World War 1 Ken Webb

[Clinio Lofton]

Aplanet relatively close to Earth could be the first ever detected with a potentially life-sustaining liquid ocean outside our Solar System, according to scientists using the James Webb space telescope.

More than 5,000 planets have been discovered outside of the Solar System so far, but only a handful are in what is called the "Goldilocks zone" -- neither too hot or too cold -- that could host liquid water, a key ingredient for life.

Lead study author Charles Cadieux, a PhD student at the University of Montreal, said that "of all currently known temperate exoplanets, LHS 1140 b could well be our best bet to one day indirectly confirm liquid water on the surface of an alien world".

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When the exoplanet LHS 1140 b was first discovered, astronomers speculated that it might be a mini-Neptune: an essentially gaseous planet, but very small in size compared to Neptune. But after analyzing data from the James Webb Space Telescope (JWST) collected in December 2023 -- combined with previous data from other space telescopes such as Spitzer, Hubble and TESS -- scientists have come to a very different conclusion.

Located some 48 light-years from Earth in the constellation Cetus, LHS 1140 b appears to be one of the most promising exoplanets in its star's habitable zone, potentially harboring an atmosphere and even an ocean of liquid water. The results of this discovery by Universit de Montral astronomers are available on ArXiv and will soon be published in The Astrophysical Journal Letters.

LHS 1140 b, an exoplanet orbiting a low-mass red dwarf star roughly one-fifth the size of the Sun, has captivated scientists due to it being one of the closest exoplanets to our Solar System that lies within its star's habitable zone. Exoplanets found in this "Goldilocks' Zone" have temperatures that would allow water to exist on them in liquid form -- liquid water being a crucial element for life as we know it on Earth.

Earlier this year, researchers led by Charles Cadieux, a Ph.D. student at UdeM's Trottier Institute for Research on Exoplanets (iREx) supervised by professor Ren Doyon, reported new mass and radius estimates for LHS 1140 b with exceptional accuracy, comparable to those of the well-known TRAPPIST-1 planets: 1.7 times the size of Earth and 5.6 times its mass.

One of the critical questions about LHS 1140 b was whether it is a mini-Neptune type exoplanet (a small gas giant with a thick hydrogen-rich atmosphere) or a super-Earth (a rocky planet larger than Earth). This latter scenario included the possibility of a so-called "Hycean world" with a global liquid ocean enveloped by a hydrogen-rich atmosphere which would exhibit a distinct atmospheric signal that could be observed using the powerful Webb Telescope.

Through an extremely competitive process, the team of astronomers obtained valuable "drector's discretionary time" (DDT) on Webb last December, during which two transits of LHS 1140 b were observed with the Canadian-built NIRISS (Near-Infrared Imager and Slitless Spectrograph) instrument. This DDT programme is only the second dedicated to the study of exoplanets in the nearly two years of Webb's operations, underscoring the importance and potential impact of these findings.

Analysis of these observations strongly excluded the mini-Neptune scenario, with tantalizing evidence suggesting exoplanet LHS 1140 b is a super-Earth that may even have a nitrogen-rich atmosphere. If this result is confirmed, LHS 1140 b would be the first temperate planet to show evidence of a secondary atmosphere, formed after the planet's initial formation.

Estimates based on all accumulated data reveal that LHS 1140 b is less dense than expected for a rocky planet with an Earth-like composition, suggesting that 10 to 20 per cent of its mass may be composed of water. This discovery points to LHS 1140 b being a compelling water world, likely resembling a snowball or ice planet with a potential liquid ocean at the sub-stellar point, the area of the planet's surface that would always be facing the system's host star due to the planet's expected synchronous rotation (much like the Earth's Moon).

"Of all currently known temperate exoplanets, LHS 1140 b could well be our best bet to one day indirectly confirm liquid water on the surface of an alien world beyond our Solar System," said Cadieux, lead author of the new study. "This would be a major milestone in the search for potentially habitable exoplanets."

While it is still only a tentative result, the presence of a nitrogen-rich atmosphere on LHS 1140 b would suggest the planet has retained a substantial atmosphere, creating conditions that might support liquid water. This discovery favors the water-world/snowball scenario as the most plausible.

Current models indicate that if LHS 1140 b has an Earth-like atmosphere, it would be a snowball planet with a vast "bull's-eye" ocean measuring about 4,000 kilometers in diameter, equivalent to half the surface area of the Atlantic Ocean. The surface temperature at the centre of this alien ocean could even be a comfortable 20 degrees Celsius.

LHS 1140 b's potential atmosphere and favorable conditions for liquid water make it an exceptional candidate for future habitability studies. This planet provides a unique opportunity to study a world that could support life, given its position in its star's habitable zone and the likelihood of its having an atmosphere that can retain heat and support a stable climate.

Confirming the presence and composition of LHS 1140 b's atmosphere and discerning between the snowball planet and bull's-eye ocean planet scenarios require further observations. The research team has emphasised the need for additional transit and eclipse measurements with the Webb Telescope, focusing on a specific signal that could unveil the presence of carbon dioxide. This feature is crucial for understanding the atmospheric composition and detecting potential greenhouse gases that could indicate habitable conditions on the exoplanet.

"Detecting an Earth-like atmosphere on a temperate planet is pushing Webb's capabilities to its limits -- it's feasible; we just need lots of observing time," said Doyon, who is also the principal investigator of the NIRISS instrument. "The current hint of a nitrogen-rich atmosphere begs for confirmation with more data. We need at least one more year of observations to confirm that LHS 1140 b has an atmosphere, and likely two or three more to detect carbon dioxide." According to Doyon, the Webb Telescope will likely have to observe this system at every possible opportunity for several years to determine whether LHS 1140 b has habitable surface conditions.

Given LHS 1140 b's limited visibility with Webb -- a maximum of only eight visits per year are possible -- astronomers will require several years of observations to detect carbon dioxide and confirm the presence of liquid water on the planet's surface.

The exoplanet, Epsilon Indi Ab, is located 12 light-years away. That's trillions of miles, but right next door, cosmically speaking. The world is somewhat like the gas giant Jupiter, but twice as massive. (For reference, "If Earth were the size of a grape, Jupiter would be about as big as a basketball," NASA notes.)

The Webb telescope, the most powerful space observatory ever built, used a coronagraph to capture the faint light from this far-off planet. A coronagraph blocks light from a specific star while capturing an image. This allows light from the nearby exoplanet to reach Webb.

In the image below, you can see Webb's coronagraph in action. "A star symbol marks the location of the host star Epsilon Indi A, whose light has been blocked by the coronagraph, resulting in the dark circle marked with a dashed white line," the space agency said. The orange object is the gas giant Epsilon Indi Ab. Only a "few tens of exoplanets" have been directly imaged before.

"Astronomers have been imagining planets in this system for decades; fictional planets orbiting Epsilon Indi have been the sites of Star Trek episodes, novels, and video games like Halo," Caroline Morley, an exoplanet researcher at the University of Texas at Austin who worked on the new study, said. "It's exciting to actually see a planet there ourselves, and begin to measure its properties."

- Infrared view: Unlike Hubble, which largely views light that's visible to us, Webb is primarily an infrared telescope, meaning it views light in the infrared spectrum. This allows us to see far more of the universe. Infrared has longer wavelengths than visible light, so the light waves more efficiently slip through cosmic clouds; the light doesn't as often collide with and get scattered by these densely packed particles. Ultimately, Webb's infrared eyesight can penetrate places Hubble can't.

Already, astronomers have successfully found intriguing chemical reactions on a planet 700 light-years away, and have started looking at one of the most anticipated places in the cosmos: the rocky, Earth-sized planets of the TRAPPIST solar system.

Mark is an award-winning journalist and the science editor at Mashable. After communicating science as a ranger with the National Park Service, he began a reporting career after seeing the extraordinary value in educating the public about the happenings in earth sciences, space, biodiversity, health, and beyond.

Previous observations of LHS 1140 b had been inconclusive. Was it a mini-Neptune with a deep hydrogen atmosphere? Or a super-Earth, a rocky world larger than Earth with a possible thinner, more Earth-like atmosphere and water? Or even a Hycean planet, with a deep global ocean and hydrogen atmosphere?

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