Skip to main content

Intriguing exoplanet could be entirely covered in ocean

Astronomers have discovered an intriguing exoplanet that could be entirely covered in water. The potential ocean world is called TOI-1452 b, located around 100 light-years away in the constellation of Draco.

The planet was discovered by an international team using data from NASA’s Transiting Exoplanet Survey Satellite, or TESS, and is a type of planet called a super-Earth which is somewhat larger and heavier than Earth. It is in its host star’s habitable zone, meaning it is the right distance from the star for liquid water to exist on its surface.

Artistic rendition of the exoplanet TOI-1452 b, a small planet that may be entirely covered in a deep ocean.
Artistic rendition of the exoplanet TOI-1452 b, a small planet that may be entirely covered in a deep ocean. Benoit Gougeon, Université de Montréal

The clues that this could be an ocean world are related to the planet’s radius, mass, and density. Although Earth has 70% of its surface covered by ocean, this water makes up less than 1% of our planet’s mass. But the planet TOI-1452 b has a density that suggests much of its mass, up to 30%, could be made up of lighter components like water.

Recommended Videos

“TOI-1452 b is one of the best candidates for an ocean planet that we have found to date,” explained lead researcher Charles Cadieux in a statement. “Its radius and mass suggest a much lower density than what one would expect for a planet that is basically made up of metal and rock, like Earth.”

Artistic representation of the surface of TOI-1452 b, which could be an “ocean planet”, i.e. a planet entirely covered by a thick layer of liquid water.
Artistic representation of the surface of TOI-1452 b, which could be an “ocean planet”, i.e. a planet entirely covered by a thick layer of liquid water. Benoit Gougeon, Université de Montréal

This makes the planet potentially similar to some moons in our solar system like Jupiter’s moons Ganymede and Callisto, or Saturn’s moons Titan and Enceladus, which are thought to host liquid oceans. However, the oceans on these moons are hidden beneath thick crusts of ice because they are so far from the sun.

Researchers are keen to study TOI-1452 b in more depth to see if it really is covered in a deep ocean, or whether there is another explanation for its size and density like being a very large rock with no atmosphere. They are hoping to schedule further observations of the planet using the James Webb Space Telescope.

“Our observations with the Webb Telescope will be essential to better understanding TOI-1452 b,” said another of the researchers, René Doyon, who is also the ​​Principal Investigator of Webb’s NIRISS instrument. “As soon as we can, we will book time on the Webb to observe this strange and wonderful world.”

The research is published in The Astronomical Journal.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Zoom into stunning James Webb image to see a galaxy formed 13.4 billion years ago
A section of a James Webb image showing a small part of the Extended Groth Strip, located between the Ursa Major and Boötes constellations.

One of the amazing things about the James Webb Space Telescope is the level of detail it is able to capture of very distant objects -- but it can be hard to picture what that means when the distances being considered are so large. Now, a new visualization gives a feel of just how detailed the data from the telescope is, by showing how it's possible to start with a stunning view of thousands of galaxies and zoom closer and closer in until you reach just one.

CEERS: Flight to Maisie's Galaxy

Read more
Astronomers spot the shiniest exoplanet ever discovered
An artist impression of exoplanet LTT9779b orbiting its host star.

When you look up at the night sky you see mostly stars, not planets -- and that's simply because planets are so much smaller and dimmer than stars. But you can see planets in our solar system, like Venus, which is one of the brightest objects in the night sky. Due to its thick, dense atmosphere, Venus reflects 75% of the sun's light, making it shine brightly. Recently, though, astronomers discovered a planet that reflects even more of its star's light, making it the shiniest exoplanet ever found.

Exoplanet LTT9779 b reflects 80% of the light from its star, which it orbits very close to. That makes it extremely hot, and researchers believe that the planet is covered in clouds of silicate and liquid metal, which is what makes it so reflective.

Read more
Astronomers spot an exoplanet creating spiral arms around its star
The Large Binocular Telescope in Arizona. The LBTI instrument combines infrared light from both 8.4-meter mirrors to image planets and disks around young and nearby stars.

When you imagine a galaxy like our Milky Way, you're probably picturing a swirl shape with arms reaching out from a central point. These spiral arms are a classic feature of many galaxies. Similar structures can be found around young stars which are surrounded by disks of matter from which planets form, called protoplanetary disks. Now, astronomers have discovered evidence that these structures could be created by recently formed exoplanets.

Astronomers used Large Binocular Telescope in Arizona to investigate a giant exoplanet named MWC 758c which seems to be forming the spiral arms around its host star. Located 500 light-years away, the star is just a few million years old, making it a baby in cosmic terms. "Our study puts forward a solid piece of evidence that these spiral arms are caused by giant planets," said lead researcher Kevin Wagner of the University of Arizona in a statement. "And with the new James Webb Space Telescope, we will be able to further test and support this idea by searching for more planets like MWC 758c."

Read more