An architected material is strength-tested by stretching until failure.
Credit: Greer Group / Caltech
Close-up of the architected material tested in this study.
Credit: Greer Group / Caltech
An architected material is strength-tested by stretching until failure.
Credit: Greer Group / Caltech
Close-up of the architected material tested in this study.
Credit: Greer Group / Caltech
Richmond Wolf
David Pyott
David Tirrell (left), Harry Gray (upper right), and Bryan Hunter.
Credit: Caltech
Parsons-Gates Hall of Administration
T cells surround a cancer cell
Credit: National Institutes of Health
Credit: Courtesy of D. Assumpcao
Credit: iStock
This fancy sea slug and its ilk contain anti-cancer compounds in their bodies. Caltech’s Brian Stoltz has developed a way to create those compounds in the lab.
Credit: Wikimedia Commons
A simulated picture of two merging black holes, each about 30 solar masses. This is approximately what a human would see if they could travel in spaceship to take a closer look at merging black holes.
Credit: SXS, the Simulating eXtreme Spacetimes (SXS) project (http://www.black-holes.org)
This simulation shows the merging of a 20 solar-mass black hole with a 40 solar-mass black hole. A new model now predicts the end state of a merger with the greatest accuracy yet, including the final black hole’s spin, mass, and recoil velocity, or “kick.” The black holes’ spins are indicated with arrows—because they differ from the orbital angular momentum (pink arrow), the orbit wobbles, or precesses. The blue and red orbs indicate patterns of gravitational waves generated in the collision.
Credit: Caltech/Vijay Varma