Sally C. Morton, executive vice president of ASU Knowledge Enterprise, presents a bold and practical framework for moving research from discovery to real-world impact
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Updates every hour. Last Updated: 15-Feb-2026 01:11 ET (15-Feb-2026 06:11 GMT/UTC)
In a must-see topical lecture called “From Discovery to Impact: A Framework for Research That Strengthens Communities,” Morton draws on Arizona State University’s pioneering model of use-inspired research — where excellence is measured by the overall economic, social, cultural, and overall health of the communities ASU serves.
Scientists have long understood that heating a metal softens it. New study shows that, counterintuitively, heat strengthens pure metal in extreme conditions. On the other hand, alloyed metals become softer, which is in line with intuition. Findings could lead to better designed metals for applications in extreme conditions, including outer space.
On 2 July, 2025, the China-led Einstein Probe (EP) space telescope detected an exceptionally bright X-ray source whose brightness varied rapidly during a routine sky survey. Its unusual signal immediately set it apart from ordinary cosmic sources, triggering rapid follow-up observations by telescopes worldwide.
This research was coordinated by the EP Science Center of the National Astronomical Observatories, Chinese Academy of Sciences (NAOC), with participation from multiple research institutions in China and abroad. Astrophysicists from the Department of Physics at The University of Hong Kong (HKU), who are integral members of the EP scientific team, worked together with the broader collaboration to interpret the event, proposing that it may mark the moment when an intermediate-mass black hole tears apart and consumes a white dwarf star. If confirmed, this would be the first observational evidence of such an extreme black hole “feeding” process. The findings have been published as a cover article in Science Bulletin.
The star, in the Andromeda galaxy, collapsed and disappeared without first exploding in a supernova.