Summary
Highlights
NASA data suggests K2-18b, located 124 light-years away, could harbor life with a 99.7% probability. Chemical compounds, including dimethyl sulfide (DMS), usually associated with living organisms on Earth, have been detected in its atmosphere at concentrations a thousand times higher than on our planet. This super-Earth or mini-Neptune is believed to be a water world covered in deep oceans, potentially teeming with diverse life.
K2-18b was discovered by the Kepler Space Telescope in 2015. Subsequent observations by the Spitzer telescope in 2017 confirmed its location in the habitable zone. The HARPS spectrograph indicated the presence of an ocean. In 2019, the Hubble Space Telescope detected water vapor. The James Webb Space Telescope in 2023 detected dimethyl sulfide, a strong biosignature. Repeated measurements in 2025 using a different instrument confirmed the DMS presence, indicating a constant replenishment that on Earth is almost exclusively linked to biological activity.
K2-18b orbits a cool red dwarf star and receives similar heat and light to Earth. It's classified as a Hycean planet, covered by a deep ocean and a hydrogen-rich atmosphere. The absence of ammonia further supports the water world hypothesis. However, some scientists debate if it could be too hot for life or a miniature gas giant without a solid surface. Despite these doubts, the probability of biosignatures is 99.7%, or 3 sigma, though a higher 5 sigma confidence (99.9994%) is needed for a definitive declaration of life.
If life exists on K2-18b, it likely started with extremophile-like microorganisms thriving in its hydrogen atmosphere and high-pressure, high-temperature oceans. More complex life forms might navigate through chemical signals or bioluminescence, as vision would be limited. Given the lower density of a hydrogen atmosphere, creatures could be much larger than on Earth, potentially resembling giant jellyfish or amorphous beings adapted to immense pressure, possibly with strong, flexible exoskeletons.
Tea Garden B, just 12.5 light-years away, might have Earth-like conditions in its 'twilight zone' due to tidal locking, with moderate temperatures and liquid water. Kepler 1649C, 301 light-years away, also orbits a red dwarf and might host life in a similar twilight zone. Both planets present the challenge of extreme temperature differences between their tidally locked day and night sides.
TOI 700D, 101 light-years away, is another intriguing candidate. Unlike tidally locked planets, it may experience day and night cycles, leading to a more stable climate. It receives 86% of Earth's light, with a surface temperature around -4°C, potentially milder with a greenhouse effect. Its star is also remarkably calm, increasing the chances of a stable atmosphere and life.
J1407b, 434 light-years away, is a giant planet with an enormous ring system 200 times larger than Saturn's, spanning 120 million km. Its rings would dominate the night sky if visible from Earth, but they are expected to thin out over time as satellites form.
GJ504b, 57 light-years away, is a pink exoplanet four times Jupiter's mass. Its unusual color is due to its young age (160 million years), as it's still losing the heat of its formation, giving it a dull magenta glow.
GJ1214b is a Neptune-like exoplanet with eight times Earth's mass and an abundance of water. However, due to extreme pressure and heat (280°C), its water exists in a strange plasma form, a supercritical fluid that exhibits properties of both liquid and gas, making it unlike any water found on Earth.
Kepler 70b, 650 light-years away, is one of the hottest exoplanets known, with a temperature reaching 6,650°C, exceeding the Sun's surface temperature. Once a gas giant, it's now a dense iron core, a remnant after its star became a red giant.
WASP 76b, 640 light-years away, is a tidally locked scorching exoplanet with temperatures reaching 2350°C on its day side, causing iron to evaporate. Extreme temperature differences lead to strong winds carrying iron vapor to the colder night side, where it cools and rains molten iron.
PSRJ17191438b, a planet orbiting a dense neutron star, is a former star whose outer layers were stripped away, leaving a carbon remnant. This diamond world is about five times the size of Earth and more massive than Jupiter, orbiting its pulsar at an incredibly close distance.
WASP 107b is a peculiar 'cotton candy' exoplanet with an incredibly low density, similar in size to Jupiter but only 30 Earth masses. Its unusually small core challenges current understanding of gas giant formation.
Glee 581D, within 20 light-years of Earth, is a promising candidate for colonization due to its habitable zone location. While tidally locked, its abundant CO2 atmosphere could keep the night side from freezing. The 'twilight zone' could offer stable conditions for life.
Discovered paired with star TYC 9486-927-1, 2MASS J2126 has the largest orbital radius known, orbiting its star at a distance of a trillion km. This results in a year lasting an astonishing 900,000 Earth years.
Astronomers discovered the first clear evidence of a moon-forming disc around exoplanet PDS70C. This disc contains enough material to form three Earth-sized moons, providing a live observation of satellite formation.
The universe might contain even stranger celestial bodies, such as hypothetical planets formed from gas and dust colliding around black holes. These 'black hole planets' would orbit at vast distances, with orbital periods spanning millions of years, pushing the boundaries of our cosmic understanding.
KOI 5AB is a planet within a triple-star system. The planet orbits star A, which has a close companion star B, and a third star C orbits both. From this exoplanet, one would witness two suns, one significantly larger and brighter than the other, and a fainter third star.