Spring 2026 Course Search

Celtic history and music from Ireland, Scotland, Bretagne, Galatia, and Cape Breton will be experienced, studied, and performed using instruments and voices. We’ll find and cross the musical bridges between regions–from the ballads of Ireland, Scotland and Wales to the Alalas of Spain, through the Scottish Gaelic speaking Highland and Islands to the dance tunes of Brittany. An end-of-term presentation will be prepared drawing on inspiration from traditional forms.

Miles Dewey Davis III (May 26, 1926 – September 28, 1991) was an American icon whose approach and innovation on the trumpet set him apart from the mainstream. Davis explored new approaches to creating and composing music. Davis was a trumpeter, bandleader, and composer. He is among the most influential and acclaimed figures in the history of jazz and 20th-century music. When you hear a Miles Davis recording, you know it's Miles. Davis's five-decade career kept him at the forefront of many major stylistic developments in jazz.

The course will be for sustained work on an animation or design project, and should be a space for both experimentation, ambition and a consistent endeavor.  Students will be expected to create a complete animation, a series of experiments, projection or interactive project.  The expectation is that students will be fully engaged in all aspects of the class from critiques, to experimenting with ideas, undertaking research and being present.

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 focus our attention on a few of the most exciting composers of the late twentieth-century, and discuss how their music has influenced the music of the current period.

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). 

Fundamentals of 2-D animation principles will be explored through drawing, from basic motion cycles to straight-ahead animation. Students will primarily work with wet/dry mediums on paper, with additional instruction in After Effects compositing workflow, and digital drawing. Weekly exercises will explore a variety of animation techniques to create short projects. While Screenings, critiques and demonstrations parallel regular viewings of student work.

This seminar course investigates the cultural, philosophical, and aesthetic dimensions of sound through critical readings, listening exercises, and discussions. Drawing from fields such as sound studies, media theory, musicology, literature, and art, Readings in Sound challenges students to consider how sound shapes experience, knowledge, identity, and space.

In this course we will be taking a hands on approach to understanding the lever harp both historically and compositionally. We will be building and stringing small 19 string harps which will be used as the basis for our compositional work where students will be creating new works of varying length for the lever harp to be presented at the end of the semester. We’ll look at what techniques are and are not achievable, what makes this instrument unique to other harps, and how to include it in larger compositional contexts.

This course introduces students to the basic language of 3D animation and modeling.  Students will be expected to become familiar with the basic principles of the MAYA program. A series of modeled objects placed in locations will be created. The emphasis will be on becoming proficient with modelling forms, texturing using Arnold Renderer, basic animation and utilizing lights and cameras.

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.