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Lava Planet 55 Cancri e Defies Expectations with Reflective Silicate Cloud Atmosphere

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Lava Planet 55 Cancri e Defies Expectations with Reflective Silicate Cloud Atmosphere

Here is what the page “Lava Planet 55 Cancri e Defies Expectations with Reflective Silicate Cloud Atmosphere” contains. Astronomers have detected what appears to be a reflective atmosphere on 55 Cancri e, a rocky lava planet once considered too extreme to hold onto any gases. The atmosphere is thought to contain vaporized silicate mineral clouds—the same family of compounds as quartz and sand. This discovery challenges previous assumptions about which exoplanets can sustain atmospheres. The finding matters because it expands the range of worlds that could host atmospheric layers, even under scorching conditions.

Researchers used data from the James Webb Space Telescope to infer the presence of these clouds. The planet, located about 41 light-years away, orbits its star so closely that its surface is likely molten. Understanding such extreme environments helps scientists refine models of planetary formation and evolution. This listing links straight to the original page, where the content is available in full.

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