Breakthrough Listen Releases Initial Results and Data from Observations of ‘Oumuamua
Artist’s concept of interstellar asteroid 1I/2017 U1 (‘Oumuamua) as it passed through the solar system after its discovery in October 2017. The aspect ratio of up to 10:1 is unlike that of any object seen in our own solar system. (Credit: European Southern Observatory / M. Kornmesser)
SAN FRANCISCO (Breakthrough Initiatives PR) – Breakthrough Listen – the initiative to find signs of intelligent life in the universe – is reporting preliminary results and making initial data available from its observations of the “interstellar visitor” ‘Oumuamua1.
The initial block of observations (the first of a planned four blocks) ran from 3:45pm to 9:45pm ET on Wednesday, December 13, using the Breakthrough Listen backend instrument on the Robert C. Byrd Green Bank Telescope in West Virginia. Listen observed ‘Oumuamua across four radio bands (corresponding to four of the radio receivers available at Green Bank, denoted L, S, X, and C), spanning billions of individual channels across the 1 to 12 GHz range.
In addition to calibration observations, the instrument accumulated 90 TB of raw data over a 2 hour observation of ‘Oumuamua itself. A search for signals that may be of artificial origin has begun, but despite the impressive computational power of the Breakthrough Listen computing cluster at Green Bank, the large data volumes mean that this will take some time to complete.
“It is great to see data pouring in from observations of this novel and interesting source,” said Andrew Siemion, Director of Berkeley SETI Research Center. “Our team is excited to see what additional observations and analyses will reveal”.
The Breakthrough Listen “turboSETI” pipeline2 combs the data for narrow bandwidth signals that are drifting in frequency. By matching the rate at which these signals drift to the expected drift due to the motion of ‘Oumuamua (in addition to rejecting interfering signals from human technology that do not match the sky position of the primary target), the software attempts to identify any signals that might be coming from ‘Oumuamua itself.
No such signals have been detected, although the analysis is not yet complete. So far, data from the S-band receiver (covering frequencies from 1.7 to 2.6 GHz) has been processed, and analysis of the remaining three bands is ongoing. A subset of the S-band data is now available for public inspection in the Breakthrough Listen archive3, and additional data will be added as it becomes available.
The data is stored in specialized formats, and analyzing it may be challenging for non-experts. We invite those who are interested to study the tutorial material4 provided by the Breakthrough Listen science team at the University of California, Berkeley, SETI Research Center and to assist with the analysis not only of this intriguing object, but of the entire Breakthrough Listen dataset.
Breakthrough Listen is a scientific program in search for evidence of technological life in the Universe. It aims to survey one million nearby stars, the entire galactic plane and 100 nearby galaxies at a wide range of radio and optical bands.
The Breakthrough Initiatives are a suite of scientific and technological programs looking for life in the Universe.
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1 For more background information on this object, see breakthroughinitiatives.org/news/14
2 As used for the analysis of 692 stars released earlier this year, and described at seti.berkeley.edu/lband2017
2 responses to “Breakthrough Listen Releases Initial Results and Data from Observations of ‘Oumuamua”
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It would be cool if the data received from Oumuamua was found to, when displayed as points along an x-y axis, outline an E.T.-like hand flipping us the bird as it pulled away from the Sun
Well no clear signal was noted. No Narrow-channel, high power signal like AM or FM Radio.
However, it is more likely an ETI would be beaming signals back to homeworld not towards us.
So we would be looking at emissions from Computers, power systems, etc.
If i were looking for ETI i’d look for anomalous IR signal. If this object were warmer then expected, especially in one area, End or beltline, i’d be very curious to image further.
Now for the record, I find this object fascinating as an Extra-solar asteroid, I give it 1:Million that it’s an active ETI platform.
That said, interesting objects deserve serious study, and it would be well worth sending a fast mover to chase it and get some serious imagery, maybe even surface spectra. I’d love to see what condensed on it in the Void.