The James Webb Space Telescope's infrared capabilities allow it to pierce dust clouds, potentially revealing never-before-seen details about early star and galaxy formation.
By comparing data from JWST with existing observations in other wavelengths, scientists can gain a more comprehensive understanding of the atmospheres of exoplanets, potentially identifying biosignatures.
The JWST's extreme sensitivity offers the potential to detect fainter and more distant objects than ever before, pushing the boundaries of our observable universe.
The success of JWST's complex deployment process paves the way for future telescopes with even more ambitious capabilities.
Analyzing the data collected by JWST will likely necessitate the development of new analytical tools and techniques to fully grasp the telescope's groundbreaking observations.