Skip to main content
Admissions guidance, study banks, and career tools — get started on Shalyam
Research News

Tiny Whirlpools Spotted on the Surface of the Sun

Mayur Tembhare
  1. Tiny whirlpools have been spotted on the surface of the Sun for the first time.

  2. The discovery was made by a team of researchers from the US, Germany, and the USA using advanced computer simulations and observations from the world's largest solar telescope.

  3. The newly detected vortices appear along the boundaries of structures known as granules, which densely cover the Sun's visible surface.

  4. Individual granules are typically between 500 and 2,000 kilometers across.

Tiny Whirlpools Spotted on the Surface of the Sun

Topic: Space

Scientists have discovered tiny whirlpools on the surface of the Sun. These whirlpools are swirling motions that could help explain how the Sun stores and releases energy. The discovery was made by a team of researchers from the US, Germany, and the USA using advanced computer simulations and observations from the world's largest solar telescope.

Scientists have captured images of tiny whirlpools on the surface of the Sun. These whirlpools are swirling motions that could help explain how the Sun stores and releases energy. The discovery comes from researchers at the US National Science Foundation National Solar Observatory (NSO), the Max Planck Institute for Solar System Research (MPS) in Germany, and the High Altitude Observatory (HAO) in the USA.

The team used observations from the world's largest solar telescope, the Daniel K. Inouye Solar Telescope, which is built and operated by the NSO in Hawaii. The telescope provided images that were detailed enough to expose plasma motions that had never previously been visible. To detect these whirlpools, the researchers needed to resolve structures on the solar surface about 20 kilometers in size.

The newly detected vortices appear along the boundaries of structures known as granules, which densely cover the Sun's visible surface. Individual granules are typically between 500 and 2,000 kilometers across. The comparison of granulation to bubbles in a boiling liquid is fitting because it is produced by moving plasma.

The researchers believe these swirling flows are evidence of Kelvin-Helmholtz instabilities, a phenomenon that occurs when two fluids move alongside one another at different speeds. This can produce shear forces where the two flows meet, leading to waves or swirling vortices.

Why It Matters

Understanding how the Sun stores and releases energy is crucial for predicting solar flares and coronal mass ejections, which can affect satellite communications and navigation systems used by India's space program. This discovery could also help scientists better understand the behavior of magnetic fields in other stars and planets.

Key Facts

  • Tiny whirlpools have been spotted on the surface of the Sun for the first time.
  • The discovery was made by a team of researchers from the US, Germany, and the USA using advanced computer simulations and observations from the world's largest solar telescope.
  • The newly detected vortices appear along the boundaries of structures known as granules, which densely cover the Sun's visible surface.
  • Individual granules are typically between 500 and 2,000 kilometers across.
  • The researchers believe these swirling flows are evidence of Kelvin-Helmholtz instabilities.

Key Terms

plasma
A gas-like state of matter that makes up the Sun's surface.
Kelvin-Helmholtz instabilities
Phenomena that occur when two fluids move alongside one another at different speeds, producing shear forces and waves or swirling vortices.
granules
Structures on the Sun's surface that are densely packed and produce granulation.

Implications

Understanding how the Sun stores and releases energy is crucial for predicting solar flares and coronal mass ejections, which can affect satellite communications and navigation systems used by India's space program. This discovery could also help scientists better understand the behavior of magnetic fields in other stars and planets.

Source: https://www.sciencedaily.com/releases/2026/08/260807035142.htm

Journal reference:

  1. David Kuridze, Friedrich Wöger, Michiel van Noort, Matthias Rempel, Robert Cameron, Thomas Rimmele, Sami K. Solanki, Sarah A. Jaeggli, Alexandra Tritschler, Han Uitenbroek, Damien Przybylski, David A. Boboltz. Ubiquitous Kelvin–Helmholtz instabilities driving plasma mixing on the Sun. Nature, 2026; DOI: 10.1038/s41586-026-10871-3

Leave a comment

← All research

Get Exclusive Insights with Every Issue

Join Shalyam Newsletter

Stay ahead in education, research, and innovation—straight to your inbox.