A research team led by York University has made a groundbreaking discovery regarding the quasar J2318, which exhibits the fastest wind ever recorded at ultraviolet wavelengths, reaching speeds of 30% of the speed of light. This quasar, located in the constellation Pegasus, contains a supermassive black hole with a mass of 1.7 billion solar masses. The study highlights the unique dynamics of quasar winds, which are propelled by the intense light emitted from the surrounding disk of gas. The findings were published in The Astrophysical Journal, with significant contributions from undergraduate students involved in the research. The team utilized data from the Sloan Digital Sky Survey (SDSS), specifically the SDSS-IV Time-Domain Spectroscopic Survey and the SDSS-V Black Hole Mapper, to identify the quasar's extreme wind. This discovery not only represents a significant advancement in understanding quasar dynamics but also emphasizes the role of student researchers in making impactful scientific contributions. The extreme outflows from quasars like J2318 are believed to have substantial effects on the galaxies they inhabit, serving as a critical link in understanding galaxy formation processes.