Hubble sees evaporating planet getting the hiccups

Jul 27, 2023 (Nanowerk News) A young planet whirling around a petulant red dwarf star is changing in unpredictable ways orbit-by-orbit. It is so close to its parent star that it experiences a consistent, torrential blast of energy, which evaporates its hydrogen atmosphere — causing it to puff off the planet. But during one orbit observed with the Hubble Space Telescope, the planet looked like it wasn’t losing any material at all, while an orbit observed with Hubble a year and a half later showed clear signs of atmospheric loss. This artist's illustration shows a planet (dark silhouette) passing in front of the red dwarf star AU Microscopii This artist’s illustration shows a planet (dark silhouette) passing in front of the red dwarf star AU Microscopii. The planet is so close to the eruptive star a ferocious blast of stellar wind and blistering ultraviolet radiation is heating the planet’s hydrogen atmosphere, causing it to escape into space. Four times Earth’s diameter, the planet is slowly evaporating its atmosphere, which stretches out linearly along its orbital path. This process may eventually leave behind a rocky core. The illustration is based on measurements made by the Hubble Space Telescope. (Image: NASA, ESA, Joseph Olmsted (STScI)) This extreme variability between orbits shocked astronomers. “We’ve never seen atmospheric escape go from completely not detectable to very detectable over such a short period when a planet passes in front of its star,” said Keighley Rockcliffe of Dartmouth College in Hanover, New Hampshire. “We were really expecting something very predictable, repeatable. But it turned out to be weird. When I first saw this, I thought ‘That can’t be right.'” Rockcliffe was equally puzzled to see, when it was detectable, the planet’s atmosphere puffing out in front of the planet, like a headlight on a fast-bound train. “This frankly strange observation is kind of a stress-test case for the modeling and the physics about planetary evolution. This observation is so cool because we’re getting to probe this interplay between the star and the planet that is really at the most extreme,” she said. Located 32 light-years from Earth, the parent star AU Microscopii (AU Mic) hosts one of the youngest planetary systems ever observed. The star is less than 100 million years old (a tiny fraction of the age of our Sun, which is 4.6 billion years old). The innermost planet, AU Mic b, has an orbital period of 8.46 days and is just 6 million miles from the star (about 1/10th the planet Mercury’s distance from our Sun). The bloated, gaseous world is about four times Earth’s diameter. AU Mic b was discovered by NASA’s Spitzer and TESS (Transiting Exoplanet Survey Satellite) space telescopes in 2020. It was spotted with the transit method, meaning telescopes can observe a slight dip in the star’s brightness when the planet crosses in front of it. Red dwarfs like AU Microscopii are the most abundant stars in our Milky Way galaxy. They therefore should host the majority of planets in our galaxy. But can planets orbiting red dwarf stars like AU Mic b be hospitable to life? A key challenge is that young red dwarfs have ferocious stellar flares blasting out withering radiation. This period of high activity lasts a lot longer than that of stars like our Sun. The flares are powered by intense magnetic fields that get tangled by the roiling motions of the stellar atmosphere. When the tangling gets too intense, the fields break and reconnect, unleashing tremendous amounts of energy that are 100 to 1,000 times more energetic than our Sun unleashes in its outbursts. It’s a blistering fireworks show of torrential winds, flares, and X-rays blasting any planets orbiting close to the star. “This creates a really unconstrained and frankly, scary, stellar wind environment that’s impacting the planet’s atmosphere,” said Rockcliffe. Under these torrid conditions, planets forming within the first 100 million years of the star’s birth should experience the most amount of atmospheric escape. This might end up completely stripping a planet of its atmosphere. “We want to find out what kinds of planets can survive these environments. What will they finally look like when the star settles down? And would there be any chance of habitability eventually, or will they wind up just being scorched planets?” said Rockcliffe. “Do they eventually lose most of their atmospheres and their surviving cores become super-Earths? We don’t really know what those final compositions look like because we don’t have anything like that in our solar system.” While the star’s glare prevents Hubble from directly seeing the planet, the telescope can measure changes in the star’s apparent brightness caused by hydrogen bleeding off the planet and dimming the starlight when the planet transits the star. That atmospheric hydrogen has been heated to the point where it escapes the planet’s gravity. The never-before-seen changes in atmospheric outflow from AU Mic b may indicate swift and extreme variability in the host red dwarf’s outbursts. There is so much variability because the star has a lot of roiling magnetic field lines. One possible explanation for the missing hydrogen during one of the planet’s transits is that a powerful stellar flare, seen seven hours prior, may have photoionized the escaping hydrogen to the point where it became transparent to light, and so was not detectable. Another explanation is that the stellar wind itself is shaping the planetary outflow, making it observable at some times and not observable at other times, even causing some of the outflow to “hiccup” ahead of the planet itself. This is predicted in some models, like those of John McCann and Ruth Murray-Clay from the University of California at Santa Cruz, but this is the first kind of observational evidence of it happening and to such an extreme degree, say researchers. Hubble follow-up observations of more AU Mic b transits should offer additional clues to the star and planet’s odd variability, further testing scientific models of exoplanetary atmospheric escape and evolution. Rockcliffe is lead author on the science paper published in The Astronomical Journal (“The Variable Detection of Atmospheric Escape around the Young, Hot Neptune AU Mic b”).