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In lieu of more conventional advanced Spanish classes, paralleling a series of often disparate tutorials, with tutees working in relative isolation, the proposal is to allow students free reign over an idea for a final, term-long project, while concurrently offering them an educated, exoteric audience to assist in fleshing out their work.
How does influence travel from one thing to another? In Newton’s mechanics of particles and forces, influences travel instantaneously across arbitrarily far distances. Newton himself felt this to be incorrect, but he did not suggest a solution to this problem of “action at a distance.” To solve this problem, we need a richer ontology: The world is made not only of particles, but also of fields. As examples of the field concept, we study the theory and applications of the electric field and the magnetic field.
Students with burgeoning linguistic skills will learn the language through an immersion in Latin American and Spanish film in the second half of this full-year introduction to the Spanish-speaking world. While there will be some discussion of more common tactics such as stylistic nuances, script-writing, acting, dubbing, and directors’ biographies, it is expected that we will continue to develop sufficient linguistic ability to focus on cinematographic and social movements, thus treating the films as ideologemes, representations of political import.
Beyond Columbus’ errant journey into the abyss and the ensuing quest for El Dorado, or Darwin’s Voyage of the Beagle, Latin America’s interior has often enticed its own learned population. Their travels, in space, time and thought, do not merely present a physical confrontation with alterity, with the continent’s supposed heart of darkness, but an intellectual clearing, an origin, from which a more equitable politics may begin.
Students will observe using the telescopes at Stickney Observatory for a series of astronomical observing projects. After a range of initial assigned projects designed to acquaint students with the capabilities of the observing equipment and astrophysically interesting observations, students will propose and carry out their own observing projects looking at astrophysical phenomena of interest to them. As this is a projects class, it is expected that students will be able to devote significant time (mostly at night) observing on their own or in small teams.