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The semimetal—one part cerium, four parts ruthenium, and six parts tin—seems to be naturally quantum critical, meaning it sits at the edge of multiple phases of matter
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New Johns Hopkins University simulations offer an intriguing look into Saturn s interior, suggesting that a thick layer of helium rain influences the planet s magnetic field.
AGU Advances, also indicate that Saturn s interior may feature higher temperatures at the equatorial region, with lower temperatures at the high latitudes at the top of the helium rain layer.
It is notoriously difficult to study the interior structures of large gaseous planets, and the findings advance the effort to map Saturn s hidden regions. By studying how Saturn formed and how it evolved over time, we can learn a lot about the formation of other planets similar to Saturn within our own solar system, as well as beyond it, said co-author Sabine Stanley, a Johns Hopkins planetary physicist.