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A WATERY 'super-Earth' roughly 50 light-years away may bear the conditions to host life.

LHS 1140 b is an exoplanet orbiting a red dwarf star in the constellation Cetus. It falls in the star's habitable zone, or the region with temperatures that can support liquid water.

LHS 1140 b, an exoplanet roughly twice the size of Earth, could hold the key to life in its temperate ocean and nitrogen-rich atmosphere
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LHS 1140 b, an exoplanet roughly twice the size of Earth, could hold the key to life in its temperate ocean and nitrogen-rich atmosphereCredit: B. Gougeon/Université de Montréal

Now, a team of scientists has determined the planet may harbor an atmosphere and an ocean similar to those on Earth.

A paper published this week in identified LHS 1140 b as one of the most promising candidates with the conditions to support life.

“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,” lead author Charles Cadieux said in a statement.

“This would be a major milestone in the search for potentially habitable exoplanets.”

The team, led by researchers from the Université de Montréal, examined data collected by Nasa's James Webb Space Telescope.

It was added to earlier data from other telescopes including Spitzer and Hubble.

In their analysis, the scientists ruled out the possibility that LHS 1140 was a mini-Neptune with a hydrogen-rich atmosphere.

Rather, they found evidence that it is, in fact, a super-Earth - a rocky or watery planet with a radius roughly twice that of Earth's.

Further analysis found reason to believe the exoplanet may have a nitrogen-rich atmosphere, similar to our home planet.

“This is the first time we have ever seen a hint of an atmosphere on a habitable zone rocky or ice-rich exoplanet," said Ryan MacDonald, Nasa Sagan Fellow in the U-M Department of Astronomy.

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“LHS 1140 b is one of the best small exoplanets in the habitable zone capable of supporting a thick atmosphere, and we might just have found evidence of air on this world.”

These findings suggest the planet has retained a substantial atmosphere and may accommodate liquid water.

And the scientists made another discovery that further supports the ocean theory.

Scientists examined data from Nasa's James Webb Space Telescope and determined the planet may be an icy "water world" with a bullseye-like ocean
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Scientists examined data from Nasa's James Webb Space Telescope and determined the planet may be an icy "water world" with a bullseye-like oceanCredit: Getty

LHS 1140 b is less dense than expected for an Earth-like planet, indicating a large fraction of its mass may be held in water.

This indicates LHS 1140 b is, in fact, a water world, likely resembling a snowball with an ocean pointing at the red dwarf like a bullseye.

Current models indicate that LHS 1140 b could bear an ocean roughly 4,000 kilometers in diameter, equivalent to half the surface area of the Atlantic Ocean.

The surface temperature could be a mild 20 degrees Celsius, or 68 degrees Fahrenheit.

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What is an exoplanet?

Here's what you need to know...

  • An exoplanet is a planet that is located outside of our solar system and is orbiting its own star, like how Earth orbits the Sun
  • They are very hard to see with telescopes because they are often hidden by the brightness of their star
  • Nasa sent the Kepler space telescope into orbit to find Earth-sized exoplanets that might support life
  • Over 5,500 exoplanets have been discovered so far, and more missions to find even more exoplanets are planned
  • A good way to spot an exoplanet is to look for wobbly stars, because a disruption to starlight can indicate that a planet is orbiting it and therefore blocking out light on occasion
  • Exoplanets are very common in the universe, and the more we find that look like Earth, the closer we get to knowing whether we're alone out there

“Our initial reconnaissance of LHS 1140 b with JWST has revealed this to be perhaps the best habitable zone exoplanet currently known for atmospheric characterization," MacDonald said.

"While we need more JWST observations to confirm the nitrogen-rich atmosphere, and to search for other gases, this is a very promising start.”

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