A potential ocean world may lie beyond our solar system

In short Simplifying... In short LHS 1140 b, once thought to be a mini-Neptune, is now seen as a rocky "super-Earth" with potential for large quantities of water, possibly making it an ocean world.

While its atmosphere is yet to be confirmed, signs of gases like CO2 and nitrogen hint at the possibility of liquid water and life.

Researchers are planning further studies with the Webb telescope to understand this intriguing exoplanet better. Was a long read? Making it simpler... Next Article Next Article

The planet was discovered in 2017

A potential ocean world may lie beyond our solar system

By Dwaipayan Roy 10:07 am Jul 14, 202410:07 am

What's the story Scientists using the James Webb Space Telescope have identified a potential ocean world, LHS 1140 b, located relatively close to Earth. This exoplanet is one of the few discovered in the "Goldilocks zone," an area neither too hot nor too cold for liquid water, a crucial component for life. Since its discovery in 2017, LHS 1140 b has been under intense scrutiny due to its potential to host life-sustaining liquid water.

Planetary evolution

From mini-Neptune to super-Earth

Initially, LHS 1140 b was believed to be a mini-Neptune, a small gas giant with an atmosphere too dense with hydrogen and helium, to support life. However, recent observations from the Webb telescope have revealed it as a rocky "super-Earth," 1.7 times larger and 5.6 times heavier than our planet. The absence of hydrogen or helium in its atmosphere has ruled out the possibility of it being a mini-Neptune.

Water presence

A potential water world

According to Martin Turbet of France's CNRS scientific research center, the density of LHS 1140 b suggests it "actually has large quantities of water." Unlike Earth, where oceans represent only 0.02% of its mass, an estimated 10 to 20% of LHS 1140 b's mass is believed to be water. The state of this water—liquid or ice—depends on the planet's atmosphere.

Exoplanet atmosphere

The best bet for alien liquid water

While there is no direct evidence of an atmosphere, several elements suggest its existence, according to Turbet. Lead study author Charles Cadieux from the University of Montreal, stated, "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." The presence of gases like CO2 will play an important role in determining whether the planet is covered in ice or water.

Surface exploration

LHS 1140 b's possible surface conditions

The surface of LHS 1140 b could be mostly ice with a vast liquid ocean, where the planet is most exposed to its star's heat, or the liquid water might be hidden under a thick shell of ice. Cadieux noted signs suggesting "the presence of nitrogen," another potential ingredient for life, but emphasized that more research is needed. The researchers plan to secure more time with the Webb telescope to further study LHS 1140 b.

Research timeline

Future research: Confirming atmosphere and detecting CO2

The researchers estimate that it will take at least a year to confirm whether LHS 1140 b has an atmosphere. Following this, they anticipate needing two or three more years to detect the presence of CO2. This timeline underscores the complexity of studying exoplanets. and the meticulous work required to understand their potential for hosting life.