Astronomers have documented a bizarre cycle of molecular destruction and rebirth on an ultra-hot, Jupiter-like exoplanet where surface temperatures exceed 7,750 degrees Fahrenheit.
Originally discovered in 2017, KELT-9b has the dubious distinction of being the hottest known exoplanet in the galaxy. This ultra-hot planet is located 670 light-years from Earth, is around 2.8 times more massive than Jupiter, and requires just 1.5 days to complete a single rotation of its host star.
KELT-9b is tidally locked, which means it has a side that perpetually faces its host star, similar to how our Moon’s near side always faces Earth. New research published in The Astrophysical Journal Letters presents evidence showing that hydrogen molecules on KELT-9b’s star-facing side are disintegrating because of the extreme heat. The ensuing bits of busted hydrogen are eventually transported to the exoplanet’s cooler side, where they reform and flow back to the hot side, and the cycle repeats itself, according to the research.
Megan Mansfield, a graduate student from the University of Chicago and the lead author of the new study, said these observations are in agreement with recent theories attempting to explain these ultra-hot exoplanets.
“These recent theories suggested that these hot planets should have hydrogen dissociation occurring—where hydrogen molecules are ripped into individual atoms on the hot dayside of the planet and then combine back into hydrogen molecules on the cooler nightside,” explained Mansfield in an email to Gizmodo. “So far, however, we’ve looked at planets that are colder than KELT-9b, so while this effect might have been happening it wasn’t as clear from the observations whether it was definitely needed.”
For KELT-9b, the planet is so hot that this breaking and reforming of hydrogen molecules is the best explanation for what the scientists observed—an exciting observation “because it suggests our models are incorporating an important piece of physics for these ultra-hot planets,” said Mansfield.
The new paper also confirms KELT-9b as being the hottest known exoplanet in the galaxy. Temperatures on the exoplanet’s dayside can reach 4,566 Kelvin (4,293 degrees Celsius, 7,759 degrees Fahrenheit), while the cooler dark side is around 2,556 Kelvin (2,283 degrees Celsius, 4,141 degrees Fahrenheit).
To map these temperatures, Mansfield and her colleagues used NASA’s soon-to-be-retired Spitzer Space Telescope, which uses infrared light to detect the tiniest heat fluctuations in distant objects. Spitzer data allowed the team to create a temperature profile of KELT-9b, which was observed with the transit method (when a distant exoplanet passes in front of its host star from our perspective on Earth).
Multiple observations of KELT-9b revealed temperatures on both halves of the planet as it rolled into view. Interestingly, the scientists noticed that differences in the temperature between the dayside and nightside weren’t as large as expected, pointing to some kind of atmospheric exchange, or heat flow, between the two sides.
To understand how atmospheric gases and heat flowed around the exoplanet, the researchers turned to computer models. This allowed Mansfield and her team to observe atmospheric behavior under different conditions. Ultimately, the best model involved the disintegration and reformation of the hydrogen molecules, or the “dissociation and recombination,” as the scientists described the phenomenon.
“This is the first time that this enhanced heat transport has been observed so clearly on a super hot object like this,” explained Mansfield. “This means ultra-hot Jupiters are different than we used to think. Before we thought that ultra-hot Jupiters would all have relatively little heat transport, but the observations of KELT-9b suggest that ultra-hot Jupiters are transporting much more heat than we previously thought.”
This latest study reminds us of a similar exoplanet, WASP 121b. But instead of shredding its hydrogen, this hot Jupiter is shredding its water.
Indeed, while KELT-9b represents an extreme case, the researchers have reason to believe this process could be happening elsewhere, even on slightly cooler exoplanets.
“This kind of planet is so extreme in temperature, it is a bit separate from a lot of other exoplanets,” said Mansfield in a NASA press release. “There are some other hot Jupiters and ultra-hot Jupiters that are not quite as hot but still warm enough that this effect should be taking place.”
Weirdly, KELT-9b’s hottest point did not appear to be static; it shifted slightly across the orb. Writing in their paper, the scientists said they don’t fully understand why this is happening, but that “magnetic effects in the planet’s highly ionized atmosphere,” could be the reason. Future research will be required to fully figure out what’s going on.
This article has been updated to include comments from Megan Mansfield.