HD 189733b, a hot Jupiter exoplanet 64 light years away with surface temperatures of 1,700°F, contains hydrogen sulfide (rotten egg molecule) despite extreme heat that should have boiled off water and ammonia during formation, indicating that hot Jupiters likely form farther out in freezing zones where sulfur compounds survive and then migrate inward, challenging the traditional gas giant formation model.
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This Planet Reeks of Rotten Eggs and Breaks Every Rule We Had #Shorts追加:
HD189733b defies physics and it reeks of hydrogen sulfide. The myth is that all gas giants form the same way Jupiter did, ice and rock first then gas. HD189733b is a hot Jupiter 64 light years away with clouds of hydrogen sulfide, the rotten egg molecule. It orbits so close to its star that surface temps hit 1700° Fahrenheit. At that heat, water and ammonia should have boiled off during formation. But here's what breaks the textbook, it still has sulfur. That means hot Jupiters don't form where we thought. They likely spawn farther out in freezing zones where sulfur compounds survive then migrate inward.
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