Scientific Frontline: "At a Glance" Summary: Shear-Flow Instability in Planet Formation
- Main Discovery: Researchers have provided the first experimental evidence that shear-flow instability occurs under conditions similar to planet-forming regions, bridging a critical gap in understanding how fine dust aggregates into planetesimals.
- Methodology: The team developed the TEMPus VoLA experiment, utilizing high-speed cameras to track the behavior of dust particles in an extremely thin gas under vacuum conditions during parabolic flights that provided simulated microgravity.
- Key Data: Each parabolic flight dive phase provided weightlessness for approximately 20 seconds, successfully allowing the observation of characteristic material flow patterns before turbulence fully developed.
- Significance: This confirmation proves that shear-flow instability is a tangible physical process capable of fostering denser dust clouds in protoplanetary disks, addressing the theoretical barrier that prevents centimeter- to hundred-meter-sized boulders from growing.
- Future Application: The experimental apparatus is being advanced for deployment on the International Space Station (ISS), where extended periods of microgravity will allow for the observation of fully developed turbulence to refine theoretical models and computer simulations.
- Branch of Science: Astrophysics, Planetary Science, Fluid Dynamics.
- Additional Detail: The research was published in Communications Physics and represents a collaborative effort among the University of Bern, the University of Zurich, ETH Zurich, and the National Center of Competence in Research (NCCR) PlanetS.

.jpg)
.jpg)





.jpg)
.jpg)
.jpg)
.jpg)

