The strongest evidence of life on an exoplanet has been found by scientists.
A planet orbiting a red dwarf star with a liquid water ocean beneath a hydrogen-rich atmosphere. This category may be a fit for the exoplanet K2-18 b based on observations made by the James Webb Space Telescope.

Scientists have obtained using the the James Webb Space Telescope that they call the strongest signs yet of possible life beyond our solar system, detecting in an exoplanet’s atmosphere the chemical fingerprints of gases that on Earth are produced only by biological processes. Two gases are observed in the planet named K2-18 b are dimethyl sulfide or DMS, and dimethyl disulfide or DMDS - which are generated on Earth by living organisms, primarily microbial life such as marine phytoplankton algae.
K2-18 b is 8.6 times as massive as Earth and has a diameter about 2.6 times as large as our planet.
It orbits in the “habitable zone” - a distance where liquid water, a key ingredient for life, can exist on a planetary surface - around a red dwarf star smaller and less luminous than our sun, located about 124 light-years from Earth in the constellation Leo. A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). One other planet also has been identified orbiting this star.
K2-18 b is part of the “sub-Neptune” class of planets, with a diameter greater than Earth’s but less than that of Neptune, our solar system’s smallest gas planet.
To ascertain the chemical composition of an exoplanet’s atmosphere, astronomers analyze the light from its host star as the planet passes in front of it from the perspective of Earth, called the transit method. As the planet transits, Webb can detect a decrease in stellar brightness, and a small fraction of starlight passes through the planetary atmosphere before being detected by the telescope. This lets scientists determine the constituent gases of the planet’s atmosphere.
How reliable are the findings?
The scientists published their findings in the peer-reviewed Astrophysical Journal Letters publication, which means that other experts in the field who studied their paper found it convincing.
But that does not mean that the scientists have found irrefutable evidence of life. Far from it.
Scientist Madhusudhan acknowledged that it is possible that the traces of DMS and DMDS found in the atmosphere of K2-18b are the outcome of chemical phenomena that are as of now, unknown to humanity.
Is there other evidence of extraterrestrial life?
The findings of the Cambridge-led team follow a series of breakthroughs in recent years that have excited scientists about the possibilities of finding life beyond Earth.
In 2011, NASA scientists announced that they had found chemicals that are components of DNA on meteorites that had landed in Antarctica. The chemical traces they had discovered couldn’t have been the result of contamination after the meteorites landed on Earth. The only explanation – that asteroids and comets could contain the building blocks of life. A year later, astronomers at Copenhagen University tracked down a sugar molecule in a distant star system. That molecule is an essential component of ribonucleic acid or RNA, a molecule that is critical for most biological functions. In 2023, astronomers found traces of organic molecules in the gases around one of Saturn’s moons, Enceladus. In mid-2024, scientists identified five greenhouse gases that they said would be telltale signs of life on any other planet.
About the Creator
Preyonjit Chakraborty
My heartiest gratitude to all. I am a writer and musician. Basically I write on aero-science, art, content, spirituality and history related topics. I want to be a great writer. I will try to make people pleased with my writing qualities.


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