L 98-59 d: A sulfur-rich magma-ocean world redefining small-planet classification
To the point
L 98-59 d is a small exoplanet with a long-lived magma ocean that stirs a sulfur-rich atmosphere, JWST detects hydrogen sulfide and sulfur dioxide high in the atmosphere, and modeling by Harrison Nicholls and colleagues suggests it formed with lots of volatiles but lost most of that gas under strong X-ray irradiation, leaving a hydrogen-dominated atmosphere while the molten interior slowly releases sulfur for billions of years, a scenario Raymond Pierrehumbert and Richard Chatterjee say could define a new class of sulfur-rich magma-ocean worlds at the rocky/gas boundary with important implications for missions like Ariel and PLATO and for future machine-learning searches.
Exploring the Cosmos with James Webb
Steeven Cadel
The Extraterrestrial Species Almanac: The Ultimate Guide to Greys, Reptilians, Hybrids, and Nordics (MUFON)
Craig Campobasso
Vespera II Exploration Station with Smart Technology
After the Flying Saucers Came: A Global History of the UFO Phenomenon
Greg Eghigian
Our recommendations from Amazon