of 44 young massive stars to investigate planet formation shows dusty, swirling disks — likely to become new solar systems. The images were taken with the Gemini Planet Imager (GPI) instrument on the Gemini South telescope of the International Gemini Observatory, a Program of NSF’s NOIRLab. Credit: International Gemini Observatory/NOIRLab/NSF/AURA/E. Rich (Michigan University)

This mosaic of dusty, swirling disks shows a sample of images captured from the International Gemini Observatory, a Program of NSF's NOIRLab, as part of an unprecedented survey of 44 young massive stars. An international team used Gemini South in Chile to investigate planet formation and uncovered a potential young Jupiter-mass planet, and confirmed the existence of two brown dwarfs. The images will be presented in sessions today at the 240th American Astronomical Society meeting.

This striking image, taken by astronomers using the Gemini South telescope in Chile, is part of a large survey of 44 young, by the Gemini Planet Imager (GPI) instrument, which imaged their dusty planet-forming disks—likely to become new solar systems—in near-. The survey found that the disks circling stars up to three times the mass of the Sun tend to have rings, whereas disks around stars that are more massive than three do not. This suggests that the more massive stars may form planets slightly differently.

Planets form in disks of gas and dust that encircle just a few million years old and GPI is one of a few instruments in the world capable of resolving these disks. Previous observations have indicated that rings, made of large and small dust grains as well as gas, are often seen in these disks. Exactly what creates these rings is uncertain, but they have been attributed to newborn planets interacting with the .

Astronomers conducting a survey called Gemini-LIGHTS (Gemini-Large Imaging with GPI Herbig/T-Tauri Survey) have sought to try and answer some of these questions by producing high-resolution images of the disks around a sample of 44 stars.

Astronomers image dusty disks, uncover companions to distant stars
A team led by University of Michigan postdoctoral researcher Evan Rich and professor John Monnier imaged 44 targets in a survey called Gemini-Large Imaging with GPI Herbig/T-tauri Survey, or Gemini-LIGHTS. The astronomers detected some form of dust around 80% of the 44 targets. The team released a gallery of 6 of the 44 targets showing a range of different morphologies that tell the researchers about the dynamics happening within the disk itself. Rich will present the summary paper’s findings at the American Astronomical Society’s annual meeting this month. His study has also been accepted for publication in the Astronomical Journal. Credit: Evan Rich, University of Michigan

"We want to answer the fundamental question of how planets form," said Evan Rich, who is a postdoc at the University of Michigan and the lead author of a new paper describing the results in The Astronomical Journal. In particular, he says the Gemini-LIGHTS survey, "concentrates on stars that are more massive than the Sun to investigate the influence that a parent star's mass might have on the process."

Gemini South captured the images of the disks in near-infrared and polarized light. It found disks around 80% of the 44 targeted stars, and also found one new candidate planet (around V1295 Aquilae) and three . Two of the brown dwarfs (around the stars (V921 Sco and HD 158643)) had already been identified as candidates by earlier observations and which have now been confirmed through these observations; the third brown dwarf, around the star HD 101412, is a new candidate.

The survey's key finding, however, is that the disks appear to behave differently depending upon the mass of the star they are circling. "Systems with small dust-grain rings are only found around stars with masses less than three times the mass of the Sun," said Rich. "This is important because forming are thought to create the ringed structure, and our findings suggest that the planet formation process might be different for stars larger than three times the mass of the Sun."

This information will be presented in a press conference and oral presentation today at the 240th American Astronomical Society Meeting.

This research was presented in a paper to appear in The Astronomical Journal.

More information: Gemini-LIGHTS: Herbig Ae/Be and massive T-Tauri protoplanetary disks imaged with Gemini Planet Imager, The Astronomical Journal (2022). DOI: 10.48550/arXiv.2206.05815

Journal information: Astronomical Journal

Provided by NOIRLab

Citation: Astronomers image dusty disks, uncover companions to distant stars (2022, June 15) retrieved 3 March 2024 from
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