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Reading: Astronomers using Webb telescope discover resilient dust from galaxy Makani’s intense journey
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Home » Blog » Astronomers using Webb telescope discover resilient dust from galaxy Makani’s intense journey
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Astronomers using Webb telescope discover resilient dust from galaxy Makani’s intense journey

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Last updated: September 10, 2025 8:07 AM
David Graff
Published: September 10, 2025
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  • Astronomers using the James Webb Space Telescope (JWST) have discovered tiny dust particles traveling far from their home galaxy, Makani, surviving a perilous journey through harsh cosmic environments that should have destroyed them.
  • These findings offer new insights into how galaxies grow, breathe, and recycle the raw materials that fuel future generations of stars.
  • The dust originates from Makani, a compact but massive galaxy that recently underwent intense bursts of star formation, propelling gas and dust outward into the galaxy’s vast halo of hot gas known as the circumgalactic medium (CGM).
  • Using JWST’s infrared instruments, the team detected the faint glow of polycyclic aromatic hydrocarbons (PAHs), complex organic molecules that cling to dust grains and serve as tracers of how dust behaves while traveling through a galaxy’s harsh environment.

Why it matters: Observing these dust grains as they move in and out of galaxies gives astronomers a new window into the life cycle of galaxies and the cosmic recycling of matter.

What they’re saying:

  • “Before this study, there had not been a direct detection of dust on such a large scale,” said lead author Sylvain Veilleux, an astronomy professor at the University of Maryland, College Park. “Webb was the key that made it happen.”
  • “It shouldn’t survive,” Veilleux said. “If dust touches gas at 10,000 degrees, it’s going to vaporize it.” Yet much of the dust endures, likely cocooned by protective cooler gas pockets.
  • “Galaxies are living beasts in a way,” Veilleux said. “They’re still evolving, and that cycle of gas in and out is important in knowing what will happen in the future.”

The researchers propose a survival mechanism called “cloud-wind mixing,” in which dust grains are shielded by cooler pockets of gas while the surrounding hotter gas slowly dissipates. This mechanism explains why PAH emission is detectable at such vast distances from the galaxy.

What’s next: Follow-up research could aim to push observations even farther, potentially detecting dust in the vast spaces between galaxies. Such a discovery could trace a journey of a million light-years or more, revealing just how far galactic material can travel.

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ByDavid Graff
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David is the editor-in-chief of Techpinions.com. Technologist, writer, journalist.
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