Science
Discover super-earths, exoplanets larger than our world but smaller than Neptune. Learn why these planets are key in the search for alien life.
A super-earth is an extrasolar planet with a mass higher than Earth's but substantially below that of the Solar System's ice giants, Uranus and Neptune. The term refers only to the planet's mass and does not imply anything about its surface conditions or habitability. These planets can be rocky, gaseous, or a combination of both, making them a diverse and common class of planets found in our galaxy. While our solar system has no super-earths, they appear to be one of the most frequent types of exoplanets discovered so far.
Super-earths are a hot topic due to advanced telescopes like the James Webb Space Telescope (JWST) and the Kepler Space Telescope. These instruments have discovered numerous super-earths, some of which are located in the 'habitable zone' of their star—the orbital region where conditions might be right for liquid water to exist. Recent findings, such as analyzing the atmospheres of these distant worlds, keep them in the news and fuel scientific and public excitement about the potential for life beyond Earth.
The study of super-earths fundamentally changes our understanding of planet formation and the prevalence of different planetary systems. It challenges the idea that our solar system's structure is typical. For the public, the search for habitable super-earths addresses profound questions about our place in the cosmos and the possibility of extraterrestrial life. This research inspires future generations of scientists and engineers and drives the development of new technologies for exploring the universe, connecting us all to the grand scale of cosmic discovery.