Spring 2026 Course Search

Theoretical Ethics aims to uncover the sources of moral knowledge and the foundations of moral obligation. You will engage in a detailed reading of two classical moral theories and study contemporary interpretations and applications of these theories. You will be expected to contribute substantially to class discussion, write two essays and present a draft of your final essay to the class.

Feminism imagines a world free of gender-based oppression and injustice. But what exactly does such freedom involve? In this course, we’ll investigate the interplay between gender, feminist theory, and philosophical views about freedom. Some prompting questions include: Is individual freedom enough? What does ubiquitous pornography mean for sexual freedom? How does politics shape desire? (How) should we rethink the family and work? Does feminist freedom require freedom from gender?

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.

Composers throughout the ages have cut their teeth on the study of counterpoint – the intricate practice of writing melodies for several voices sounding at once. In this course, we’ll look mainly at 16th-century composers of counterpoint, and sing through pieces from Palestrina to Weelkes, while learning to compose in a variety of practices such as canons, the motet, and familiar style. We’ll gradually work our way from two-voice to four-voice counterpoint, and set texts in a variety of harmonic styles.

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). 

In this course, students will develop skills in aural perception, learning to visualize, sing, and notate music through melodic, harmonic, and rhythmic exercises. Students will learn to identify key signatures, intervals, 7th chords, triads, key relationships, common cadences and phrase structures, larger forms, tempo markings, and more.

Hannah Arendt (1906-1975) was a political theorist whose work has become increasingly influential in recent years. A student of Martin Heidegger and Karl Jaspers, her extensive writings cover such topics as the nature of power, the meaning of the political, and the problem of revolution. This course is a detailed exploration of some of her major works, including The Human Condition, On Revolution, and Eichmann in Jerusalem: A Report on the Banality of Evil, as well as an engagement with some of the critical literature on her work.

This course is an introduction to the theory of knowledge in the analytical tradition. We will engage with topics such as skepticism about the external world, the nature of belief, truth, and justification, as well as foundationalism and coherentism,, internalism versus externalism, along with other topics.

John Rawls (1921-2003) was arguably the most important and influential political philosopher of the twentieth century. His first major work, A Theory of Justice (1971) transformed the field of political philosophy and his ideas and arguments remain at the center of the philosophical debate on the question of justice. This course consists of a careful study of the main arguments in his early and late work as well as a consideration of some of the critical literature.

The Tuning in the Trees is an advanced seminar in microtonality that treats tuning systems as both technical structures and living landscapes. Students will explore how musical intervals emerge from natural patterns—such as tree bifurcations, harmonic ratios, and number sequences—while engaging deeply with Just intonation, Meantone, Bohlen–Pierce, and other non-Western tunings.

Aristocles (known to us as "Plato") lived and wrote in Athens in the 5th c. BCE. More than 2400 years later, Alfred North Whitehead’s famous remark still resonates: “The safest general characterization of the European philosophical tradition is that it consists of a series of footnotes to Plato…the wealth of general ideas scattered through them…have made [Plato’s] writings an inexhaustible mine of suggestion” (Process and Reality, 1929).

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.