Spring 2026 Course Search

Historical Dress: The Park-McCullough Project Spring ‘26

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.

The seventeenth-century Flemish painter-diplomat Peter Paul Rubens is at the heart of a course that proposes the intrinsic baroqueness of diverse strains of high modernism. Our transdisciplinary project crosses entrenched nationalistic and chronological borders between modern and early modern art and artists including Bacon, Guston, Manet, Newman, Picasso, Bearden, and Titian in addition to Robert Rauschenberg (1925-2008), himself a more conceptually various and possibly more prolific artist even than Rubens (1577-1640) to whom some 3,000 paintings and drawings have been attributed.

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.

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). 

How do we transition to a low-carbon economy in a manner that doesn’t reinscribe the social and environmental injustices that have plagued our fossil-fueled economy? On one hand, the continued burning of fossil fuels is producing environmental crises that threaten to destabilize the very foundations of collective life, with poor and historically marginalized communities bearing the brunt of the suffering. On the other hand, renewable energy technologies are far from environmentally and socially benign.

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.

Economic inequality is often described in terms of uneven distribution of income and wealth. Yet, more importantly, it reflects uneven access to opportunities, advantages, and life chances. Why do some people enjoy a higher standard of living and better quality of life than others? Are such inequalities fair and just? What role do history, policy, and institutions play in sustaining or reducing inequality?

Why does chronic hunger endure even in times of prosperity? How can famine devastate entire regions in extreme cases, while food deserts quietly persist in wealthy countries like the United States? And what does it mean to treat nourishment not as charity or commodity, but as a right of citizenship?

To be LGBTQIA and AAPI is to occupy two disparate, marginalized identities that seem to be be in constant flux. What might the literature of this intersection teach us about larger questions of community, belonging, and resistance? This 2000-level class attempts to locate a Queer Asian Pacific America through literature, from Chinese American lesbian poets of the 1980s to Fatimah Asghar's recent cross-genre coming-of-age novel; from David Henry Hwang’s reimagining of Madame Butterfly to queer Hawaiian reclamations of aloha; and beyond.

Qualitative inquiry seeks to discover and to describe in narrative reporting what particular people do in their everyday lives and what the actions mean to them. This course is intended for students who wish to learn more about the impact of theoretical frameworks on their ongoing knowledge projects at Bennington College.

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.