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    Press and public relations officer
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    Max Planck Institute for Astronomy, Heidelberg

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    Dr. Norbert Junkes
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    Max Planck Institute for Radio Astronomy, Bonn

    Max Planck Institute for Radio Astronomy

    Dr. Roy van Boekel
    Head of Protoplanetary Disk Science Group
    Phone:+49 6221 528-405

    Max Planck Institute for Astronomy, Heidelberg

    Max Planck Institute for Astronomy

    Prof. Dr. Thomas K. Henning
    Director
    Phone:+49 6221 528-200

    Max Planck Institute for Astronomy, Heidelberg

    Max Planck Institute for Astronomy

    Prof. Dr. Gerd Weigelt
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    Phone:+49 228 525-243

    Max Planck Institute for Radio Astronomy, Bonn

    Max Planck Institute for Radio Astronomy

    Original publication

    1.
    J. Varga, M. Hogerheijde, R. van Boekel et al.
    The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?
    DOI

    Related article

    MPIA Institute announcement from 5 March 2018

    MATISSE sees first light at ESO´s Paranal Observatory in Chile

    MPIA Institute announcement from 5 March 2018 [more]

    Links

    Cosmic brick factory

    A new instrument reveals the site for planet birth around a young star

    January 21, 2021

    Studying the formation of planets close to their host stars by observations has been extremely challenging so far. As part of an international collaboration, scientists - among others from the Max Planck Institutes for Astronomy and for Radioastronomy - have employed a new instrument called MATISSE which has now uncovered evidence for a vortex at the inner rim of a planet-forming disk around a young star. It appears to move on an orbit around its star similar to Mercury’s orbit around the Sun. Astronomers think such vortices are sites where small particles converge and grow to form planets’ building blocks. Max Planck researchers contributed considerably to building MATISSE, an infrared imager for ESO’s Very Large Telescope Interferometer.
    The reconstructed image of the dusty disk (left) around the young star HD 163296, derived from the MATISSE observations. The false-colour image shows the thermal radiation from the disk at infrared wavelengths. The observations revealed a strong asymmetry which presents itself as a bright clump located at the upper right part in the image. A vortex concentrating material in a horseshoe-shaped region in the inner disk (to the right) could be causing this asymmetry. It orbits the central star at a distance similar to that of Mercury revolving around the Sun. Zoom Image
    The reconstructed image of the dusty disk (left) around the young star HD 163296, derived from the MATISSE observations. The false-colour image shows the thermal radiation from the disk at infrared wavelengths. The observations revealed a strong asymmetry which presents itself as a bright clump located at the upper right part in the image. A vortex concentrating material in a horseshoe-shaped region in the inner disk (to the right) could be causing this asymmetry. It orbits the central star at a distance similar to that of Mercury revolving around the Sun. [less]

    Astronomers have discovered more than 4000 planets orbiting stars other than the Sun. However, scientists still have to figure out the details of how those planets form from the disks made of dust and gas that surround their parent stars. During recent years, sophisticated instrumentation has provided close-up views on such planet-forming disks. However, they generally lack the angular resolution and sensitivity to probe the disks’ inner regions where terrestrial planets are supposed to emerge from rocky building blocks that eventually grow from tiny dust grains.

    An extensive collaboration of scientists led by Jozsef Varga from Leiden Observatory (The Netherlands) have now managed to overcome those limits by utilising a new instrument called MATISSE (Multi AperTure mid-Infrared SpectroScopic Experiment). The observations were made with essential contributions by astronomers of the Max Planck Institutes for Astronomy (MPIA) and for Radioastronomy (MPIfR). At infrared wavelengths these observations provide evidence for a vortex embedded inside a ring of hot dust at the inner edge of the protoplanetary disk of the young star HD 163296. The potential vortex revealed itself as a hot spot that produces an asymmetry at the disk’s inner edge. The scientists inferred that it revolves around the star roughly within a month by including published data. Its trajectory resides at a distance from the central star comparable to Mercury’s orbit around the Sun.

    Theoretical calculations have predicted the occurrence of vortices in disks, where material swirls around like a tornado and accumulates dust. “The higher dust density induces faster grain growth than anywhere else in the disk, which may render those whirls to be efficient factories to produce the building blocks of future planets,” Roy van Boekel explains. He leads the Protoplanetary Disk Science Group and manages the MATISSE project at MPIA. Some of the newly formed rocky bricks collide under high speeds which causes grinding of the material to tiny grains. They can attain higher temperatures than larger pebbles which is the likely origin of the hot spot found in the data.

    Group photo of the MATISSE team next to a MATISSE instrument cryostat. Zoom Image
    Group photo of the MATISSE team next to a MATISSE instrument cryostat.

    This spectacular result will appear in the scientific journal Astronomy & Astrophysics as the MATISSE team’s first scientific publication. “MATISSE is a new infrared instrument for the VLTI (Very Large Telescope Interferometer) which the European Southern Observatory (ESO) operates at its Paranal site in Chile,” Michael Lehmitz, an engineer at MPIA says. “MPIA contributed to an international consortium that designed and built MATISSE by integrating the delicate optics into a cryostat that cools them down to -235° C.” Subsequent low-temperature performance tests were also carried out at MPIA. MATISSE combines the light collected from up to four individual VLT units, performing spectroscopic and imaging observations. With such a design, the facility simulates the imaging power of a telescope of up to 200 metres in diameter, capable of producing the most detailed images ever at mid-infrared wavelengths.

    “We explicitly designed MATISSE to probe the inner zones of exoplanet-forming disks that have not been accessible before by available astronomical instrumentation,” Thomas Henning, director at MPIA and Co-PI of MATISSE points out. “I am proud and excited that the discovery of a potential vortex in the disk of HD 163296 demonstrates that we can investigate the processes that produce Earth-like planets at small distances from the host star.”

    The study presented here belongs to an extensive Guaranteed Time Observation (GTO) program, which investigates the planet-forming mechanisms in the inner zones of protoplanetary disks. Over the next few years, the GTO program will study many more systems like HD 163296. This way, it will improve our understanding of how the formation of Earth-like planets proceeds around a wide variety of young stars.

    "This first scientific result marks the starting point for further research. One of the goals is to study stars with dust disks and specifically those in which Earth-like planets can form," says Gerd Weigelt, director at MPIfR, who led a long involvement in the development of MATISSE as head of the Infrared Interferometry Research Group at the institute.

    MN

     
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