UC Berkeley Space Sciences Lab

UC Berkeley Space Sciences Lab The UC Berkeley Space Sciences Laboratory (SSL) designs, builds and operates NASA missions. Jones and Cornelius A. It was not until 1961, when Mr. James E.

The Laboratory began its operations in January 1960 with the appointment of its first director, Professor Samuel Silver. Starting life in a corner of the old Leuschner Observatory on the main campus, the active interest of faculty members in the space sciences led to a rapid deployment of the physical and biological research programs. The modest quarters were soon inadequate for the group of resea

rch associates and graduate students. An especially large project on space physiology initiated by Professors Hardin B. Tobias required much more space than available on campus, forcing the Laboratory to move to the Ford Assembly Building in Richmond, California, a property acquired by the University several years earlier. The space physics program directed by Professor Kinsey A. Anderson and involving experiments carried by balloons, rockets, and satellites quickly outgrew its quarters requiring a move off campus as well. The Laboratory rented a store at 2119 University Avenue, just west of the University, and converted it into a figurative beehive of research activities. At the peak of its use, the "Market" (or the "Shoe Store") as this facility was known, housed electronic shops, the machine shop, the data processing equipment, environmental test equipment, and research projects on the moon and the planets, the interplanetary medium, and the upper atmosphere of the earth. Also housed here were social scientists who were studying the physical scientists and the problems of organization and administration of research. In its early years, the National Aeronautics and Space Administration followed the policy of funding university research on an individual project basis. Webb became the Administrator of NASA, that the agency formulated a broad and far-reaching program of space research and exploration. The Office of Grants and Research Contracts instituted two programs: the Sustaining Grant Program and the Facilities Program. The Berkeley campus was one of the first universities to receive grants under these two programs. The Sustaining Grant, which provided the Space Sciences Laboratory with a core of funds for interdisciplinary research in the physical, biological, engineering, and social sciences, gave the Laboratory a foundation on which to build faculty programs and to generate new areas of graduate training through research. The grant was invaluable in developing the space sciences program on the Berkeley campus. The NASA Facilities Grant precipitated the construction of SSL's original buildings. The growth of multiple programs represented the fulfillment of one of laboratory's goals, namely to stimulate faculty and student participation in space research. But the second major objective, that of developing the multidisciplinary substance and unique character of space research, could not be realized in a physically fragmented laboratory. With the construction of the new buildings, that goal was finally achieved. The building grant was awarded by the National Aeronautics and Space Administration (NASA) in 1962 and the building dedicated on Thursday, October 27, 1966. SSL employs about 400 people in scientific, technical, and administrative positions, including professors, research scientists, students, engineers, technicians, and programmers. Most of the staff works at the Silver Laboratory and Addition building, located in a wooded site near the crest of the Berkeley hills overlooking the Berkeley campus. The rest are located in several campus departments and at Lawrence Berkeley National Laboratory. SSL has the following facilities for space related research: 1) A high bay: a 60 foot high open area with two cranes that allows assembly of large scientific instruments or payloads for high altitude balloons or spacecraft; 2) An 11-meter diameter dish antenna for communication with spacecraft, sending up commands and bringing down the data; 3) A Mission Operations Center and Science Operations Center (MOC/SOC) for the operation of spacecraft and their scientific instruments; 4) Vacuum test and calibration facilities; 5) Fabrication facilities, including five Class 1000 clean rooms, vacuum chambers, clean benches, computers, testing equipment, and electronics equipment located in the clean rooms to fabricate space instruments; 6) Five cosmochemistry labs to test lunar samples, meteorites, and other space material to assist in understanding the age of the solar system. SSL is a national leader in Science Education. Its programs include the Center for Science Education @ Space Sciences Laboratory which aims to:
• Improve teaching and learning of science, mathematics, and technology
• Facilitate and increase scientists' involvement in education and public outreach
• Increase the participation of underserved groups in space science
• Adapt space science research discoveries for broad audiences
• Provide easy and equitable access to space science resources
• Increase the scientific literacy of the general public, and the Science Education Gateway, a national consortium of scientists, museums, and educators, working together to bring the latest science to students, teachers, and the general public. SSL also has a CalSpace Center of Excellence, funded jointly by the campus, California Space Institute (a UC Multi Campus Research Unit, and SSL & UCB funds).

08/27/2026

The Solar Radio Burst Tracker project needs your help to identify solar radio bursts in Parker Solar Probe spectra. Click on the following link to learn more and volunteer. https://tinyurl.com/2mah93bp

SSL's Weijie Sun & Jiutong Zhao, along with Michigan Engineering's Ryan Dewey, analyzed MESSENGER mission data and found...
07/27/2026

SSL's Weijie Sun & Jiutong Zhao, along with Michigan Engineering's Ryan Dewey, analyzed MESSENGER mission data and found that Mercury has intermittent radiation belts. The findings could help protect the ESA - European Space Agency/JAXA(宇宙航空研究開発機構) BepiColombo mission when it reaches Mercury this year.

Scientists thought Mercury's magnetic field was disrupted by the sun too often to trap a radiation belt, but new analysis of MESSENGER data says that's not always the case.

The ESCAPADE team used its Visible and Infrared Observation System cameras to snap these incredible pictures of the Eart...
07/25/2026

The ESCAPADE team used its Visible and Infrared Observation System cameras to snap these incredible pictures of the Earth and the Moon from 363,250 miles away! 🙌 Looking forward to our close-up as Blue and Gold slingshot around the Earth this fall.

Shaosui Xu, associate research physicist at SSL, was lead author on a paper that described how Mars' localized auroras a...
07/23/2026

Shaosui Xu, associate research physicist at SSL, was lead author on a paper that described how Mars' localized auroras are generated through a similar process as those on Earth, despite Mars having no global magnetic field. “It’s incredible to be part of the team that found the answer...” said Xu.

NASA MAVEN (Mars Atmosphere and Volatile Evolution) mission scientists have uncovered a key puzzle piece in understanding certain types of auroras on Mars,

We’d like to give a shout out to Joseph Brynes, an alum of SSL’s 2025 ASSURE summer REU program, and now an awesome Cal ...
07/10/2026

We’d like to give a shout out to Joseph Brynes, an alum of SSL’s 2025 ASSURE summer REU program, and now an awesome Cal student researcher working on the Parker Solar Probe mission. We love your enthusiasm and dedication Joseph, and are honored to have you continuing your higher education journey with us! For more on SSL’s ASSURE program, which is just getting started again for 2026, please visit ssl.berkeley.edu/assure

Thanks to Dr. Nicky Fox, Associate Administrator for NASA's Science Mission Directorate, for stopping by SSL to tell us ...
07/07/2026

Thanks to Dr. Nicky Fox, Associate Administrator for NASA's Science Mission Directorate, for stopping by SSL to tell us about the latest opportunities with NASA science. We were happy to provide an update on NASA's ESCAPADE Mission, and hopefully you’ll enjoy the LEGO .

The recent FOXSI-5 mission demonstrates potential of advanced X-ray imaging and sounding rockets for solar physics.
06/11/2026

The recent FOXSI-5 mission demonstrates potential of advanced X-ray imaging and sounding rockets for solar physics.

The images collected by the FOXSI team over its five flights are demonstrating the effectiveness of their next-generation X-ray optics and proving that sounding rockets have great potential to compliment satellite missions for basic solar science.

06/10/2026

SSL project scientist Davin Larson describes the SupraThermal Ion Sensor (STIS) instrument on NOAA's SOLAR-1 spacecraft. STIS will contribute to SOLAR-1's critical monitoring of coronal mass ejections, which can disrupt satellites and ground-based infrastructure.

This was the first mission I was honored to be a part of.
06/07/2026

This was the first mission I was honored to be a part of.

June 7th - on this day in 1992, NASA's Extreme Ultraviolet Explorer (EUVE) was launched on a Delta II 6920-10 rocket out of Space Launch Complex 17A at Cape Canaveral Air Force Station.

Also known as Explorer LXVII, the 3,275 kg EUVE was built by UC Berkeley Space Sciences Lab. It was designed to operate in the extreme ultraviolet (EUV) range of the spectrum, and was used to carry out a full-sky survey, and subsequently, a deep-survey and pointed observations.

Initially planned for a mission duration of six months, EUVE operated for 8.5 years.

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