Spring 2026 Course Search

This course asks each student to work in a self-directed way among a community of critical thinkers. Finding one’s voice, as a maker, requires research sources of influence and inspiration. Students are expected to undertake a significant amount of work outside of regular class meetings. At this point in your Visual Arts Education you must be able to represent serious attention and dedication to your work, and prove that you can manage your time and energy towards advanced inquiry.

This course focuses on the additive construction methods essential to contemporary sculpture. Students will embark on independent projects that hone their skills in constructing armatures and exploring innovative skinning techniques. Throughout the term, participants will learn to build and manipulate forms using primarily additive processes, developing their own sculptural vocabulary in a studio environment. There will be two personal independent projects in this class that will ultimately converge into a dynamic, large-scale collaborative sculpture.

In this course we will focus on cutting and welding non-ferrous metals. Hand cutting and CNC assisted plasma cutting will be the methods in which stock will be cut. The fabrication processes will begin through brazing methods (acetylene) for connecting non-similar metals. There will also be instruction on pinpoint forging as well as the safe use of the blacksmithing forge in the Sculpture department. We will then advance to learning the skills involved in using the GTAW welders for non-ferrous welding.

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.

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). 

These technical applications, can lead you to a concept due to the design/practicality of said application.

Graduate Teaching Fellows in Dance are integrated into the dance program as teaching assistants. In consultation with their academic advisors and the dance faculty, MFA candidates develop an assistantship schedule of approximately ten hours weekly; the courses they develop and teach are listed in the curriculum. All Teaching Fellows bring their own professional histories and contribute their own manners of teaching.

This course is designed to assist graduate students with the research and development of their new work. The weekly format is determined with the students. In class, they show works-in-progress, try out ideas with their colleagues, and discuss issues involved in their creative processes. Though the class meets only once a week, students are expected to spend considerable time each week in active, ongoing creative research; their independent projects will be presented to the public, either formally or informally, by the end of the term.

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.