COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring. |
University of Cambridge > Talks.cam > Department of Earth Sciences Seminars (downtown) > Metals, Magnetism and Meteorites: A brief guide to magnetic field generation on small planetary bodies
Metals, Magnetism and Meteorites: A brief guide to magnetic field generation on small planetary bodiesAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact David Wallis. Planetary magnetic fields are generated by vigorous convection of an electrically-conductive, molten metallic core. Paleomagnetic measurements have revealed that a surprising number of small planetesimals, with radii of just a few hundred kilometres, were able to sustain active magnetic fields in their early histories. This provides invaluable insight into their interior structure, formation and thermal histories. In order to extract these magnetic field histories, many novel experimental approaches have been utilized including synchrotron X-ray microscopy and quantum diamond microscopy. In particular, these methods have allowed paleomagnetic records to be extracted from tetrataenite, a mineral with an exceptionally robust ability to preserve records of magnetic fields that were active billions of years ago. Paleomagnetic records extracted from nanoscale tetrataenite structures in pallasite meteorites have demonstrated that the parent body must have had a large core and a thin mantle. Also, contrary to popular belief, these results show that pallasites do not represent core-mantle-boundary material. The formation of pallasite meteorites remains debated with several formation mechanisms currently in contention including ferrovolcanism, impacts and partial differentiation. By combining paleomagnetic data with petrological and geochemical observations, each of the proposed mechanisms can be systematically ruled in or out. Determining the nature and formation of small planetary bodies is key in understanding the processes that eventually resulted in the formation of the planets in our solar system today. This talk is part of the Department of Earth Sciences Seminars (downtown) series. This talk is included in these lists:
Note that ex-directory lists are not shown. |
Other listsCambridge University Entrepreneurs (CUE) yk373's list Clare College Graduate Research ForumOther talksPhysics for Sustainable Development ‘“Like Olive Shoots Around Your Table”: Locating the Early Modern Infant’ Child Development Forum Lent I Evolutionary Genetics of Visual Preferences: Beauty, Brains and Butterfly Diversity Challenges and future directions in cochlear implants Covariant properties of holographic entanglement |