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Researchers trace Venus' lower haze to cosmic dust, not volcanic ash

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GoKawiil Brief

A team led by planetary scientist Hiroki Karyu at Tohoku University used a microphysical model to explain the yellowish haze in Venus' lower atmosphere, first seen by Venera and Pioneer Venus probes in the 1970s. The study, published in Nature Astronomy, found the haze forms when sulfuric acid reacts with dust particles left behind by meteorites burning up in the atmosphere, ruling out volcanic ash or surface dust as the source.

Why It Matters

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The finding resolves a decades-old puzzle about Venus' atmosphere and suggests cosmic dust plays a broader role in shaping the planet's clouds than previously assumed, since Karyu's team says these particles help seed cloud formation elsewhere in the main cloud deck. It also narrows the case against volcanic activity as the explanation, even as other research indicates Venus remains more volcanically active than once believed.

Key Takeaways
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Source: arstechnica.com, 2026-10-01

Published there as: “Venus' mysterious haze is actually cosmic dust”

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