Exoplanet LHS 1140 b Retains Atmosphere, Offering Insights into Cosmic Shoreline Theory
The discovery of an atmosphere on the exoplanet LHS 1140 b, a super-Earth located about 48 light-years away, marks a significant milestone in the study of exoplanets. This planet, orbiting a quiet red dwarf star, has been confirmed to have a helium-rich, hydrogen-poor upper atmosphere. The finding was initially predicted through a planetary evolution model and later confirmed by observations using the Magellan Clay telescope. This discovery is particularly noteworthy because LHS 1140 b is situated within its star's habitable zone, making it a prime candidate for studying atmospheric retention in rocky planets. The presence of an atmosphere on LHS 1140 b contrasts with its neighboring planet, LHS 1140 c, which shows no atmospheric traces, illustrating the concept of the cosmic shoreline—a theoretical boundary that determines whether a planet can maintain an atmosphere.