2015 Spring Physics Colloquium Series: Matt Tiscareno, Ph.D.

DateJanuary 16, 2015
Time4:00 - 5:00 pm
LocationBaylor Sciences Building, Room E.125
Matt Tiscareno, Ph.D.

Senior Research Associate

Cornell University

Saturns Rings - An Accessible Astrophysical Disk

Saturn's ring system is an astrophysical disk that is neither light-years away nor billions of years in the past. We can visit this disk at close range and observe a number of phenomena that also operate in disks of other kinds. As a result, we see small-scale processes that shape ring texture, connect those processes to the bodies and structures that cause them, and watch closely as the disk changes with time. We will discuss recent Cassini observations that elucidate disk processes including

1) "self-gravity wakes" and "spiral density waves," both of which were originally
proposed for galaxies but are observed with exquisite precision in Saturn's rings,

"propeller" features caused by 100-meter to km-sized moonlets embedded in the disk; these are the first objects ever to have their orbits tracked while embedded in a disk, rather than orbiting in free space, and hold the potential of deepening our understanding of planetary migration, and

3) irregular edge shapes in the gaps opened up by larger moons (10 km and more), which may hold clues to angular momentum transport.

For more information, please contact:
Dr. Lorin Matthews 254-710-2279
PublisherDepartment of Physics
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