February 23 - 29, 2020: Issue 439
Breakthrough Listen Releases 2 Petabytes Of Data From SETI Survey Of Milky Way: Parkes Radio Telescope Data Collected
February 17, 2020: University of California - Berkeley
The Breakthrough Listen Initiative today (Friday, Feb. 14) released data from the most comprehensive survey yet of radio emissions from the plane of the Milky Way Galaxy and the region around its central black hole, and it is inviting the public to search the data for signals from intelligent civilisations.
At a media briefing today in Seattle as part of the annual meeting of the American Association for the Advancement of Science (AAAS), Breakthrough Listen principal investigator Andrew Siemion of the University of California, Berkeley, announced the release of nearly 2 petabytes of data, the second data dump from the four-year old search for extraterrestrial intelligence (SETI). A petabyte of radio and optical telescope data was released last June, the largest release of SETI data in the history of the field.
The data, most of it fresh from the telescope prior to detailed study from astronomers, comes from a survey of the radio spectrum between 1 and 12 gigahertz (GHz). About half of the data comes via the Parkes radio telescope in New South Wales, Australia, which, because of its location in the Southern Hemisphere, is perfectly situated and instrumented to scan the entire galactic disk and galactic centre. The telescope is part of the Australia Telescope National Facility, owned and managed by the country's national science agency, CSIRO.
The remainder of the data was recorded by the Green Bank Observatory in West Virginia, the world's largest steerable radio dish, and an optical telescope called the Automated Planet Finder, built and operated by UC Berkeley and located at Lick Observatory outside San Jose, California.
"Since Breakthrough Listen's initial data release last year, we have doubled what is available to the public," said Breakthrough Listen's lead system administrator, Matt Lebofsky. "It is our hope that these data sets will reveal something new and interesting, be it other intelligent life in the universe or an as-yet-undiscovered natural astronomical phenomenon."
The National Radio Astronomy Observatory (NRAO) and the privately-funded SETI Institute in Mountain View, California, also announced today an agreement to collaborate on new systems to add SETI capabilities to radio telescopes operated by NRAO. The first project will develop a system to piggyback on the National Science Foundation's Karl G. Jansky Very Large Array (VLA) in New Mexico and provide data to state-of-the-art digital backend equipment built by the SETI Institute.
"The SETI Institute will develop and install an interface on the VLA, permitting unprecedented access to the rich data stream continuously produced by the telescope as it scans the sky," said Siemion, who, in addition to his UC Berkeley position, is the Bernard M. Oliver Chair for SETI at the SETI Institute. "This interface will allow us to conduct a powerful, wide-area SETI survey that will be vastly more complete than any previous such search."
"As the VLA conducts its usual scientific observations, this new system will allow for an additional and important use for the data we're already collecting," said NRAO Director Tony Beasley. "Determining whether we are alone in the universe as technologically capable life is among the most compelling questions in science, and NRAO telescopes can play a major role in answering it."
"For the whole of human history, we had a limited amount of data to search for life beyond Earth. So, all we could do was speculate. Now, as we are getting a lot of data, we can do real science and, with making this data available to general public, so can anyone who wants to know the answer to this deep question," said Yuri Milner, the founder of Breakthrough Listen.
Earth transit zone survey
In releasing the new radio and optical data, Siemion highlighted a new analysis of a small subset of the data: radio emissions from 20 nearby stars that are aligned with the plane of Earth's orbit such that an advanced civilisation around those stars could see Earth pass in front of the sun (a "transit" like those focused on by NASA's Kepler space telescope). Conducted by the Green Bank Telescope, the Earth transit zone survey observed in the radio frequency range between 4 and 8 gigahertz, the so-called C-band. The data were then analyzed by former UC Berkeley undergraduate Sofia Sheikh, now a graduate student at Pennsylvania State University, who looked for bright emissions at a single radio wavelength or a narrow band around a single wavelength. She has submitted the paper to the Astrophysical Journal.
"This is a unique geometry," Sheikh said. "It is how we discovered other exoplanets, so it kind of makes sense to extrapolate and say that that might be how other intelligent species find planets, as well. This region has been talked about before, but there has never been a targeted search of that region of the sky."
While Sheikh and her team found no technosignatures of civilisation, the analysis and other detailed studies the Breakthrough Listen group has conducted are gradually putting limits on the location and capabilities of advanced civilisations that may exist in our galaxy.
Artist’s concept of a nearby civilisation signalling Earth after observing our planet crossing in front of the sun. Astronomers have now scanned 20 nearby stars in the Earth transit zone in search of such signals. (UC Berkeley image courtesy of Breakthrough Listen)
"We didn't find any aliens, but we are setting very rigorous limits on the presence of a technologically capable species, with data for the first time in the part of the radio spectrum between 4 and 8 gigahertz," Siemion said. "These results put another rung on the ladder for the next person who comes along and wants to improve on the experiment."
Sheikh noted that her mentor, Jason Wright at Penn State, estimated that if the world's oceans represented every place and wavelength we could search for intelligent signals, we have, to date, explored only a hot tub's worth of it.
"My search was sensitive enough to see a transmitter basically the same as the strongest transmitters we have on Earth, because I looked at nearby targets on purpose," Sheikh said. "So, we know that there isn't anything as strong as our Arecibo telescope beaming something at us. Even though this is a very small project, we are starting to get at new frequencies and new areas of the sky."
Beacons in the galactic centre?
The so-far analysed observations from the galactic disk and galactic centre survey were a priority for Breakthrough Listen because of the higher likelihood of observing an artificial signal from that region of dense stars. If artificial transmitters are not common in the galaxy, then searching for a strong transmitter among the billions of stars in the disk of our galaxy is the best strategy, Simeon said.
On the other hand, putting a powerful, intergalactic transmitter in the core of our galaxy, perhaps powered by the 4 million-solar-mass black hole there, might not be beyond the capabilities of a very advanced civilisation. Galactic centres may be so-called Schelling points: likely places for civilisations to meet up or place beacons, given that they cannot communicate among themselves to agree on a location.
"The galactic centre is the subject of a very specific and concerted campaign with all of our facilities because we are in unanimous agreement that that region is the most interesting part of the Milky Way galaxy," Siemion said. "If an advanced civilisation anywhere in the Milky Way wanted to put a beacon somewhere, getting back to the Schelling point idea, the galactic center would be a good place to do it. It is extraordinarily energetic, so one could imagine that if an advanced civilisation wanted to harness a lot of energy, they might somehow use the supermassive black hole that is at the center of the Milky Way galaxy."
Visit from an interstellar comet
Breakthrough Listen also released observations of the interstellar comet 2I/Borisov, which had a close encounter with the sun in December and is now on its way out of the solar system. The group had earlier scanned the interstellar rock 'Oumuamua, which passed through the center of our solar system in 2017. Neither exhibited technosignatures.
"If interstellar travel is possible, which we don't know, and if other civilizations are out there, which we don't know, and if they are motivated to build an interstellar probe, then some fraction greater than zero of the objects that are out there are artificial interstellar devices," said Steve Croft, a research astronomer with the Berkeley SETI Research Center and Breakthrough Listen. "Just as we do with our measurements of transmitters on extrasolar planets, we want to put a limit on what that number is."
Regardless of the kind of SETI search, Siemion said, Breakthrough Listen looks for electromagnetic radiation that is consistent with a signal that we know technology produces, or some anticipated signal that technology could produce, and inconsistent with the background noise from natural astrophysical events. This also requires eliminating signals from cellphones, satellites, GPS, internet, Wi-fi and myriad other human sources.
In Sheikh's case, she turned the Green Bank telescope on each star for five minutes, pointed away for another five minutes and repeated that twice more. She then threw out any signal that didn't disappear when the telescope pointed away from the star. Ultimately, she whittled an initial 1 million radio spikes down to a couple hundred, which she was able to eliminate as Earth-based human interference. The last four unexplained signals turned out to be from passing satellites.
Siemion emphasised that the Breakthrough Listen team intends to analyse all the data released to date and to do it systematically and often.
"Of all the observations we have done, probably 20% or 30% have been included in a data analysis paper," Siemion said. "Our goal is not just to analyse it 100%, but 1000% or 2000%. We want to analyze it iteratively."
Breakthrough Listen, based at UC Berkeley, is supported by a $100 million, 10-year commitment from the Breakthrough Initiatives, founded in 2015 by Yuri and Julia Milner to explore the universe, seek scientific evidence of life beyond Earth and encourage public debate from a planetary perspective.
- Data Release 2 portal
- SETI Institute and National Radio Astronomy Observatory Team Up for SETI Science at the Very Large Array
- Berkeley SETI Research Center
- Breakthrough Initiatives
- Sofia Sheikh’s website
The Very Large Array (VLA) is a collection of 27 radio antennas located at the NRAO site in Socorro, New Mexico. Each antenna in the array measures 25 meters (82 feet) in diameter and weighs about 230 tons. Credit: Alex Savello/NRAO
Leading Australian Telescopes To Get Technology Upgrades
Related News: January 17, 2020: CSIRO
CSIRO's iconic Parkes radio telescope – fondly known as 'The Dish' – will get a new receiver that will significantly increase the amount of sky it can see at any one time, enabling new science and supporting local innovation in the space sector.
The receiver is one of two projects announced today that will deliver technology enhancements for Australia's leading radio telescopes.
Australian Research Council Linkage Infrastructure, Equipment and Facilities (LIEF) grants have been awarded for the development of a new receiver for the Parkes radio telescope, and a major upgrade for the Australia Telescope Compact Array near Narrabri in NSW.
Both telescopes are owned and operated by Australia's national science agency, CSIRO, for use by astronomers in Australia and around the world.
A $1.15M LIEF grant will support a $3M project to build a sensitive receiver called a 'cryoPAF' for the Parkes radio telescope.
Once complete, the new cryoPAF will sit high above the Parkes telescope's dish surface and receive radio signals reflected up from the dish.
Its detectors will convert radio signals into electrical ones, which can be combined in different ways so that the telescope 'looks' in several different directions at once.
The cryoPAF will be cooled to -253°C to reduce 'noise' in its electrical circuits, enhancing the ability to detect weak radio signals from the cosmos at frequencies from 700 MHz to 1.9 GHz.
The grant was led by The University of Western Australia, which will coordinate construction and commissioning of the cryoPAF. CSIRO will design, build and install the instrument.
There are five further research organisations involved in the project.
Professor Lister Staveley-Smith from The University of Western Australia node of ICRAR, who led the grant application, said the cryoPAF has three times more field of view than the previous instrument, allowing quicker and more complete surveys of the sky.
"The new receiver will help astronomers to study fast radio bursts and pulsar stars, and observe hydrogen gas throughout the Universe," Professor Staveley-Smith said.
A phased-array feed or PAF is a close-packed array of radio detectors.
CSIRO has previously designed and built innovative phased-array feeds for its ASKAP telescope in Western Australia, and a test version of the cryoPAF was used successfully on the Parkes telescope in 2016.
Director of CSIRO Astronomy and Space Science, Dr Douglas Bock, said that in addition to boosting the capabilities of the Parkes telescope, the cryoPAF receiver technology had the potential to create spin-off opportunities.
"Phased arrays have found extensive use in defence radar, medical imaging and even optical laser beam steering, with emerging applications in satellite communications and telecommunications," Dr Bock said.
"Their further development at radio wavelengths has technology applications beyond radio astronomy with the potential to fuel the growth of space-related industries here in Australia."
A second LIEF grant, worth $530,000, will support a $2.6M upgrade of the Australia Telescope Compact Array.
The existing digital signal processor will be replaced with a GPU-powered processor to double the bandwidth of the telescope's signal electronics.
The project is being led by Professor Ray Norris from Western Sydney University, working closely with CSIRO and seven other university partners.
Professor Norris said the upgrade will enable Australian researchers to address major challenges in our understanding of the Universe, and make more ground-breaking discoveries, across broad areas of astrophysics.
"The upgrade will enable the telescope to study radio counterparts to gravitational wave sources, and it will enable it to make detailed observations of initial discoveries made with the Australian Square Kilometre Array Pathfinder and other Australian telescopes," Professor Norris said.
CSIRO is a leader in radio astronomy technology development, working in close partnership with astronomers who use its telescopes as well as international observatory customers.
"We've been developing specialised instrumentation for radio telescopes since the 1940s, when the field of radio astronomy first emerged, for our own and international telescopes," Dr Bock said.
"Through our close collaborations with research partners and our expertise in technology development, we'll keep the telescopes at the cutting edge of science."
CSIRO owns and operates a wide range of science-ready national research facilities and infrastructure that is used by thousands of Australian and international researchers each year. The Parkes radio telescope and Australia Telescope Compact Array are part of the Australia Telescope National Facility, which is funded by the Australian Government.