James Webb Space Telescope Observes Hot Jupiter Exoplanet with Unexplained Twin Gas Tails
The James Webb Space Telescope (JWST) has made a groundbreaking discovery of a distant 'hot Jupiter' exoplanet, WASP-121b, which exhibits two extensive gas tails composed of helium. This observation marks the first comprehensive study of atmospheric escape from a planet outside our solar system during a complete orbit. WASP-121b, located approximately 858 light-years away, is an 'ultrahot Jupiter' that orbits its star every 30 hours, with its atmosphere reaching temperatures of around 4,200 degrees Fahrenheit. The intense heat causes lighter gases like hydrogen and helium to escape into space, altering the planet's size and composition over millions of years. The JWST's Near-Infrared Spectrograph (NIRSpec) was used to observe the planet for 37 consecutive hours, revealing the longest continuous detection of helium escape. The helium forms two distinct tails, one trailing behind the planet due to stellar winds and radiation, and the other leading the planet, likely influenced by gravitational forces.