Astronomers have captured detailed images of a gas giant forming within a protoplanetary disk, offering new insights into how planets are born. The observations, made using the ALMA (Atacama Large Millimeter/submillimeter Array) observatory in Chile, focus on the WISPIT 2 system, which is about 430 light-years from Earth. This system includes a gas giant named WISPIT 2b, five times more massive than Jupiter, which is still gathering gas from its surroundings. This process was detected using the "Hα line," a specific type of light emitted by hot hydrogen atoms, which indicates ongoing accretion. The WISPIT 2 system was discovered in August 2025 and is the second known system where a protoplanet can be clearly seen. A second planet, WISPIT 2c, was identified in March 2026 using advanced instruments on the Very Large Telescope (VLT), including SPHERE and GRAVITY+. More recently, research published in August 2026 revealed that the system contains two stars orbiting very closely around each other, rather than a single central star. This binary star configuration adds complexity to the planet formation process. Using ALMA's powerful imaging capabilities, astronomers observed how WISPIT 2b interacts with the surrounding gas in the disk. Observations conducted in September 2025, November 2025, and March 2026 revealed distinct structures, including a cavity created by WISPIT 2c and a gap formed by WISPIT 2b. Around WISPIT 2b, the team detected swirling patterns of gas, a phenomenon predicted by simulations of how planets interact with their disks but never before observed in real life. These findings offer direct evidence of a gas giant actively shaping its environment during its formation. The discovery could help settle ongoing debates about similar swirling features observed in other protoplanetary disks. Some scientists believe these features are caused by hidden planets, while others think they result from natural turbulence in the disk. WISPIT 2b is the only known protoplanet where such direct interaction with surrounding gas has been observed. Currently, the observations focus on a gas giant located 57 astronomical units (AU) from the central stars—nearly twice the distance of Neptune from the Sun. Most known exoplanets are much closer to their host stars. However, the techniques used in this study may allow future observations with more advanced instruments, such as ESO's Extremely Large Telescope and an upgraded ALMA, to capture images of gas giants at distances similar to Jupiter and Saturn from their stars. This could provide a more complete picture of planet formation across different regions of a solar system.