NASA’s TESS mission has discovered TOI-715 b, a super-Earth located 137 light-years away in the conservative habitable zone of an M-dwarf star. The planet is 1.5 times the size of Earth and orbits its star every 19 days, making it a prime candidate for atmospheric study by the James Webb Space Telescope.
TLDR: NASA researchers have identified TOI-715 b, a rocky super-Earth orbiting within the habitable zone of a nearby red dwarf star. Located 137 light-years away, the planet’s size and position make it a leading candidate for future atmospheric analysis to search for signs of water and potential habitability.
NASA’s Transiting Exoplanet Survey Satellite (TESS) has identified a significant new exoplanet that could provide a breakthrough in the search for habitable worlds. The planet, designated TOI-715 b, is a “super-Earth” approximately 1.5 times the width of our home planet. It orbits a small, reddish star about 137 light-years away from Earth. This discovery is particularly notable because the planet resides within the “conservative” habitable zone of its parent star, a region where conditions are most likely to allow for the presence of liquid water on the surface.
Astronomers distinguish between the “optimistic” and “conservative” habitable zones when evaluating new worlds. While the optimistic zone represents a broader range where water might exist, the conservative zone is a much narrower and more scientifically rigorous band. TOI-715 b sits firmly within this tighter region, suggesting that if atmospheric conditions are right, it could maintain the surface temperatures necessary for life. The planet completes a full orbit around its star in just 19 days, a rapid cycle that allows for frequent observation by space-based telescopes.
The parent star, TOI-715, is an M-dwarf, a type of star that is smaller, cooler, and redder than our Sun. These stars are the most common type in the Milky Way galaxy and have become primary targets for exoplanet hunters. Because M-dwarfs are dimmer than the Sun, planets can orbit much closer to them while remaining within the habitable zone. This proximity makes it easier for instruments like TESS to detect the slight dip in light as a planet passes in front of its star, a method known as the transit technique.
Researchers at NASA’s Jet Propulsion Laboratory and the University of Birmingham led the validation of the TESS data. Their analysis suggests that the system may also contain a second, Earth-sized planet. If confirmed, this second candidate would be the smallest habitable-zone planet TESS has discovered to date. The presence of multiple rocky planets in the same system provides a unique opportunity for comparative planetology, allowing scientists to study how different sizes and orbits affect planetary evolution.
One of the primary challenges for habitability on M-dwarf planets is the tendency of these stars to produce intense solar flares. These bursts of radiation can potentially strip away a planet’s atmosphere over millions of years. However, TOI-715 appears to be a relatively quiet star for its class, which increases the likelihood that TOI-715 b has retained its atmosphere. Determining the composition of this atmosphere is the next major hurdle for the research team.
The James Webb Space Telescope (JWST) is the primary tool slated for follow-up observations. By analyzing the light filtering through the planet’s atmosphere during a transit, the JWST can identify chemical signatures such as water vapor, methane, or carbon dioxide. These findings would provide the first definitive evidence of whether TOI-715 b is a truly habitable world or a barren rock. The planet’s 19-day orbit ensures that the JWST will have many opportunities to capture data during transits.
Future research will also focus on measuring the planet’s mass using the radial velocity method. This technique tracks the slight wobble of the parent star caused by the planet’s gravitational pull. Combining the mass data with the size measurements from TESS will allow scientists to calculate the planet’s density. This calculation is essential for determining whether the world is a rocky terrestrial planet, a water world, or a gas-shrouded sub-Neptune. These findings will refine our understanding of how common Earth-like environments are in the local galaxy.

