Science

Jupiter-like planet more massive than first thought, according to new space telescope images

Astronomers have directly imaged a 'cold' gas giant planet that is just 12 light-years from Earth and is more massive than previously believed.

Data has led to new information about this previously discovered body

In the foreground to the left is a sphere half illuminated on the right side, almost filling the image vertically. The surface consists of several parallel, pale-coloured bands aligned horizontally. To the top right is a much smaller orange, circular light source, illuminating the large sphere in the foreground. The background is black with numerous tiny white dots.
Artist’s impression of a cold gas giant orbiting a red dwarf. Only a point of light is visible on the images captured by the James Webb Space Telescope. Nevertheless, the initial analysis suggests the presence of a gaseous planet that may have properties similar to Jupiter. (T. Müller (MPIA/HdA))

Astronomers using the James Webb Space Telescope (JWST) have imaged a planet that is, relatively speaking, in our galactic backyard — and that fresh data has led to new details about this massive "cold" Jupiter.

The gas giant exoplanet has the unceremonious name of Epsilon Ind Ab. Epsilon (or "Eps") is the fifth letter in the Greek alphabet or — in this case — the fifth-brightest star in the constellation Indus, which is where the "Ind" comes from. "A" is the star, and "b" denotes the planet.

Eps Ind Ab (sometimes referred to as Eps Indi Ab) orbits in a three-body system. But hold on: it's not like the best-selling book and the hit Netflix series 3 Body Problem: two are very close brown dwarfs — bodies that lie somewhere between planets and stars and are often referred to as failed stars — while the other is a red dwarf star.

While the main star lies two billion kilometres away from the planet, the two brown dwarfs are more than 224 billion kilometres away, or about more than 40 times farther than Pluto is from Earth.

The planet was known — but not well

This planet was known to astronomers, but as the researchers write in their new study, published Wednesday in the journal Nature, a lot of information about Eps Ind Ab was incorrect.

With no ground-based images, however, astronomers had little to go on.

But with the incredible "eyes" of JWST, a group of astronomers from around the world were able to finally see this massive Jupiter-like planet. And while it may be just a bright dot in a photograph, that white dot contains a lot of information. 

A photograph with a black background and a symbol of a star with a bright point of light to the lower left.
This image of the gas-giant exoplanet Epsilon Ind Ab was taken with the coronagraph on NASA’s James Webb Space Telescope’s MIRI (mid-infrared instrument). A star symbol marks the location of the host star Epsilon Ind A, whose light has been blocked by the coronagraph, resulting in the dark circle marked with a dashed white line. Eps Ind Ab is one of the coldest exoplanets ever directly imaged. (NASA, ESA, CSA, STScI, E. Matthews [Max Planck Institute for Astronomy])

When astronomers first looked at the JWST photograph of Eps Ind Ab, they immediately knew something was wrong: It wasn't where it was supposed to be.

"We looked at it and did all the measurements, like rotated it so that it's aligned to the north and everything like that. And we're like, 'Wait a minute, it's in completely the wrong place,'" said lead author of the paper, Elisabeth Matthews of the Max Planck Institute for Astronomy in Germany.

"So then we had to do all of this work to confirm that it really was a planet and not a background galaxy."

JWST a 'wild horse'

Using the JWST data, they made some more discoveries.

Initial data from the ground suggested the planet was 3.25 times the mass of Jupiter. With data from the new images, they found that it was six times Jupiter's mass. In astronomy, references to mass relate to the weight of a particular body. 

As well, they learned that the planet orbits the star every 200 years, instead of every 45.2 years.   

Scientists were also able to measure its temperature, estimated at roughly 0 C. That's considered quite cold when it comes to exoplanet discoveries.

WATCH | Animation of Esp Ind Ab: 

This is particularly exciting for astronomers studying exoplanets. Most of the ones that have been discovered are young and hot, still radiating much of the energy from their formation.

Detecting cooler, older ones is more difficult.

"We're fairly good at detecting planets, especially with the transit and the radial velocity measurement, but then characterizing their atmospheres as much harder," Matthews said.

"So this is kind of opening up that new parameter space. It's allowing us to actually characterize a cold atmosphere for the first time. And then I think — like really long-term — we also want to be able to push toward characterizing cold but much smaller planets, so things more like the Earth."

The planet was initially found through a process called radial velocity, where a star wobbles slightly due to the tug of a nearby planet, but it had never before been imaged. Most exoplanets are discovered using the transit method where there is a slight dip in a star's brightness as a planet passes in front of it. 

Paul Delaney, an astronomer and professor emeritus at York University's department of physics and astronomy in Toronto, said it's a great illustration of JWST's capabilities.

An image of a starry background that shows two separate images in separate boxes: On the left is a blue one that shows an illustration of a star at centre with a bright white dot at the top left. On the right is a red image that also shows the star and the white dot, but with markings indicating one is an actual star and the white dot is a planet.
An image of Eps Ind Ab. The inserts show cropped versions of the images obtained at mid-infrared wavelengths. A coronagraph blocks the light from the star that would outshine both images. Instead, a new object becomes visible to the top left. (T. Müller [MPIA/HdA], E. Matthews [MPIA])

"It's a finely tuned telescope, and it is producing data that is of such a high quality, that it's making headlines," said Delaney, who was not involved in the study.

"Everybody is always sort of hanging now on James Webb's next observation. I think it's great for astronomy."

Delaney said in just two years, the amount of data collected by the telescope has already outpaced what was gathered by its predecessor, the Hubble Space Telescope, which was launched in 1990. 

"It's like a wild horse. It's just running away furiously."

And while JWST may not be used for detecting planets — its focus will be to study already-discovered ones to get more information on these distant worlds — it's helping astronomers better understand how planets like our own form.

Matthews said scientists will be further studying Eps Ind Ab to determine its atmosphere. 

"I still find it kind of incredible that we have such a big planet so close to us. It's just a little less than 12 light-years away. So it's like right there," said Matthews.

"It's really accessible to study in more detail. And it's a really strange planet, honestly, but I think a really exciting planet that will hopefully be able to use to learn a lot more physics as well."

Corrections

  • A previous version of this story included a headline that stated the planet was bigger than previously thought. In fact, it was more massive than previously thought.
    Jul 24, 2024 5:25 PM ET

ABOUT THE AUTHOR

Nicole Mortillaro

Senior Science Reporter

Based in Toronto, Nicole covers all things science for CBC News. 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. In 2021, she won the Kavli Science Journalism Award from the American Association for the Advancement of Science for a Quirks and Quarks audio special on the history and future of Black people in science. You can send her story ideas at [email protected].