Spring 2026 Course Search

Historical Dress: The Park-McCullough Project Spring ‘26

Delights of Ephemera explores the significance of mass-produced materials in the context of art movements and exhibitions. Contrary to its definition, ephemera can have power and permanence, giving agency to marginal and marginalized groups and providing a record of actions outside institutional structures. A poster for an exhibition can be as important—or, in terms of its historical presence, more important—as the exhibition itself.

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.

In this course, we will explore various projects that aim to connect people with their surroundings and communities.
We will also explore the strategies that various artists have implemented to increase their audiences and interest in the arts.
We will analyze and design projects that seek sustainability, diversification, and access to the experience of art and culture.

By evaluating environments we could design artistic projects that promote art, artistic education, and the promotion of cultural products as actions to build community, identity, and a creative economy.

This course is a seminar focusing on films that were made by filmmakers and collectives which saw themselves as inaugurating a new kind of filmmaking modeled neither on the commercial American filmmaking, nor on the European “Auteur” Cinema, instead crafting a third position, a cinema that was implicated in anti-capitalist and anti-imperialist struggles of the time. These works challenged ideas of authorship, questioned the role of the filmmaker in political transformation, and proposed alternatives to the forms of production that filmmaking made use of.

This production course introduces students to the fundamentals of working in video and the language of film form. Drawing on the energy, intensity and criticality of avant-garde film and contemporary video art practices, students will complete a series of projects exploring dimensions of cinematography, mise-en-scène, editing and sound design before producing a final self-determined project. Concepts crucial to time-based media such as apparatus, montage and identification will be introduced through screenings, discussions and texts by a diverse range of artists, filmmakers, and theorists.

Self-reflexive narratives, improvisation, non-linearity, slow cinema, alternative representations of time and space, experimental film grammars, poetic scripts, collective direction, Brechtian techniques.  All of these processes and more will be explored in this hands-on production based course. Working collaboratively and on your peers’ work in various roles is required for this course. This course is appropriate to students doing advanced work in film and video as we will be taking a project from research, writing and structuring to post-production in the span of a term.

All but a handful of the objects you see in the night sky are stars in our Galaxy, the Milky Way. Although we know about these stars only from studying their light, we know today that they are not just points of light, but large, gravitationally‐bound balls of plasma governed by the laws of physics. Stars, together with dust, gas, and dark matter, are found in larger structures – galaxies. In turn, galaxies, are located in even larger structures called galaxy groups and galaxy clusters.

The physics of light and color initially appears simple: light is a wave and the wavelength of light determines color. While this basic physical description of light is easy to state, going deeper quickly opens up large range of questions. How do different wavelengths of light combine to make colors? How does light from different sources interfere? How does light change path when it travels through different materials? How do humans sense light both in and outside of the visible spectrum? How does our perception of color affect how we interpret our world?

Physically, sound is simply the compression of air around us. However, this relatively simple description obscures a much richer understanding of sound. From how different sounds are generated and perceived to how different sounds can combine to make something new to how to design acoustically pleasant spaces, the physics of sound plays a key role. This course is about the fundamentals that underlie sound and is designed to serve as an introduction to those who are interested in going further.

In this course, students will gain experience with using simple programmable robots and how they can be utilized in STEM education. The focus of this class will be on learning and designing lessons for K-12 students utilizing these robots. This class is accessible for students at all levels of computer programming experience (including none). 

Historical Dress: The Park-McCullough Project Spring '26

Working in collaboration with the local Park-McCullough Historic Governor’s Mansion, students will create a new archive of the historic dress collection.

Students will work towards completing one moving image piece or body or work of their own devising during the course of the semester. This course is primarily intended for seventh- and eighth-term students with a Plan concentration in Film/Video who have already taken Advanced Projects I in the prior fall, but exceptions may be made by permission of the instructor.

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.