NASA's James Webb Space Telescope is helping scientists understand sub-Neptunes, the most common type of exoplanet in our galaxy, by observing exoplanet TOI-421 b.
Sub-Neptunes, smaller gassy planets shrouded in mystery and haze, were unexpected discoveries prior to the Kepler telescope's findings.
Webb's observations revealed the composition of TOI-421 b's atmosphere, including water vapor, carbon monoxide, sulfur dioxide, and a hydrogen-dominated atmosphere.
Contrary to expectations, TOI-421 b's clear atmosphere suggests a different formation and evolution process from other observed sub-Neptunes.
The hot sub-Neptune TOI-421 b orbits a Sun-like star and has a unique hydrogen-rich atmosphere, challenging previous assumptions.
The team aims to observe more hot sub-Neptunes to determine if TOI-421 b is an outlier or representative of a broader trend.
The researchers believe that this new way of studying sub-Neptunes may accelerate the understanding of these common exoplanets.
The findings were published in the Astrophysical Journal Letters on May 5, providing new insights into the formation and evolution of sub-Neptunes.
NASA's James Webb Space Telescope continues to unravel mysteries in our solar system and beyond, contributing to our understanding of distant worlds and the universe's origins.
The telescope is an international program led by NASA in collaboration with ESA and CSA, advancing space science exploration.