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Tag Archives: Green Bank Telescope

From a UC Berkeley press release, July 20, 2015:

The Breakthrough Prize Foundation and its founder, internet investor Yuri Milner, have signed a contract with UC Berkeley to lead a major escalation in the search for extraterrestrial intelligence (SETI). The foundation has committed $100 million over 10 years to UC Berkeley and other participating institutions for a project called Breakthrough Listen, the most comprehensive scientific SETI project yet.

The Breakthrough Prize Foundation has already contracted with two of the world’s largest radio telescopes – the 100-meter Robert C. Byrd Green Bank Telescope in West Virginia and the 64-meter Parkes Telescope in New South Wales, Australia – to devote between 20 and 25 percent of their telescope time to searching for signals from other civilizations. The funding will also allow the Automated Planet Finder at the Lick Observatory near San Jose, CA, to search for optical laser signals from other planets.

For the Breakthrough Listen program, UC Berkeley will build high-speed digital electronics and high-bandwidth signal processing instruments to gather and analyze the radio and optical data collected by the telescopes, and will train the next generation of SETI scientists.

The program will generate vast amounts of data, all of which will be open to the public. Over time this could constitute the largest amount of scientific data ever made available to the public, according to the foundation.

Links: the full UC Berkeley press release, Breakthrough Listen homepage.


From an NRAO press release, March 9, 2015:

From earthbound optical telescopes, the surface of Venus is shrouded beneath thick clouds made mostly of carbon dioxide. To penetrate this veil, probes like NASA’s Magellan spacecraft use radar to reveal remarkable features of this planet, like mountains, craters, and volcanoes.

Credit: B. Campbell, Smithsonian, et al., NRAO/AUI/NSF, Arecibo

Credit: B. Campbell, Smithsonian, et al., NRAO/AUI/NSF, Arecibo

Recently, by combining the highly sensitive receiving capabilities of the National Science Foundation’s (NSF) Green Bank Telescope (GBT) and the powerful radar transmitter at the NSF’s Arecibo Observatory, astronomers were able to make remarkably detailed images of the surface of this planet without ever leaving Earth. The radar signals from Arecibo passed through both our planet’s atmosphere and the atmosphere of Venus, where they hit the surface and bounced back to be received by the GBT in a process known as bistatic radar.

This capability is essential to study not only the surface as it appears now, but also to monitor it for changes. By comparing images taken at different periods in time, scientists hope to eventually detect signs of active volcanism or other dynamic geologic processes that could reveal clues to Venus’s geologic history and subsurface conditions.

Links: NRAO press release.