Gateway Expeditions into Black Holes and Exoplanets

Gateway Expeditions into Black Holes and Exoplanets

A First-Year Ampersand Program

Explore black holes and exoplanets to uncover how space bends, planets form, and life might exist beyond Earth. 

Gateway Expeditions into Black Holes and Exoplanets introduces students to some of the most compelling questions in contemporary astrophysics. Students investigate the extreme processes close to black holes, and on the conditions that support life in other solar systems. Through accessible, concept-driven coursework and experiential learning, the program emphasizes scientific curiosity, critical thinking, and discovery—offering an engaging introduction to modern astrophysical research without requiring advanced mathematical preparation.

How to Sign Up

Signing up for a First-Year Program is a structured process designed to help match you with a program that best fits your interests. Ampersand Programs require a short essay responding to a program-specific prompt.

If you plan to rank this Ampersand Program, prepare a 250-500 word essay that responds to the following prompt: Assume you had the technology to quickly travel to exoplanets or black holes in the Universe. What questions would you ask, or what measurements would you make to better understand their properties?

Learn More About Sign-Ups

Ampersand Program Courses

Semester 1: All About Black Holes

Black holes are the Universe’s most extreme objects: they are so massive and compact that gravity bends space and time into a knot. The signature property of a black hole is that you can get in, but not out. In this first-year seminar, we discuss what is currently known about black holes, starting from Einstein’s theories about space, time, and gravity, through the first observational evidence for black holes, to the latest images of the shadows cast by black holes taken with the largest telescopes on earth.  This class is designed to bend your mind when figuring out why clocks run slower when approaching the edge of a black hole, what could be at the center of a black hole or even at the other side. At the same time, we will discuss the inner workings of the most advanced telescopes that astronomers have developed to study black holes, and the strategies astronomers employ to develop ever more sensitive instruments. Also expect a fair bit of astronomy in this class, when we discuss how black holes form, when and how they grow, and which roles they play in cosmic eco-systems such as the Milky Way Galaxy. 

Semester 2: Gateway Expeditions into Exoplanets, Physics 1210 

Discovery and characterization of planets beyond our Solar System have transformed our view of the cosmos and our home planet, Earth. These alien worlds, referred to as exoplanets, are opportune cosmic laboratories for improving our understanding of the formation of planets and the origin of life. Many of these worlds are highly dissimilar to those in our Solar System, requiring significant paradigm shifts in modeling the physical processes that govern them. In line with this rigorous exploration, exoplanet research has recently become a significant branch of astrophysics. Gateway Expeditions into Exoplanets is a new introductory, non-calculus course that provides an introduction to exoplanets, covering their formation and evolution, diverse properties, and potential to support life. 

Ampersand Program Faculty

https://physics.wustl.edu/xml/faculty_staff/20640/rss.xml
Tansu Daylan

Tansu Daylan

Assistant Professor of Physics

Dr. Tansu Daylan’s research program seeks to better understand the particle nature of dark matter and how exoplanets form, evolve, migrate, and potentially support life.

https://physics.wustl.edu/xml/faculty_staff/11854/rss.xml
Henric Krawczynski

Henric Krawczynski

Chair and Professor of Physics

​Professor Krawczynski works on experimental and theoretical astroparticle physics. His work aims at revealing the inner workings of astrophysical black holes, and using black hole and neutron star observations for testing the theory of General Relativity and the Standard Model of Particle Physics in regimes not accessible in terrestrial laboratories.