Skip to main content

Astronomers discover rare ‘exo-Venus’ just 40 light-years away

Gliese 12 b, which orbits a cool, red dwarf star located just 40 light-years away, promises to tell astronomers more about how planets close to their stars retain or lose their atmospheres. In this artist’s concept, Gliese 12 b is shown retaining a thin atmosphere.
Gliese 12 b, which orbits a cool, red dwarf star located just 40 light-years away, promises to tell astronomers more about how planets close to their stars retain or lose their atmospheres. In this artist’s concept, Gliese 12 b is shown retaining a thin atmosphere. NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)

Astronomers have discovered a rare type of planet called an “exo-Venus,” which is between the size of Earth and Venus and is located just 40 light-years away — practically in our back yard. Although scientists think that planets of this size could be very common in our galaxy, they are hard to identify because they are so much smaller than the big gas giants that are more commonly discovered. This new planet also seems to have similar temperatures to Earth, and studying it could help to explain how atmospheres develop and how Earth became habitable.

Recommended Videos

The planet is named Gliese 12 b and was identified using a range of Earth-based telescopes as well as NASA’s TESS space telescope. It orbits its host star, called Gliese 12, in just 12.8 Earth days, so it is very close in and a year there is extremely short. However, because the star is a cool red dwarf type, it is estimated to maintain a relatively comfortable temperature of 42°C (107°F), making it much cooler than most exoplanets discovered so far.

However, that estimate assumes that the planet doesn’t have an atmosphere. It could be without atmosphere, have an Earth-like atmosphere, or it could have an extremely thick atmosphere like Venus, which could raise its temperature to hundreds of degrees. Researchers are keen to learn whether there is an atmosphere there, not only to know about its habitability (whether liquid water could exist on the planet’s surface) but also so they can learn about how atmospheres develop around rocky planets.

“Gliese 12 b represents one of the best targets to study whether Earth-size planets orbiting cool stars can retain their atmospheres, a crucial step to advance our understanding of habitability on planets across our galaxy,” said lead author Shishir Dholakia of the University of Southern Queensland in Australia in a statement. “Much of the scientific value of this planet is to understand what kind of atmosphere it could have. Since Gliese 12 b gets in between the amount of light as Earth and Venus get from the Sun, it will be valuable for bridging the gap between these two planets in our solar system.”

A big topic of research in planetary science right now is why Earth and Venus diverged. The planets are a similar size and distance from the sun, and could once have been similar. But today, the Earth is teeming with life and Venus is a hellish world of extreme temperature and pressure. Studying planets like Gliese 12 b could help explain how this divergence occurred and whether Earth-like or Venus-like is the more common outcome.

“We know of only a handful of temperate planets similar to Earth that are both close enough to us and meet other criteria needed for this kind of study, called transmission spectroscopy, using current facilities,” said another researcher, Michael McElwain of NASA’s Goddard Space Flight Center. “To better understand the diversity of atmospheres and evolutionary outcomes for these planets, we need more examples like Gliese 12 b.”

The research is published in the journal the Monthly Notices of the Royal Astronomical Society and the Astrophysical Journal Letters.

Please enable Javascript to view this content

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
First indications of a rare, rainbow ‘glory effect’ on hellish exoplanet
For the first time, potential signs of the rainbow-like ‘glory effect’ have been detected on a planet outside our Solar System. Glory are colourful concentric rings of light that occur only under peculiar conditions. Data from ESA’s sensitive Characterising ExOplanet Satellite, Cheops, along with several other ESA and NASA missions, suggest this delicate phenomenon is beaming straight at Earth from the hellish atmosphere of ultra-hot gas giant WASP-76b, 637 light-years away.

Just from looking at our own solar system, we can see that planets come in a wide variety of colors -- from the dusty red of Mars to the bright blues of Uranus and Neptune. Planets like Jupiter have beautiful bands of color caused by variations in the atmosphere, while it's hard to even see the surface of Venus because its atmosphere is so thick. But there are other variations in color which planets can display, like a stunning rainbow-hued set of circular rings called a glory.

Glories are observed on Earth, and have been seen just once on another planet, Venus. But now, researchers believe they may have identified a glory on a planet outside our solar system for the first time. The extreme exoplanet WASP-76b could be host to the first known extrasolar glory, observed by the European Space Agency (ESA)'s Characterising ExOplanet Satellite (Cheops).

Read more
Astronomers discover a super-Earth located in the habitable zone
This illustration shows one way that planet TOI-715 b, a super-Earth in the habitable zone around its star, might appear to a nearby observer.

Astronomers have discovered a type of exoplanet called a "super-Earth" located in the habitable zone of its small star, and it's right in our cosmic backyard, just 137 light-years away. The planet, named TOI-715 b, is intriguing to astronomers who are increasingly interested in the possibility of habitable planets orbiting stars quite different from our sun.

Although it might seem to make sense to look for potentially habitable planets when looking for Earth-like planets orbiting sun-like stars, those aren't the only targets that astronomers are interested in. One issue is that most discovered exoplanets are much larger than Earth, partly because it is so hard to detect smaller planets. Another issue is that the most common star in our galaxy by far is not a yellow dwarf star like our sun, but a smaller, dimmer, redder type called a red dwarf. When researchers discover rocky planets orbiting around red dwarfs, a few of which have been identified to date, that increases the pool of potentially habitable worlds that could be out there.

Read more
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