NASA’s planet-hunting satellite TESS (Transiting Exoplanet Survey Satellite) has been used to discover more about one of the most extreme planets ever detected, KELT-9 b, which is not only hotter on the surface than some stars but also has two summers and two winters every 36 hours.
KELT-9 b is famous for being the hottest exoplanet yet discovered, with a surface temperature of 7,800 degrees Fahrenheit (4,300 degrees Celsius). It’s so hot that the hydrogen molecules in its atmosphere are torn apart in planetwide meltdowns.
“The weirdness factor is high with KELT-9 b,” John Ahlers, an astronomer at Universities Space Research Association and NASA’s Goddard Space Flight Center said in a statement. “It’s a giant planet in a very close, nearly polar orbit around a rapidly rotating star, and these features complicate our ability to understand the star and its effects on the planet.”
One reason that the planet has such extreme features is that it is tidally locked, meaning one side of the planet always faces the sun. It is this side that becomes extremely hot, while the far side is relatively cooler, leading to strange interactions in the planet’s atmosphere as parts of it warm and cool.
Another reason the planet is strange is that its host star is unusual as well, spinning 38 times faster than the sun to complete a rotation in just 16 hours. The speed of this rotation affects the star’s shape, making it flatter at the poles and thicker around the circumference. In turn, this shape changes the temperature distribution of the star, with the poles being hotter and the equator being cooler.
When the planet passes over the star’s poles it experiences a kind of “summer” and when it passes over the cooler equator it experiences a kind of “winter.” “So KELT-9 b experiences two summers and two winters every year, with each season about nine hours,” NASA explains.
As well as being a fascinating example of an extreme planet and star system, KELT-9 can also help scientists learn about detecting other exoplanets.
“Of the planetary systems that we’ve studied via gravity darkening, the effects on KELT-9 b are by far the most spectacular,” Jason Barnes, a professor of physics at the University of Idaho and a co-author of the paper, said in the statement. “This work goes a long way toward unifying gravity darkening with other techniques that measure planetary alignment, which in the end we hope will tease out secrets about the formation and evolutionary history of planets around high-mass stars.”
The findings are published in the Astronomical Journal.
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