Ultra-Hot “Super-Earth” Exoplanet 65 Light-Years Away Could Have No Atmosphere

Terrestrial Super-Earth GJ 1252 b

Illustration of the terrestrial super-Earth GJ 1252 b, which lies approximately 65 light-years from Earth. Credit: NASA/JPL-Caltech

Researchers have closely studied GJ 1252 b, a “super-Earth” exoplanet discovered in 2020, and suggest it may have a minimal or even non-existent atmosphere due to its extreme temperatures. Future investigations with the James Webb Space Telescope will aim to confirm these findings and explore the planet’s surface properties.

GJ 1252 b is a rocky, terrestrial “super-Earth” that was discovered in 2020. Astronomers have given the exoplanet a closer look and found that it could have a very minimal atmosphere or possibly no atmosphere at all.

The planet, which orbits an M-type star, is “the smallest exoplanet yet for which we have such tight constraints on its atmosphere,” said lead author Ian Crossfield. He is an astronomer and assistant professor at the University of Kansas.

Super-Earths are a class of planets unlike any in our solar system. They have a greater mass than Earth but are no more than 10 times its mass. This means that they are more massive than Earth yet lighter than ice giants like Neptune and Uranus. They can be made of gas, rock, or a combination of both.

Key Facts

Astronomers often discover and study exoplanets by observing how much light the planets block out as they pass in front of their host stars, a technique known as the “transit method.” GJ 1252 b, an exoplanet about 65 light-years away with a radius 1.18 times larger than Earth, was discovered in 2020 by NASA’s Transiting Exoplanet Survey Satellite (TESS) with this method. Astronomers in this new study observed the exoplanet with the Spitzer Space Telescope before it retired and were able to get a closer look at the planet and its atmosphere.

Using Spitzer, the team detected a secondary eclipse. This occurs when a planet passes behind a star and the planet’s light is blocked. The planet’s light comes from its own infrared radiation (or heat), as well as light reflected from the star.


Astronomers searching for signs of life in the cosmos focus on a number of different details in exoplanets. Many of these details serve as a comparison between the exoplanet and Earth, as Earth remains the only planet where we have confirmed the presence of life.

GJ 1252 b isn’t much larger than Earth. However, it is much hotter as it is closer to its star. Also, as astronomers discovered in this study, it is lacking much of an atmosphere.

“We’re just beginning to learn how often, and under what circumstances, rocky planets can keep their atmospheres,” said astronomer and study co-author Laura Kreidberg, the director of the Atmospheric Physics of Exoplanets (APEx Department at the Max Planck Institute for Astronomy. “This measurement is an indication that for the hottest planets, it’s unlikely that thick atmospheres typically survive.”

To determine what the exoplanet’s atmosphere (if there is one) could be like, astronomers measured infrared radiation from GJ 1252 b as its light was obscured during a secondary eclipse. These observations revealed the planet’s scorching day-side temperature, which is estimated to reach as high as 2,242 degrees Fahrenheit (1228 degrees Celsius). In fact, GJ 1252 b is so hot that gold, silver, and copper would all melt on the planet.

The exoplanet’s expected temperatures, when compared to atmospheric models, suggest that it likely has a surface pressure of less than 10 bar (for reference, Earth’s surface pressure is approximately 1 bar.) While the planet’s sizzling hot temperatures would make it difficult for an atmosphere to be stable for long, it is possible that this exoplanet could have an atmosphere with a density like Earth’s, an atmosphere up to 10 times denser than Earth’s, or even no atmosphere whatsoever.

Given its extreme temperatures and low surface pressure, the astronomers on this team have predicted that GJ 1252 b likely has no atmosphere at all. This is currently the smallest exoplanet for which scientists have such a clear idea of its atmosphere.

Fun Facts

GJ 1252b is an exoplanet that was first detected with TESS and then investigated more thoroughly with Spitzer before the telescope’s mission ended in 2020. With further exploration using the James Webb Space Telescope (JWST), the researchers could put even tighter constraints on this planet’s atmosphere, an exciting possibility.

“At the time, Spitzer was the only facility in the known universe that could make these sorts of measurements. Now, Spitzer has been turned off, but JWST is there and at these wavelengths, it’s much more sensitive than Spitzer was. So, what we did with difficulty with Spitzer we can now start to do easily and for larger numbers of rocky planets with JWST,” Crossfield said.

“JWST observations in the infrared have the potential to reveal the surface properties of hot, rocky planets like this. Different types of rock have different spectral signatures, so we could potentially learn what type of rock GJ 1252b is made of,” Kreidberg added.

Studying GJ 1252 b further with JWST poses an exciting possibility for scientists, as it would be interesting to confirm an atmosphere on such a small and hot exoplanet as it would also be fascinating to explore the composition of a planet like this with no atmosphere at all.

A team at the University of Kansas, led by Crossfield, led this study which discovered strange new details about the atmosphere of GJ 1252b.  The study, published in the Astrophysical Journal Letters.

Reference: “GJ 1252b: A Hot Terrestrial Super-Earth with No Atmosphere” by Ian J. M. Crossfield, Matej Malik, Michelle L. Hill, Stephen R. Kane, Bradford Foley, Alex S. Polanski, David Coria, Jonathan Brande, Yanzhe Zhang, Katherine Wienke, Laura Kreidberg, Nicolas B. Cowan, Diana Dragomir, Varoujan Gorjian, Thomas Mikal-Evans, Björn Benneke, Jessie L. Christiansen, Drake Deming and Farisa Y. Morales, 23 September 2022, Astrophysical Journal Letters.
DOI: 10.3847/2041-8213/ac886b

Additionally involved in this paper were researchers from the University of California, Riverside, NASA’s Jet Propulsion Laboratory (JPL), the Caltech/IPAC-NASA Exoplanet Science Institute, the University of Maryland, the Earth and Planets Laboratory at the Carnegie Institution for Science, the Max Planck Institute for Astronomy, McGill University, the University of New Mexico, Albuquerque, NM, and the Institute for Research on Exoplanets at the University of Montreal.

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