Skip to main content

Hubble watches an extreme exoplanet being stripped by its star

Of the many strange exoplanets discovered to date, one of the most extreme has to be a world called AU Mic b. This Neptune-sized planet orbits close enough to its star that a year there lasts just over a week, and it is bombarded by dramatic flares from its host star which cook the planet with radiation.

Recently, Hubble observed this system to learn more about the relationship between the exoplanet and its star, technically called AU Microscopii.  The planet’s hydrogen atmosphere is blown away by radiation from the star, but there were confusing findings that seemed to show that no atmosphere was being lost at some times, but significant amounts of atmosphere were lost at other times.

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. NASA, ESA, Joseph Olmsted (STScI)

“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 lead researcher Keighley Rockcliffe of Dartmouth College in a statement. “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.'”

This strange variability could be due to changes in the flares given off by the star. The star is very young to host planets, at less than 100 million years old, and its flares are caused by the interaction of magnetic fields and the stellar atmosphere. This creates an extreme stellar wind effect which blows away the atmosphere of the nearby planet.

The researchers suggest that the strange variation in the planet’s atmospheric loss could be due to a particularly strong solar flare occurring shortly before Hubble took its measurements which could have ionized the hydrogen coming off the planet, making it invisible to Hubble’s instruments. Or it could be that the stellar winds do actually cause the atmospheric loss to vary considerably.

The researchers are interested in learning about how exoplanets fare in extreme radiation environments like this one.

“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.”

The research is published in The Astronomical Journal.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Hubble image shows a lonely star glowing over an irregular background galaxy
The bright star BD+17 2217. Arp 263 – also known as NGC 3239 in the foreground and irregular galaxy Arp 263 in the background.

This week's image from the Hubble Space Telescope is notable for the way it was composed as much as for the object it shows. Composed of two different exposures which have been merged, it shows the star BD+17 2217 shining over the background irregular galaxy Arp 263.

Irregular galaxies are those with irregular structures, unlike elliptical galaxies or spiral galaxies such as our Milky Way. Arp 263 is patchy and cloudy, with some areas glowing brightly due to star formation while other areas appear practically bare. Such galaxies are typically formed due to interactions with other galaxies, which can occur when a massive galaxy passes by and pulls the original galaxy out of shape. In the case of Arp 263, it is thought that it developed its irregular shape when two galaxies merged.

Read more
Hubble observes a cluster of boulders around impacted asteroid Dimorphos
A NASA/ESA Hubble Space Telescope image of the asteroid Dimorphos taken on 19 December 2022.

Last year, NASA deliberately crashed a spacecraft into an asteroid, in a first-of-its-kind test of planetary defense. At the time, telescopes around the world including the Hubble Space Telescope observed the impact between the DART spacecraft and the Dimorphos asteroid, capturing footage of the plumes of dust thrown up. Now, Hubble has observed Dimorphos once again and seen that a number of boulders have been ejected from the asteroid.

The Hubble image shown below was taken on 19 December 2022, around four months after the impact, and shows the bright streak of the asteroid across the sky, surrounded by small boulders which were knocked loose during the impact. This view was only possible after several months as the impact initially sent up large amounts of dust which made it difficult to see the asteroid in detail.

Read more
This star shredded its companion to create a stunning double-lobed nebula
A billowing pair of nearly symmetrical loops of dust and gas mark the death throes of an ancient red-giant star, as captured by Gemini South, one half of the International Gemini Observatory, operated by NSF’s NOIRLab. The resulting structure, said to resemble an old style of English jug, is a rarely seen bipolar reflection nebula. Evidence suggests that this object formed by the interactions between the dying red giant and a now-shredded companion star. The image was obtained by NOIRLab’s Communication, Education & Engagement team as part of the NOIRLab Legacy Imaging Program.

Nebulae are some of the most beautiful structures to be found in space: vast clouds of dust and gas that are illuminated by light from nearby stars. These regions are often busy sites of star formation, as new stars are born from clumps of dust that collect more material due to gravity. Within the category of nebulae, there are different types such as emission nebulae, where the gases are ionized by radiation and glow brightly, or supernova remnants, which are the structures left behind after massive stars come to the end of their lives and explode.

A recent image captured by NOIRLab's Gemini South telescope shows a rare type of nebula called a bipolar reflection nebula. Known as the Toby Jug Nebula for its similar shape to a traditional English jug, nebula IC 2220 is 1,200 light-years away in the constellation of Carina, or the Keel.

Read more