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UK To Join In On The Search For Extraterrestrial Intelligence

July 6, 2013
Image Caption: The Lovell Telescope at Jodrell Bank inspired the first proposals to search for radio signals from extraterrestrial civilizations. Credit: Anthony Holloway, University of Manchester

April Flowers for redOrbit.com – Your Universe Online

To promote academic research in the UK relating to the Search for Extraterrestrial Intelligence (SETI), a new network has been launched. Academics from 11 institutions across the UK are being brought together by the UK SETI Research Network (UKSRN), whose Patron is the Royal Astronomer, Professor Martin Rees.

The network covers a wide range of diverse topics, including potential methods for detecting signals, the linguistic challenge of deciphering messages, the probability of an extraterrestrial civilization interacting with Earth and the longevity of civilizations.

The scientists of UKSRN presented current activity and considered future strategy at the Royal Astronomical Society’s National Astronomy Meeting in St. Andrews on July 5, 2013.

“We hope that the existence of the network will excite interest from people in the UK astronomical community that have been thinking about SETI and encourage them to contribute their work. In this session at NAM, we are presenting the whole range of UK SETI activities to the community and hope that it will promote a wider understanding of, and activity in, this subject,” said Dr. Alan Penny, coordinator of UKSRN.

PROJECTS IN PROGRESS

The capability of the UK’s recently commissioned e-MERLIN array of seven radio telescopes for SETI projects was described by Dr. Tim O’Brien from The University of Manchester’s Jodrell Bank Observatory. Dr. O’Brien also reported on progress in initial test observations.

“The first proposal to search for radio signals from extraterrestrial civilizations was actually inspired by the construction of the Lovell Telescope at Jodrell Bank,” said O’Brien. “We went on to take part in the SETI Institute’s Project Phoenix from 1998 to 2003, searching for signals from about a thousand nearby stars. At that time the equipment required to sift through the data was expensive and unusual, but our modern telescopes are potentially capable of conducting these type of observations as a matter of course.”

The Lovell Telescope, an internationally known landmark in the world of astronomy at Jodrell Bank since 1957, is part of the e-Merlin array. The array is connected by optical fibers and spread over 135 miles from Jodrell Bank to Cambridge. The e-Merlin array is a multi-telescope approach offering a large potential for distinguishing true extraterrestrial signals from interference generated here on Earth, a key problem for all radio SETI projects.

“It’s early days for this new SETI work at Jodrell but we think that using e-MERLIN, and future facilities such as the Square Kilometer Array, we could make an important contribution to the search for intelligent life elsewhere in the Universe,” said O’Brien.

Dr. John Elliott, Leeds Metropolitan University, is a researcher on the nature of communication. His research includes how language structure can be identified, and methods for subsequent decipherment and dissemination. Elliot has analyzed many language systems, including 60 human languages covering all the different types of systems and many non-human communication systems, such as robots and dolphins. By understanding our analytical capabilities for communication, Elliot believes we can develop strategies for extra-terrestrial message discovery and understanding.

“Suppose SETI succeeds and we detect a technological beacon. Any message is unlikely to be written in Martian English, so standard decipherment/decryption techniques used by the military and security agencies are not going to help much. To put the challenge into context, we still have scripts from antiquity that have remained undeciphered over hundreds of years, despite many serious attempts,” said Elliott.

Elliot focuses his research on finding the unique elements of communication phenomena that make them distinguishable from other signals in the universe, regardless of the source.

“By looking beneath the surface veneer of the arbitrary sounds and symbols used, we can ‘see’ the language machine itself: its mechanisms, constraints, and evolutionary forces of efficiency and compromise that shape it. By understanding these structures, it should be possible to glean information on the intelligence of the message author,” said Elliott.

During a conversation about SETI in 1950, physicist Enrico Fermi asked, “Where is everybody?” Fermi was referencing the paradox between the high estimates for the probability of alien life and the lack of contact or evidence. This paradox remains a key area of research in the SETI field. For example, Dr. Anders Sandberg of the Future of Humanity Institute at Oxford University investigates the question of how far away in space and time a civilization could start and still have a chance of interacting with Earth today.

“If this were a very limited range, the Fermi question, “Where are they?” would be easy to answer: they couldn’t have got here yet. However, we show in our paper that, beyond a certain technological level, civilizations can spread not just across their own galaxy but across enormous intergalactic distances. This is mostly limited by how fast their devices are and the expansion of the universe. There are millions or billions of galaxies from which a civilization could have reached us, if it were established early,” said Sandberg.

The answer to Fermi’s question is more extreme than originally thought, Sandberg’s team has concluded. “If life or intelligence is rare, it must be millions or billions of times rarer; if advanced societies wipe themselves out, or decide to not go exploring, they need to converge to this outcome with extremely high probability, since it only takes one that escapes this fate to fill the universe,” said Sandberg.

Dr. Austin Gerig is a senior research fellow in Complex Networks at the University of Oxford. His work estimates that the fraction of civilizations in the universe that are long-lived and analyses the human race’s prospects for survival.

Dr Gerig said, “We know that (1) we exist and that (2) our birth number within our civilization is approximately 70 billion (i.e., approximately 70 billion people were born before us). From such little information, we can reasonably, and perhaps surprisingly, conclude that (1) many other civilizations exist and that (2) most of these civilizations are small, i.e., most will die out before producing trillions of people.”

Gerig’s team has focused on a specific consequence of this reasoning. The consequence, called the universal doomsday argument, states that long-lived civilizations must be rare because if they were not, we would find ourselves living in one.

“If most civilizations are small, then our own civilization is likely to be small, i.e., it is likely to die out within the next few centuries. Our research indicates this is the case, but that our estimates of survival are greater than previously thought using a more traditional form of the doomsday argument,” said Gerig.

Another scientist, Duncan Forgan of the Royal Observatory Edinburgh, is investigating the possibility of detecting large structures built by civilizations orbiting other stars. Researchers use what is called the transit method to detect extrasolar planets. In other words, they measure the dip in starlight as a planet passes in front of its star. Using this technique, the Kepler Space Telescope has detected a whole host of new exoplanets, and many new future telescopes and missions lined up to succeed Kepler. Forgan investigates whether a detectable difference in the shape of the lightcurve of an exoplanet transit would be made by the obstruction of the stellar disc by a large orbiting structure.

“I looked at one type of megastructure, which is essentially a very large mirror. The mirror reflects the star’s own radiation and produces thrust, much like a sail produces thrust from wind. This thrust could be used to move a civilization’s host star from its ‘natural’ orbit if it posed some harm to the civilization, for example a dangerous close approach to another star or dust cloud,” said Forgan.

Forgan’s investigations revealed that a giant mirror of this type would leave characteristic trace in the transit data of an exoplanet. This trace could be detectable with the next generation of telescopes.

“While the odds of seeing megastructures are probably very low, we will soon have a huge archive of exoplanet data to search for these objects – at no extra cost to SETI scientists. We may detect the presence, or remains, of an alien civilization that felt the need to move their star!” said Forgan.


Source: April Flowers for redOrbit.com - Your Universe Online



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