The Kepler telescope is designed to observe approximately 100,000 stars continuously over a 3.5-year mission, allowing it to detect exoplanets through transit events. It utilizes a large field of view and powerful CCDs, enabling it to monitor the brightness of multiple stars simultaneously. Although transits can be brief, Kepler's continuous monitoring increases the likelihood of detecting these events. The telescope captures images every 15 minutes, making it feasible to identify changes in brightness for individual stars. This extensive data collection will keep scientists engaged long after the mission concludes.