The temperature of TOI-421 b is about 1,340 degrees Fahrenheit, well above the presumed threshold. Without haze or clouds, researchers expected to see a clear atmosphere – and they did!
The lightweight hydrogen atmosphere was the big surprise to theresearchers. “We had recently wrapped our mind around the idea that those first few sub-Neptunes observed by Webb had heavy-molecule atmospheres, so that had become our expectation, and then we found the opposite,” said Kempton. This suggests TOI-421 b may have formed and evolved differently from the cooler sub-Neptunes observed previously.
The findings raise big questions:
Q: Did TOI-421 b form differently than the cooler sub-Neptunes we’ve studied before?
Q: Could it represent a whole new class of hot, haze-free sub-Neptunes?
Q: Or are we simply beginning to uncover the incredible diversity of planets beyond our solar system?"
SciTechDaily
A: You are beginning to uncover the DESIGNED incredible diversity of planets beyond our solar system. Through faith we understand that the worlds were framed by the word of God,... Hebrews 11:3