Science

Exoplanet orbiting nearby star 'disappears'

In 2008, NASA announced that a new exoplanet was found orbiting a star 25 light-years away. But now it seems to have vanished. It turns out that it likely wasn’t a planet at all.

What was initially thought to be a new exoplanet may have been something even more rare

Data from the NASA/ESA Hubble Space Telescope has revealed an expanding cloud of dust produced by a collision between two large bodies orbiting the bright nearby star Fomalhaut. This is the first time such a catastrophic event around another star has been imaged. (ESA/NASA, M. Kornmesser)

In 2008, NASA announced that a new exoplanet was found orbiting a star 25 light-years away. But now it seems to have vanished.

It turns out that it likely wasn't a planet at all.

The initial observation of the potential exoplanet, named Fomalhaut b, was made in 2004 using the Hubble Space Telescope, with follow-up observations in 2006.

The host star, Fomalhaut, has long fascinated astronomers. The star is found in the southern constellation Piscis Austrinus and is surrounded by a cloud of dust. Images reveal it to look like the fictional Eye of Sauron in the movie The Lord of the Rings

While most exoplanets are discovered through the transit method — when a star's light dips ever so slightly as the planet crosses in front of it — this was directly observed by Hubble. And the dot appeared to be moving, thus supporting evidence of an exoplanet.

But additional observations by Hubble in 2014 revealed ... nothing. 

This image, taken with the Advanced Camera for Surveys aboard the NASA/ESA Hubble Space Telescope, shows what was initially identified as an exoplanet orbiting the star Fomalhaut. The inset at bottom right is a composite image showing the planet's position during Hubble observations taken in 2004 and 2006. (NASA, ESA and P. Kalas [University of California, Berkeley, USA])

This exoplanet wasn't making any sense at all.

"Fomalhaut b has always been a mystery," Andras Gaspar, an astronomer at the University of Arizona and corresponding author of the new paper published in the journal Proceedings of the National Academy of Sciences, said in an email. "For starters, its colours were a bit off from what one would expect from a massive exoplanet."

But stranger still, in Hubble's initial images, the "planet" was bright in visible light but produced no heat signature in infrared light, as an object like this should. Some of the hypotheses for this was that there could be a ring of dust around Fomalhaut, or the planet was similar to Saturn and itself sported a massive ring. 

Then Gaspar and corresponding author George Rieke looked through data and realized that Fomalhaut b wasn't where it was supposed to be, which further piqued their curiosity. 

What Hubble actually witnessed

Their paper concludes that instead of an exoplanet, what Hubble witnessed was a rare collision between two large, icy asteroids that produced fine dust particles. 

Following recommendations from one of the reviewers of their paper, they went back and analyzed the object and noticed that it was expanding, further strengthening their case of an expanding cloud of dust.

Capturing something like this is rare. It just happened to be a case of Hubble looking in the right place at the right time. But it's not without precedent, Gaspar said.

"Sometimes we do get lucky and see an unlikely event," he said. "Humans have observed and noted quite a few supernovae going off over the last millenia; we have seen the Shoemaker-Levy 9 comet impact Jupiter; the massive Tunguska impact [in Siberia] in 1908 went undiscovered for years."

Illustration from the Hubble Space Telescope’s observations of Fomalhaut b’s expanding dust cloud from 2004 to 2013. (NASA, ESA, and A. Gaspar and G. Rieke [University of Arizona])

Catching something of this magnitude is important for understanding how planets and star systems form.

"The Fomalhaut system is the ultimate test lab for all of our ideas about how exoplanets and star systems evolve," Rieke, also from the University of Arizona, said in a statement. "We do have evidence of such collisions in other systems, but none of this magnitude has ever been observed. This is a blueprint for how planets destroy each other."

Rieke and Gaspar have booked time for follow-up observations on the upcoming James Webb Space Telescope, set to launch in 2021. 

"Witnessing such an event, as rare it is, is fascinating. The Earth-moon system formed in a massive collision (much more massive than this)," Gaspar said. "Collisions produce the asteroid fragments that impact Earth to this day and provide us with shooting stars to see at night, and large asteroids that movies have taught us to fear and that we are actively searching for."

ABOUT THE AUTHOR

Nicole Mortillaro

Senior Reporter, Science

Nicole has an avid interest in all things science. As an amateur astronomer, Nicole can be found looking up at the night sky appreciating the marvels of our universe. She is the editor of the Journal of the Royal Astronomical Society of Canada and the author of several books.

Comments

To encourage thoughtful and respectful conversations, first and last names will appear with each submission to CBC/Radio-Canada's online communities (except in children and youth-oriented communities). Pseudonyms will no longer be permitted.

By submitting a comment, you accept that CBC has the right to reproduce and publish that comment in whole or in part, in any manner CBC chooses. Please note that CBC does not endorse the opinions expressed in comments. Comments on this story are moderated according to our Submission Guidelines. Comments are welcome while open. We reserve the right to close comments at any time.

Become a CBC Member

Join the conversation  Create account

Already have an account?

now