Roger Fu, MIT Graduate Student
/ education /
BA in Earth and Planetary Sciences and Astrophysics, Harvard College 2009
/ description /
I joined the paleomagnetism lab in spring 2011. Most of my work revolves around understanding the early solar system, in particular the formation and evolution of the first solid bodies.
I am first and foremost a paleomagnetist, and my primary projects aim to measure some of the earliest solids in the solar system- chondritic meteorites- for a recording of the magnetic field of the primordial protosolar disk. The nature of these magnetic fields have broad implications for the dynamics of the protoplanetary disk and the style of accretion on both large and small scale.
Another set of paleomagnetic projects study the magnetic record found in the HED meteorites, which likely originate from the asteroid Vesta. Our measurements strongly suggest that this asteroid once harbored a magnetic core dynamo.
As for paleomagnetic techniques, I'm modeling the geodynamics of Vesta, which had a thin and heavily fractured lithosphere during its earliest history. These conditions likely allowed Vesta to approach a hydrostatic figure as observed on the terrestrial planets and icy satellites.
In the past I have worked on melt migration on planetesimals, the interior dynamics of icy super-Earths, phyllosilicates on Mars, X-ray observations of distant galaxies, molecules in circumstellar envelopes, and the indigenous astronomy of the Pewenche people of South America. I still work on some of these topics part-time. Email me if you'd like to chat about anything on (or not on) this page!
/ email /
/ mailing address /
77 Massachusetts Ave.
Cambridge, MA 02139
/ phone numbers /
/ curriculum vitae /
/ list of publications /
R. R. Fu, B. P. Weiss, D. L. Shuster, J. Gattacceca, T. L. Grove, C. Suavet, E. A. Lima, L. Li, A. T. Kuan (2012) An Ancient Core Dynamo in Asteroid Vesta, Science, 338, 238-241 / link / / supplementary information /
R. R. Fu and B. P. Weiss (2012) Detrital remanent magnetization in the solar nebula, Journal of Geophysical Research-Planets, 117, E02003 / link /
R. R. Fu, A. Moullet, N. A. Patel, J. Biersteker, K. L. Derose, K. H. Young (2012) Arcsecond resolution mapping of Sulfur Dioxide emission in the circumstellar envelope of VY Canis Majoris, The Astrophysical Journal, 746:42, 1-12 / link /
R. Fu, R.J. O'Connell, and D.D. Sasselov (2010) The Interior Dynamics of Water Planets, The Astrophysical Journal, 807, 1326-1334 / link /
E. Z. Noe Dobrea, J. L. Bishop, N. K. McKeown, R. Fu, et al (2010) Mineralogy and stratigraphy of phyllosilicate‐bearing and dark mantling units in the greater Mawrth Vallis/west Arabia Terra area: Constraints on geological origin, Journal of Geophysical Research, 115
G. Trinchieri, S. Pellegrini, G. Fabbiano, R. Fu, N. J. Brassington et al. (2008) Discovery of Hot Gas in Outflow in NGC 3379, The Astrophysical Journal, 688, 1000-1008