Skip to main content

Astronomers discover Earth-sized exoplanet covered in volcanoes

Astronomers have discovered an Earth-sized planet that is highly volcanically active — an unusual finding that means it could possibly support life. The newly discovered planet, LP 791-18d, is thought to be covered in volcanoes and could be as active as Jupiter’s moon Io, which is the most volcanically active body in our solar system.

Exoplanet LP 791-18 d, illustrated in this artist’s concept, is an Earth-size world about 90 light-years away. A more massive planet in the system, shown as a small blue dot on the right, exerts a gravitational tug that may result in internal heating and volcanic eruptions, like on Jupiter’s moon Io.
Exoplanet LP 791-18 d, shown in this artist’s concept, is an Earth-size world about 90 light-years away. A more massive planet in the system, shown as a small blue dot on the right, exerts a gravitational tug on the exoplanet that may result in internal heating and volcanic eruptions, like on Jupiter’s moon Io. NASA’s Goddard Space Flight Center/Chris Smith (KRBwyle)

While we generally associate volcanoes with destruction, they can in fact be an important part of making a planet habitable because of the way they help create and sustain an atmosphere. It isn’t yet known if this particular planet has an atmosphere, but the volcanic activity makes it more likely. It is located within the habitable zone, where water could potentially exist on its surface.

It was discovered using data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and the now-retired Spitzer Space Telescope, which observed a small red dwarf star located 90 light-years away.

Some of the distinctive features of the planet have to do with how it rotates around its star, with one side always facing inward and the other side always facing outward. That leads to extreme conditions on the two sides of the planet. “LP 791-18 d is tidally locked, which means the same side constantly faces its star,” explained lead researcher Björn Benneke in a statement. “The day side would probably be too hot for liquid water to exist on the surface. But the amount of volcanic activity we suspect occurs all over the planet could sustain an atmosphere, which may allow water to condense on the night side.”

It is thought that the planet could be volcanically active because of the other planets in the same star system, LP 791-18 b and c. Planet c in particular passes very close to planet d during its orbit, which could be creating internal friction inside the planet and heating it up, causing volcanoes to be active on its surface. This relationship between the interior of a planet and active volcanoes has the interest of scientists who are studying conditions for life.

“A big question in astrobiology, the field that broadly studies the origins of life on Earth and beyond, is if tectonic or volcanic activity is necessary for life,” said co-author Jessie Christiansen. “In addition to potentially providing an atmosphere, these processes could churn up materials that would otherwise sink down and get trapped in the crust, including those we think are important for life, like carbon.”

For a next step, researchers plan to use the James Webb Space Telescope to observe the exoplanet and see if it does indeed have an atmosphere.

“The discovery of an Earth-size planet in the habitable zone that is potentially volcanically active is a huge step forward in the search for life outside the solar system,” said another of the researchers, Mohamad Ali-Dib. “The next step is to observe the system using the [James Webb Space Telescope] to see what it can tell us about its atmosphere.”

The research is published in the journal Nature.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Astronomers discover extremely hot exoplanet with ‘lava hemisphere’
Like Kepler-10 b, illustrated above, the exoplanet HD 63433 d is a small, rocky planet in a tight orbit of its star. HD 63433 d is the smallest confirmed exoplanet younger than 500 million years old. It's also the closest discovered Earth-sized planet this young, at about 400 million years old.

Astronomers have discovered an Earth-sized exoplanet with an unusually extreme climate where one half of the planet is thought to be covered in lava. The planet HD 63433 d is tidally locked, meaning one side of it always faces its star while the other half always faces out into space, creating a huge difference in temperatures between the planet's two faces.

Like Kepler-10 b, illustrated above, the exoplanet HD 63433 d is a small, rocky planet in a tight orbit of its star. HD 63433 d is the smallest confirmed exoplanet younger than 500 million years old.  NASA/Ames/JPL-Caltech/T. Pyle

Read more
See the weather patterns on a wild, super hot exoplanet
This is an artist’s impression of the exoplanet WASP 121-b, also known as Tylos. The exoplanet’s appearance is based on Hubble data of the object. Using Hubble observations, another team of scientists had previously reported the detection of heavy metals such as magnesium and iron escaping from the upper atmosphere of the ultra-hot Jupiter exoplanet, marking it as the first of such detection. The exoplanet is orbiting dangerously close to its host star, roughly 2.6% of the distance between Earth and the Sun, placing it on the verge of being ripped apart by its host star's tidal forces. The powerful gravitational forces have altered the planet's shape.

When it comes to understanding exoplanets, or planets outside our solar system, the big challenge is in not only finding these planets, but also understanding what they are like. And one of the biggest factors that scientists are interested in is whether an exoplanet has an atmosphere and, if so, what it is composed of. But, just like with weather here on Earth, exoplanet atmospheres aren't static. So the Hubble Space Telescope was recently used for an intriguing observation -- comparing data from an exoplanet atmosphere that had previously been observed, to see how it changed over time.

Hubble looked at planet WASP-121 b, an extreme planet that is so close to its star that a year there lasts just 30 hours. Its surface temperatures are over 3,000 Kelvins, or 5,000 degrees Fahrenheit, which researchers predict would lead to some wild weather phenomena. As it is such an extreme planet, WASP-121 b is well-known and has been observed by Hubble several times over the years, beginning in 2016.

Read more
Astronomers spot rare star system with six planets in geometric formation
Orbital geometry of HD110067: Tracing a link between two neighbour planets at regular time intervals along their orbits, creates a pattern unique to each couple. The six planets of the HD110067 system together create a mesmerising geometric pattern due to their resonance-chain.

Astronomers have discovered a rare star system in which six planets orbit around one star in an elaborate geometrical pattern due to a phenomenon called orbital resonance. Using both NASA's Transiting Exoplanet Survey Satellite (TESS) and the European Space Agency's (ESA) CHaracterising ExOPlanet Satellite (CHEOPS), the researchers have built up a picture of the beautiful, but complex HD110067 system, located 100 light-years away.

The six planets of the system orbit in a pattern whereby one planet completes three orbits while another does two, and one completes six orbits while another does one, and another does four orbits while another does three, and so one. The six planets form what is called a "resonant chain" where each is in resonance with the planets next to it.

Read more