The Super Cryogenic Dark Matter Search (SuperCDMS) experiment, based at SNOLAB in Sudbury, Ontario, Canada, has achieved a critical milestone by cooling its detectors to just above absolute zero. This temperature is essential for the superconducting sensors to operate effectively, allowing for the detection of dark matter, which is believed to constitute much of the universe's mass. Texas A&M University physicist Dr. Rupak Mahapatra and his team designed these advanced semiconductor detectors, which are crucial for identifying 'light dark matter'—a challenging target due to its low mass. The underground location of SNOLAB, approximately 6,800 feet deep, protects the experiment from cosmic rays and other noise that could interfere with the faint signals sought by scientists. With the detectors now cold enough to function, the team will start commissioning the 24 detectors, tuning them for a year-long data collection phase. This experiment not only aims to uncover dark matter but also to explore rare isotopes and uncharted energy levels. The SuperCDMS project is supported by the U.S. Department of Energy Office of Science, the National Science Foundation, and Canadian research councils.