The Space Sciences Laboratory (SSL) @UCBerkeley (UCB) is a preeminent university lab for space research and has participated in 50+ NASA missions since 1959.
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ALT Three UC Berkeley Space Sciences team members are edited to stand in front of a background featuring the upper edge of a planet in space. The image features details on their upcoming Reddit AMA event.
ALT A rendered image courtesy of Rocket Lab, showing the ESCAPADE mission's two identical satellites — “Blue” and “Gold” — orbiting around Mars.
ALT Photo of a Hall thruster identical to those on NASA’s Psyche operating in a vacuum chamber at JPL during tests. A ring of blue light emits a hazy stream of glowing material. The blue light is generated by xenon ions being accelerated through an electromagnetic field, which gives the spacecraft a gentle but steady acceleration. NASA/JPL-Caltech
ALT Three UC Berkeley Space Sciences team members are edited to stand in front of a background featuring the upper edge of a planet in space. The image features details on their upcoming Reddit AMA event.
ALT A rendered image courtesy of Rocket Lab, showing the ESCAPADE mission's two identical satellites — “Blue” and “Gold” — orbiting around Mars.
ALT UC Berkeley Space Sciences Lab engineers Chris Smith (left) and Bradley Pafchek (right) guide the COSI detector assembly toward its baseplate on July 08, 2026. Credit: UC Berkeley/Alan Toth
ALT John Tomisck, COSI’s principal investigator, and project systems engineer Ellen Taylor watch through a window as engineers Bradley Pafchek and Chris Smith guide the COSI detector assembly toward its baseplate on July 08, 2026. Credit: UC Berkeley/Alan Toth
ALT Engineers Bradley Pafchek and Matt Rubly examine the COSI (Compton Spectrometer and Imager) detector assembly at Space Sciences Laboratory on July 15, 2026. COSI is an upcoming mission that will measure gamma rays, the highest-energy form of light, to help scientists study energetic phenomena in the Milky Way and beyond. Credit: UC Berkeley/Alan Toth
ALT The COSI gamma-ray detector assembly rests on its baseplate on July 08, 2026. The gold part of the box is one of two thermal shields the mission will use to keep the detectors cold. Credit: UC Berkeley/Alan Toth
ALT Prof. Aziza Suleymanzade, from Berkeley Physics, delivering a presentation at the UC Berkeley Space Sciences Laboratory standing in front of a projected slideshow.
ALT Prof. Aziza Suleymanzade, from Berkeley Physics, delivering a presentation at the UC Berkeley Space Sciences Laboratory standing in front of a projected slideshow with a graphic depicting a hypothetical quantum network.
ALT Side-by-side comparison of two views of the gas giant Saturn, labeled “August 29, 2025” at the top left corner. At left is a straight-on view of Saturn, a globe with pale yellow horizontal bands at the equator and orange and pink at the mid-latitudes. Some bands towards the north and south pole have a light blue hue. There are prominent horizontal rings circling at the equator. At right, labeled “Saturn’s south pole,” the south-polar view of Saturn shows concentric bands in its atmosphere, mostly tan and orange, surrounding a dark central region that has a 10-sided outline. A small, dashed circle at the very center of the pole with an “X” inside denotes missing data.
