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Six-panel sequence showing colorized simulations of star formation. Over time, swirling blue and yellow gas shapes evolve from a single star to the formation of a binary and then a five-star system. Distances are labeled in AU.

The First Stars: Formation, Properties, and Impact

Ralf Klessen, Heidelberg University

A bright spiral galaxy viewed from above in space, with a highlighted red beam pointing outward from its center and a circular marker around the galaxy鈥檚 core.

The Microlensing Planet Landscape on the Eve of Roman

Jennifer Yee, Harvard University

Colorful galaxy cluster in deep space with numerous stars, glowing clouds of purple and pink gas, and bright points of light scattered across a dark, star-filled background.

Particle Heating and Acceleration in Galaxy Clusters

Ellen Zweibel, University of Wisconsin-Madison

A woman with shoulder-length brown hair, wearing a black jacket, a black and white floral scarf, and a silver necklace, smiles in front of a light-colored brick wall.

Sackler Lecture: Einstein’s Waves: New Cosmic Sounds

One century following Einstein's prediction of spacetime disturbances and gravitational waves, the laser-enabled special detectors LIGO achieved the most accurate measurement ever made by humans across science and engineering and revealed to us the gravitational-wave signals produced by the most powerful collisions of black holes in the universe. These revolutionary discoveries have given birth to a brand new field of astronomy, a completely new way of sensing the cosmos and exploring its darkest corners. I will review the first direct detections of gravitational waves and what they can teach us about the nature of black holes and other exotic cosmic events.