April 2015

DateEventLocation
Saturday, Jan 31–Sunday, May 17
5:00 pm
Astronomical: Photographs of Our Solar System and Beyond

The evolution of photography has been inextricably bound up with the field of astronomy. Since photography's earliest days, it has been used as a tool to advance astronomical observation and thought, yielding some of the most curious and compelling images in the medium's history. Featuring works by a diversity of makers ranging from pioneering scientists to artists and amateurs, this exhibition surveys mankind's ongoing efforts to chart and understand an expanding universe.

Center for Creative Photography Gallery
1030 N. Olive Rd.

Free to the public
Center for Creative Photography Gallery: Room
Monday, Apr 6
4:00 pm — 5:00 pm
TAP Colloquium: Smadar Naoz
TAP Colloquia
Kuiper Space Sciences: Room 312
Tuesday, Apr 7
2:00 pm — 5:00 pm
Final Ph.D. Defense: Catherine M. Elder
Final Defense
Ph.D. in Planetary Sciences

Catherine M. Elder
Department of Planetary Sciences

The Effects of Melt on Impact Craters on Icy Satellites and on the Dynamics of Io's Interior
Kuiper Space Sciences: Room 309
Tuesday, Apr 14
3:45 pm — 5:00 pm
LPL Colloquium: Dr. Catherine Johnson
Dr. Catherine Johnson
Professor
University of British Columbia

Mercury's Magnetic Field: Stories from the Planet, Present and Past

Mercury is the only inner solar system body other than Earth to possess an active core dynamo-driven magnetic field, and the only planet with a highly dynamic, small magnetosphere. Measurements made by the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft have provided a wealth of data on Mercury's magnetic field environment. Mercury's weak magnetic field was discovered 40 years ago by the Mariner 10 spacecraft; but its large-scale geometry, strength and origin could not be definitively established. MESSENGER data have shown that the field is dynamo-generated and can be described as an offset axisymmetric dipole field: the magnetic equator lies ~0.2 RM (RM = 2440 km) north of the geographic equator and the dipole moment is 0.03% that of Earth's. Re-analysis of the Mariner 10 observations has established that there has been no measurable secular variation in the internal field over 40 years. The spherical harmonic degree power spectra for the field and its secular variation provide critical constraints for viable dynamo models. Induced core fields result from time-varying magnetopause fields and their magnitude confirms the core radius estimated from MESSENGER gravity and Earth-based radar data. Field-aligned currents have been identified, that likely close in the planetary interior at depths below the base of the crust. Recent magnetic field measurements at altitudes below 50 km have the potential to resolve fields of crustal origin, which have not been seen at higher altitudes.
Kuiper Space Sciences: Room 312
Monday, Apr 20
4:00 pm — 5:00 pm
TAP Colloquium: Norbert Wex
TAP Colloquia
Kuiper Space Sciences: Room 312
Tuesday, Apr 21
3:45 pm — 5:00 pm
LPL Colloquium: Dr. Alexander Hayes
Dr. Alexander Hayes
Assistant Professor
Cornell University
Kuiper Space Sciences: Room 312
Monday, Apr 27
4:00 pm — 5:00 pm
TAP Colloquium: Cora Dvorkin
TAP Colloquia
Kuiper Space Sciences: Room 312
Tuesday, Apr 28
3:45 pm — 5:00 pm
LPL Graduate Student Colloquia: Hamish Hay and Shane Stone
Hamish Hay
Graduate Student in the Department of Planetary Sciences

Shane Stone
Graduate Student in the Department of Planetary Sciences
Kuiper Space Sciences: Room 312