Skip to main content
  1. Home
  2. Space
  3. News

James Webb telescope searches for habitability in the famous TRAPPIST-1 system

By

Of all the planets we’ve discovered beyond our solar system, the majority are not Earth-like at all. They are most often gas giants like Jupiter that orbit very close to their stars, making them extremely hot. These are also generally the easiest type of exoplanet to detect. Very few of the thousands of discovered exoplanets could be potentially habitable — fewer than 50 in total. That’s why astronomers were so excited by the finding in 2017 of a system called TRAPPIST-1, which has seven rocky Earth-sized exoplanets, four of which are in the habitable zone.

But TRAPPIST-1 is a long way away, at 40 light-years’ distance, so it isn’t easy to see these planets in detail. Astronomers had some information about the planets’ sizes and orbits, but to really know if life could ever have emerged there, they needed information on the planets’ atmospheres. And the James Webb Space Telescope provided the means to investigate that.

This artist’s concept portrays the seven rocky exoplanets within the TRAPPIST-1 system, located 40 light-years from Earth. NASA/JPL-Caltech/R. Hurt (IPAC)

“We want to know if rocky planets have atmospheres or not,” said Sebastian Zieba, lead author of Webb’s research into the TRAPPIST-1 system, in a statement. “In the past, we could only really study planets with thick, hydrogen-rich atmospheres. With Webb, we can finally start to search for atmospheres dominated by oxygen, nitrogen, and carbon dioxide.”

Recommended Videos

The recent study looked at TRAPPIST-1 c, which was thought to be a Venus-like planet that was tidally locked to its star — so one side, the dayside, would always be facing the star and would have a temperature of about 225 degrees Fahrenheit. “TRAPPIST-1 c is interesting because it’s basically a Venus twin: It’s about the same size as Venus and receives a similar amount of radiation from its host star as Venus gets from the sun,” explained co-author Laura Kreidberg. “We thought it could have a thick carbon dioxide atmosphere like Venus.”

This artist' concept shows what the hot rocky exoplanet TRAPPIST-1 c could look like based on this work. TRAPPIST-1 c, the second of seven known planets in the TRAPPIST-1 system, orbits its star at a distance of 0.016 AU (about 1.5 million miles), completing one circuit in just 2.42 Earth-days. TRAPPIST-1 c is slightly larger than Earth, but has around the same density, which indicates that it must have a rocky composition. Webb’s measurement of 15-micron mid-infrared light emitted by TRAPPIST-1 c suggests that the planet has either a bare rocky surface or a very thin carbon dioxide atmosphere.
This artist’s concept shows what the hot, rocky exoplanet TRAPPIST-1 c could look like. Webb’s measurement of 15-micron mid-infrared light emitted by TRAPPIST-1 c suggests that the planet has either a bare rocky surface or a very thin carbon dioxide atmosphere. NASA, ESA, CSA, Joseph Olmsted (STScI)

However, when the researchers used Webb to observe TRAPPIST-1 c’s atmosphere, they found it was very different from Venus’s thick, carbon dioxide-rich atmosphere. Instead, the planet has an extremely thin atmosphere — if it has an atmosphere at all.

Related

The results are something of a disappointment for those hoping to find habitability, as it means that the planet probably formed without much water. And it’s possible that the other planets in the system could have formed without water too, making it less likely that they could be habitable.

Even though the results are not what was expected, they are still an exciting demonstration of how technology has developed to allow us to see exoplanet atmospheres. “It is extraordinary that we can measure this,” said Kreidberg. “There have been questions for decades now about whether rocky planets can keep atmospheres. Webb’s ability really brings us into a regime where we can start to compare exoplanet systems to our solar system in a way that we never have before.”

The research is published in the journal Nature.

Editors' Recommendations

Topics
Georgina Torbet
Georgina Torbet
Space Writer
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
One galaxy, two views: see a comparison of images from Hubble and Webb
The peculiar galaxy NGC 3256 takes centre stage in this image from the NASA/ESA Hubble Space Telescope. This distorted galaxy is the wreckage of a head-on collision between two spiral galaxies which likely occurred 500 million years ago, and it is studded with clumps of young stars which were formed as gas and dust from the two galaxies collided.

It might not seem obvious why astronomers need multiple different powerful space telescopes. Surely a more powerful telescope is better than a less powerful one? So why are there multiple different telescopes in orbit, either around Earth or around the sun?

The answer is to do with two main factors. One is the telescope's field of view, meaning how much of the sky it looks at. Some telescopes are useful for looking at large areas of the sky in less detail, working as survey telescopes to identify objects for further research or to look at the universe on a large scale -- like the recently launched Euclid mission. While others, like the Hubble Space Telescope, look at small areas of the sky in great detail, which is useful for studying particular objects.

Read more
James Webb spots the most distant active supermassive black hole ever discovered
Crop of Webb's CEERS Survey image.

As well as observing specific objects like distant galaxies and planets here in our solar system, the James Webb Space Telescope is also being used to perform wide-scale surveys of parts of the sky. These surveys observe large chunks of the sky to identify important targets like very distant, very early galaxies, as well as observe intriguing objects like black holes. And one such survey has recently identified the most distant active supermassive black hole seen so far.

While a typical black hole might have a mass up to around 10 times that of the sun, supermassive black holes are much more massive, with a mass that can be millions or even billions of times the mass of the sun. These monsters are found at the heart of galaxies and are thought to play important roles in the formation and merging of galaxies.

Read more
Saturn as you’ve never seen it before, captured by Webb telescope
Saturn captured by the James Webb Space Telescope

NASA has shared a gorgeous image of Saturn captured recently by the James Webb Space Telescope (JWST).

Webb’s first near-infrared observations of the second largest planet in our solar system also show several of Saturn’s moons: Dione, Enceladus, and Tethys.

Read more