K2-18b: Tracing the Possibility of Life Beyond Earth

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On April 17, an international research team published a paper in which it reported that the distant exoplanet K2-18b may be habitable.

In a significant development in space science, an international research team has reported signs that exoplanet K2-18b, located 124 light-years away from Earth in the Leo constellation, may exhibit characteristics of a habitable world.
The recent findings, based on data from the James Webb Space Telescope (JWST), suggest the presence of potential biomarkers in its atmosphere, sparking cautious optimism within the scientific community.

K2-18b is a distant exoplanet discovered in 2015 by the Kepler telescope. It is about 5.2 times wider and nine times more massive than Earth.
Orbiting its host star K2-18, the planet receives a comparable amount of stellar radiation as Earth receives from the Sun, making it a strong candidate for further habitability studies.
In 2019, NASA’s Hubble Space Telescope detected signs of water vapour in K2-18b’s atmosphere.
Later, in 2023 and 2024, the James Webb Space Telescope provided stronger evidence of carbon dioxide and methane, essential components in the quest to find life-supporting planets.

Researchers theorize that K2-18b could be a Hycean world, a type of planet enveloped by a hydrogen-rich atmosphere and potentially hosting a liquid water ocean beneath.
Computer simulations suggest that such worlds may possess moderate greenhouse conditions and even a stratosphere, despite their exotic environment.
The JWST has indicated the presence of carbon-based molecules like carbon oxides and even dimethyl sulphide (DMS) or dimethyl disulphide (DMDS).
On Earth, DMS is primarily produced by marine phytoplankton, indicating that its presence in extra-terrestrial atmospheres could point to biological activity.

The detection of DMS or DMDS is considered the most exciting outcome of the K2-18b analysis.
On Earth, DMS is almost exclusively of biological origin, released when oceanic phytoplankton decompose.
It is also produced when bacteria break down plant matter. The detection of DMS in large quantities, up to 1,000 times higher than on Earth, suggests there may be an active production source on K2-18b’s surface.
However, distinguishing between DMS and DMDS is complex due to their overlapping spectral signals.
Moreover, the possibility of non-biological sources, such as volcanic eruptions or cometary chemistry, complicates direct interpretation.

Despite these intriguing findings, the scientific community urges caution.
The JWST data have limitations, including detection thresholds and reliance on computer models that may not perfectly simulate unknown atmospheric dynamics.
There have been prior instances of premature claims in exoplanet studies.
For instance, in 2024, researchers discovered that comet 67P/Churyumov-Gerasimenko contained DMS of abiotic origin, raising the possibility that DMS may not always be a biosignature.
Additionally, a U.S.-based study suggested K2-18b could be a “mini-Neptune” with a gas-rich envelope, not necessarily requiring biological processes to explain its chemical composition.
Another reanalysis published in early 2025 challenged earlier findings, claiming there is no statistically significant evidence of carbon dioxide or DMS.

Detecting potential life-supporting conditions from vast distances relies heavily on indirect evidence.
These include signs of specific molecules, thermal conditions, and radiation levels.
However, confirmation of extraterrestrial life would require direct detection, something that current technologies like JWST cannot provide conclusively.
Hence, while K2-18b remains a promising candidate, claims of it being habitable must be tempered with scientific rigour and scepticism.

K2-18b presents a compelling case for habitability, with its hydrogen-rich atmosphere, the presence of water vapour, and signs of carbon-based molecules.
The potential detection of dimethyl sulphide lends further intrigue to this distant world.
However, with conflicting studies and technological limitations, scientists continue to investigate the data with caution.
K2-18b may or may not host life, but its study will undoubtedly enrich our understanding of planetary atmospheres and the parameters for life beyond Earth.