Skip to main content

New type of ocean-covered ‘Hycean’ exoplanet could support life

When it comes to looking for life elsewhere in the universe, we tend to be very Earth-centric: We look for planets that are similar to our own, assuming that life elsewhere will be similar to us and require similar conditions. However, a new type of exoplanet has been identified by astronomers at the University of Cambridge, and even though it is very different from Earth it could still support life.

The new class of planet is called a “Hycean” planet, meaning an ocean-covered world with abundant hydrogen in its atmosphere. The researchers believe that this type of planet could be common and as they are potentially habitable this significantly increases the possible locations to search for life outside our solar system.

 Artist's impression of a Hycean planet.
Artist’s impression of a Hycean planet. Amanda Smith

“Hycean planets open a whole new avenue in our search for life elsewhere,” said lead researcher Nikku Madhusudhan from the University of Cambridge’s Institute of Astronomy in a statement.

These planets are typically larger than Earth, at up to 2.6 times its size, and can be hotter as well, with atmospheric temperatures of up to 200 degrees Celsius. However, despite these high temperatures their oceans could still host microbial life, as suggested by another recent study into a large exoplanet with a hydrogen-rich atmosphere. This study found that there could be liquid water on the planet’s surface beneath its atmosphere. If this is true for Hycean planets as well, then the habitable zone — the area around a star where a planet must orbit for liquid water to be able to exist on its surface — could be larger for these planets than for other types of planets.

“Essentially, when we’ve been looking for these various molecular signatures, we have been focusing on planets similar to Earth, which is a reasonable place to start,” said Madhusudhan. “But we think Hycean planets offer a better chance of finding several trace biosignatures.”

Biosignatures are chemical indications of life and are one of the main ways that researchers look for life elsewhere in the universe.

“A biosignature detection would transform our understanding of life in the universe,” said Madhusudhan. “We need to be open about where we expect to find life and what form that life could take, as nature continues to surprise us in often unimaginable ways.”

The research is published in The Astrophysical Journal.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
See planets being born in new images from the Very Large Telescope
This composite image shows the MWC 758 planet-forming disc, located about 500 light-years away in the Taurus region, as seen with two different facilities. The yellow colour represents infrared observations obtained with the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument on ESO’s Very Large Telescope (VLT). The blue regions on the other hand correspond to observations performed with the Atacama Large Millimeter/submillimeter Array (ALMA).

Astronomers have used the Very Large Telescope to peer into the disks of matter from which exoplanets form, looking at more than 80 young stars to see which may have planets forming around them. This is the largest study to date on these planet-forming disks, which are often found within the same huge clouds of dust and gas that stars form within.

A total of 86 young stars were studied in three regions known to host star formation: Taurus and Chamaeleon I, each located around 600 light-years away, and Orion, a famous stellar nursery located around 1,600 light-years away. The researchers took images of the disks around the stars, looking at their structures for clues about how different types of planets can form.

Read more
James Webb photographs two potential exoplanets orbiting white dwarfs
Illustration of a cloudy exoplanet and a disk of debris orbiting a white dwarf star.

Even though scientists have now discovered more than 5,000 exoplanets, or planets outside our solar system, it's a rare thing that any telescope can take an image of one of these planets. That's because they are so small and dim compared to the stars that they orbit around that it's easier to detect their presence based on their effects on the star rather than them being detected directly.

However, thanks to its exceptional sensitivity, the James Webb Space Telescope was recently able to image two potential exoplanets orbiting around small, cold cores of dead stars called white dwarfs directly.

Read more
Small exoplanet could be hot and steamy according to Hubble
This is an artist’s conception of the exoplanet GJ 9827d, the smallest exoplanet where water vapour has been detected in its atmosphere. The planet could be an example of potential planets with water-rich atmospheres elsewhere in our galaxy. It is a rocky world, only about twice Earth’s diameter. It orbits the red dwarf star GJ 9827. Two inner planets in the system are on the left. The background stars are plotted as they would be seen to the unaided eye looking back toward our Sun, which itself is too faint to be seen. The blue star at upper right is Regulus, the yellow star at bottom centre is Denebola, and the blue star at bottom right is Spica. The constellation Leo is on the left, and Virgo is on the right. Both constellations are distorted from our Earth-bound view from 97 light-years away.

One of the big topics in exoplanet research right now is not just finding exoplanets but also looking at their atmospheres. Tools like the James Webb Space Telescope are designed to allow researchers to look at the light coming from distant stars and see how it is filtered as it passes by exoplanets, allowing them to learn about the composition of their atmospheres. But scientists are also using older telescopes like the Hubble Space Telescope for similar research -- and Hubble recently identified water vapor in an exoplanet atmosphere.

“This would be the first time that we can directly show through an atmospheric detection that these planets with water-rich atmospheres can actually exist around other stars,” said researcher Björn Benneke of the Université de Montréal in a statement. “This is an important step toward determining the prevalence and diversity of atmospheres on rocky planets."

Read more