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Showing posts with label extraterrestrial civilization. Show all posts
Showing posts with label extraterrestrial civilization. Show all posts

Tuesday, July 21, 2015



SETI


Breakthrough Initiatives, a $100 million, 10-year multi-disciplinary effort to dramatically accelerate the search for intelligent life in the Universe, was announced recently by Russian billionaire Yuri Milner and Stephen Hawking. Project leaders include Martin Rees, Frank Drake, Geoff Marcy, Pete Worden, Ann Druyan, Dan Werthimer and Andrew Siemion.
 


Russian Billionaire Yuri Milner was joined at The Royal Society recently by Stephen Hawking, Martin Rees, Frank Drake, Geoff Marcy, Pete Worden and Ann Druyan to announce the unprecedented $100 million global Breakthrough Initiatives to reinvigorate the search for life in the universe.

Breakthrough Initiatives

The first of two initiatives announced, Breakthrough Listen, will be the most powerful, comprehensive and intensive scientific search ever undertaken for signs of intelligent life beyond Earth. The second, Breakthrough Message, will fund an international competition to generate messages representing humanity and planet Earth, which might one day be sent to other civilizations.

Breakthrough Listen

  • Biggest scientific search ever undertaken for signs of intelligent life beyond Earth.
  • Significant access to two of the world's most powerful telescopes – 100 Meter Robert C. Byrd Green Bank Telescope in West Virginia, USA ("Green Bank Telescope")1 and 64-metre diameter Parkes Telescope in New South Wales, Australia ("Parkes Telescope").
  • 50 times more sensitive than previous programs dedicated to SETI research.
  • Will cover 10 times more of the sky than previous programs.
  • Will scan at least 5 times more of the radio spectrum – and 100 times faster.
  • In tandem with a radio search, Automated Planet Finder Telescope at Lick Observatory in California, USA ("Lick Telescope")2 will undertake world's deepest and broadest search for optical laser transmissions.
  • Initiative will span 10 years.
  • Financial commitment is $100,000,000.
  • Unprecedented scope

The program will include a survey of the 1,000,000 closest stars to Earth. It will scan the center of our galaxy and the entire galactic plane. Beyond the Milky Way, it will listen for messages from the 100 closest galaxies. The telescopes used are exquisitely sensitive to long-distance signals, even of low or moderate power:
  • If a civilization based around one of the 1,000 nearest stars transmits to us with the power of common aircraft radar, Breakthrough Listen telescopes could detect it.
  • If a civilization transmits from the center of the Milky Way, with any more than 12 times the output of interplanetary radars we use to probe the Solar System, Breakthrough Listen telescopes could detect it.
  • From a nearby star (25 trillion miles away), Breakthrough Listen's optical search could detect a 100-watt laser (energy output of normal household light bulb).
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Open Data, Open Source, Open Platform

The program will generate vast amounts of data. All data will be open to the public. This will likely constitute the largest amount of scientific data ever made available to the public. The Breakthrough Listen team will use and develop the most powerful software for sifting and searching this flood of data.

All software will be open source. Both the software and the hardware used in the Breakthrough Listen project will be compatible with other telescopes around the world, so that they could join the search for intelligent life. As well as using the Breakthrough Listen software, scientists and members of the public will be able to add to it, developing their own applications to analyze the data.

Crowdsourced processing power

Breakthrough Listen will also be joining and supporting SETI@home, University of California, Berkeley's ground breaking distributed computing platform, with 9 million volunteers around the world donating their spare computing power to search astronomical data for signs of life. Collectively, they constitute one of the largest supercomputers in the world.

Breakthrough Message

  • International competition to create digital messages that represent humanity and planet Earth.
  • The pool of prizes will total $1,000,000.
  • Details on the competition will be announced at a later date.
  • This initiative is not a commitment to send messages. It's a way to learn about the potential languages of interstellar communication and to spur global discussion on the ethical and philosophical issues surrounding communication with intelligent life beyond Earth.

Project Leadership

  • Martin Rees, Astronomer Royal, Fellow of Trinity College; Emeritus Professor of Cosmology and Astrophysics, University of Cambridge.
  • Pete Worden, Chairman, Breakthrough Prize Foundation.
  • Frank Drake, Chairman Emeritus, SETI Institute; Professor Emeritus of Astronomy and Astrophysics, University of California, Santa Cruz; Founding Director, National Astronomy and Ionosphere Center; Former Goldwin Smith Professor of Astronomy, Cornell University.
  • Geoff Marcy, Professor of Astronomy, University of California, Berkeley; Alberts SETI Chair.
  • Ann Druyan, Creative Director of the Interstellar Message, NASA Voyager; Co-Founder and CEO, Cosmos Studios; Emmy and Peabody award winning Writer and Producer.
  • Dan Werthimer, Co-founder and chief scientist of the SETI@home project; director of SERENDIP; principal investigator for CASPER.
  • Andrew Siemion, Director, Berkeley SETI Research Center.

Milner said: "With Breakthrough Listen, we're committed to bringing the Silicon Valley approach to the search for intelligent life in the Universe. Our approach to data will be open and taking advantage of the problem-solving power of social networks."

Hawking said: "I strongly support the Breakthrough Initiatives and the search for extraterrestrial life."

Drake said: "Right now there could be messages from the stars flying right through the room, through us all. That still sends a shiver down my spine. The search for intelligent life is a great adventure. And Breakthrough Listen is giving it a huge lift."

Voyager Interstellar Message

"With Breakthrough Listen, we're committed to bringing the Silicon Valley approach to the search for intelligent life in the Universe."



"We've learned a lot in the last fifty years about how to look for signals from space. With the Breakthrough Initiatives, the learning curve is likely to bend upward significantly," he added.

Druyan said:

The Breakthrough Message competition is designed to spark the imaginations of millions, and to generate conversation about who we really are in the universe and what it is that we wish to share about the nature of being alive on Earth. Even if we don't send a single message, the act of conceptualizing one can be transformative. In creating the Voyager Interstellar Message, we strived to attain a cosmic perspective on our planet, our species and our time. It was intended for two distinct kinds of recipients - the putative extraterrestrials of distant worlds in the remote future and our human contemporaries. As we approach the Message's fortieth anniversary, I am deeply grateful for the chance to collaborate on the Breakthrough Message, for what we might discover together and in the hope that it might inform our outlook and even our conduct on this world.



SOURCE  Breakthrough Iniitiatives


By 33rd SquareEmbed


Tuesday, April 14, 2015

The Fermi Paradox - Are We The First?

 Space
The apparent contradiction between high estimates of the probability of the existence of extraterrestrial civilization and humanity's lack of contact with, or evidence for, such civilization continues as a massive survey of 100,000 galaxies has found no evidence of ET.





After searching 100,000 galaxies for signs of highly advanced extraterrestrial life, a team of scientists using observations from NASA's WISE orbiting observatory has found no evidence of advanced civilizations in them.

"The idea behind our research is that, if an entire galaxy had been colonized by an advanced spacefaring civilization, the energy produced by that civilization's technologies would be detectable in mid-infrared wavelengths  exactly the radiation that the WISE satellite was designed to detect for other astronomical purposes," said Jason T. Wright, an assistant professor of astronomy and astrophysics at the Center for Exoplanets and Habitable Worlds at Penn State University, who conceived of and initiated the research.

The research team's first paper about its Glimpsing Heat from Alien Technologies Survey (G-HAT), will be published in the Astrophysical Journal Supplement Series. Also among the team's discoveries are some mysterious new phenomena in our own Milky Way galaxy.

NASA Wise Telescope

"Whether an advanced spacefaring civilization uses the large amounts of energy from its galaxy's stars to power computers, space flight, communication, or something we can't yet imagine, fundamental thermodynamics tells us that this energy must be radiated away as heat in the mid-infrared wavelengths," Wright said. "This same basic physics causes your computer to radiate heat while it is turned on."

"These galaxies are billions of years old, which should have been plenty of time for them to have been filled with alien civilizations, if they exist. Either they don't exist, or they don't yet use enough energy for us to recognize them."


Theoretical physicist Freeman Dyson proposed in the 1960s that advanced alien civilizations beyond Earth could be detected by the telltale evidence of their mid-infrared emissions. It was not until space-based telescopes like the WISE satellite that it became possible to make sensitive measurements of this radiation emitted by objects in space.

Roger Griffith, a postbaccalaureate researcher at Penn State and the lead author of the paper, scoured almost the entire catalog of the WISE satellite's detections — nearly 100 million entries — for objects consistent with galaxies emitting too much mid-infrared radiation. He then individually examined and categorized around 100,000 of the most promising galaxy images. Wright reports, "We found about 50 galaxies that have unusually high levels of mid-infrared radiation. Our follow-up studies of those galaxies may reveal if the origin of their radiation results from natural astronomical processes, or if it could indicate the presence of a highly advanced civilization."

In any case, Wright said, the team's non-detection of any obvious alien-filled galaxies is an interesting and new scientific result. "Our results mean that, out of the 100,000 galaxies that WISE could see in sufficient detail, none of them is widely populated by an alien civilization using most of the starlight in its galaxy for its own purposes. That's interesting because these galaxies are billions of years old, which should have been plenty of time for them to have been filled with alien civilizations, if they exist. Either they don't exist, or they don't yet use enough energy for us to recognize them," Wright said.

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"This research is a significant expansion of earlier work in this area," said Brendan Mullan, director of the Buhl Planetarium at the Carnegie Science Center in Pittsburgh and a member of the G-HAT team. "The only previous study of civilizations in other galaxies looked at only 100 or so galaxies, and wasn't looking for the heat they emit. This is new ground."

Matthew Povich, an assistant professor of astronomy at Cal Poly Pomona, and a co-investigator on the project, said "Once we had identified the best candidates for alien-filled galaxies, we had to determine whether they were new discoveries that needed follow-up study, or well-known objects that had a lot of mid-infrared emission for some natural reason." Jessica Maldonado, a Cal Poly Pomona undergraduate, searched the astronomical literature for the best of the objects detected as part of the study to see which were well known and which were new to science. "Ms. Maldonado discovered that about a half dozen of the objects are both unstudied and really interesting looking," Povich said.

"When you're looking for extreme phenomena with the newest, most sensitive technology, you expect to discover the unexpected, even if it's not what you were looking for," said Steinn Sigurdsson, professor of astronomy and astrophysics at Penn State's Center for Exoplanets and Habitable Worlds and a co-investigator on the research team. "Sure enough, Roger and Jessica did find some puzzling new objects. They are almost certainly natural astronomical phenomena, but we need to study them more carefully before we can say for sure exactly what's going on."

Among the discoveries within our own Milky Way galaxy are a bright nebula around the nearby star 48 Librae, and a cluster of objects easily detected by WISE in a patch of sky that appears totally black when viewed with telescopes that detect only visible light. "This cluster is probably a group of very young stars forming inside a previously undiscovered molecular cloud, and the 48 Librae nebula apparently is due to a huge cloud of dust around the star, but both deserve much more careful study," Povich said.

"As we look more carefully at the light from these galaxies," said Wright, "we should be able to push our sensitivity to alien technology down to much lower levels, and to better distinguish heat resulting from natural astronomical sources from heat produced by advanced technologies. This pilot study is just the beginning."


SOURCE  University of Pennsylvania via EurekAlert

By 33rd SquareEmbed

Thursday, May 8, 2014

Researcher Says We Are Not Ready To Talk With E.T.

 SETI
A newly published study suggests that mankind is still not ready for contact with a supposed extraterrestrial civilization.




The project scientists at the Search for Extraterrestrial Intelligence program (SETI) are known for tracking possible extraterrestrial signals, but now they are also considering sending messages from Earth telling of our position. Now, a researcher from the University of Cádiz in Spain questions this idea in view of the results from a survey taken by students, revealing the general level of ignorance about the cosmos and the influence of religion when tackling these matters.

The study suggests that mankind is still not ready for contact with a supposed extraterrestrial civilization.

The SETI project is an initiative that began in the 1970s with funding from NASA, but that has evolved towards the collaboration of millions of Internet users for the processing of data from the Arecibo Observatory (Puerto Rico), where space tracking is carried out.

"Regarding our relation with a possible intelligent extraterrestrial life, we should not rely on moral reference points of thought, since they are heavily influenced by religion. Why should some more intelligent beings be ‘good’?"


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Now the members of this controversial project are trying to go further and not only search for extraterrestrial signs, but also actively send messages from Earth (Active SETI) to detect possible extraterrestrial civilizations. Astrophysicists, such as Stephen Hawking, have already warned of the risk that this implies for humanity, since it could favour the arrival of beings with more advanced technology and dubious intentions.

The ethical and sociological implications of this proposal have been analysed by the neuro-psychologist Gabriel G. de la Torre, professor at the University of Cádiz and participant in previous projects such as Mars 500 or space psychology topical team project financed by the European Space Agency, who wonders: “Can such a decision be taken on behalf of the whole planet? What would happen if it was successful and ‘someone’ received our signal? Are we prepared for this type of contact?”

To answer these questions, the professor sent a questionnaire to 116 American, Italian and Spanish university students. The survey assessed their knowledge of astronomy, their level of perception of the physical environment, their opinion on the place that things occupy in the cosmos, as well as religious questions – for example, “do you believe that God created the universe?” – or on the likelihood of contact with extraterrestrials.

The results, published in the journal Acta Astronautica, indicate that, as a species, humanity is still not ready for trying to actively contact a supposed extraterrestrial civilisation, since people lack knowledge and preparation. For this reason, SETI researchers are recommended in this study to look for alternative strategies.

“This pilot study demonstrates that the knowledge of the general public of a certain education level about the cosmos and our place within it is still poor. Therefore, a cosmic awareness must be further promoted – where our mind is increasingly conscious of the global reality that surrounds us – using the best tool available to us: education,” De la Torre emphasised. ”In this respect, we need a new Galileo to lead this journey”.

It was deduced from the questionnaires, which will soon be available to everyone on line, that university students and the rest of society lack awareness on many astronomical aspects, despite the enormous progress of science and technology. It also revealed that the majority of people consider these subjects according to their religious belief and that they would rely on politicians in the event of a huge global-scale crisis having to be resolved.

“Regarding our relation with a possible intelligent extraterrestrial life, we should not rely on moral reference points of thought, since they are heavily influenced by religion. Why should some more intelligent beings be ‘good’?,” added the researcher, who believes that this matter should not be monopolized by a handful of scientists: “In fact, it is a global matter with a strong ethical component in which we must all participate.”

What do you think?  Are you ready to talk to E.T.?


SOURCE  SiNC

By 33rd SquareEmbed

Wednesday, November 6, 2013


 Space
Statistical analysis of all the NASA Kepler observations have indicated to astronomers at UC Berkeley and the University of Hawaii, Manoa that one in five stars like our sun have planets about the size of Earth and a surface temperature conducive to life.




NASA’s Kepler space telescope, now crippled and its four-year mission at an end, nevertheless provided enough data to answer its main research question: How many of the 200 billion stars in our galaxy have potentially habitable planets?

Based on a statistical analysis of all the Kepler observations, astronomers at UC Berkeley and University of Hawaii, Manoa now estimate that one in five stars like the sun have planets about the size of Earth and a surface temperature conducive to life.

Given that about 20 percent of stars are sun-like, the researchers say, that amounts to several tens of billions of potentially habitable, Earth-size planets in the Milky Way Galaxy.

“When you look up at the thousands of stars in the night sky, the nearest sun-like star with an Earth-size planet in its habitable zone is probably only 12 light years away and can be seen with the naked eye. That is amazing,” said UC Berkeley graduate student Erik Petigura, who led the analysis of the Kepler data.

habitable zone

“It’s been nearly 20 years since the discovery of the first extrasolar planet around a normal star. Since then, we have learned that most stars have planets of some size orbiting them, and that Earth-size planets are relatively common in close-in orbits that are too hot for life,” said Andrew Howard, a former UC Berkeley post-doctoral fellow who is now on the faculty of the Institute for Astronomy at the University of Hawaii.

“With this result, we’ve come home, in a sense, by showing that planets like our Earth are relatively common throughout the Milky Way Galaxy.”

Petigura, Howard and Geoffrey Marcy, UC Berkeley professor of astronomy, will publish their analysis and findings this week in the online early edition of the journal Proceedings of the National Academy of Sciences.

“For NASA, this discovery is really important, because future missions will try to take an actual picture of a planet, and the size of the telescope they have to build depends on how close the nearest Earth-size planets are,” Howard said. “An abundance of planets orbiting nearby stars simplifies such follow-up missions.”
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The team cautioned that Earth-size planets in orbits about the size of Earth’s are not necessarily hospitable to life, even if they reside in the habitable zone around a star where the temperature is not too hot and not too cold.

“Some may have thick atmospheres, making it so hot at the surface that DNA-like molecules would not survive. Others may have rocky surfaces that could harbor liquid water suitable for living organisms,” Marcy said. “We don’t know what range of planet types and their environments are suitable for life.”

Last week, however, Howard, Marcy and their colleagues provided hope that many such planets actually are rocky and could support liquid water. They reported that one Earth-size planet discovered by Kepler – albeit, a planet with a likely temperature of 2,000 Kelvin, which is far too hot for life as we know it – is the same density as Earth and most likely composed of rock and iron, like Earth.

“This gives us some confidence that when we look out into the habitable zone, the planets Erik is describing may be Earth-size, rocky planets,” Howard said.

Habitable Planets Much More Common Than Previously Calculated

NASA launched the Kepler space telescope in 2009 to look for planets outside the solar system that cross in front of, or transit, their stars, which causes a slight diminution – about one hundredth of 1 percent – in the star’s brightness. From among the 150,000 stars photographed every 30 minutes for four years, NASA’s Kepler team reported more than 3,000 planet candidates. Many of these are much larger than Earth – ranging from large planets with thick atmospheres, like Neptune, to gas giants like Jupiter – or in orbits so close to their stars that they are roasted.

To sort them out, Petigura and his colleagues are using the Keck telescopes in Hawaii to obtain spectra of as many stars as possible. This will help them determine each star’s true brightness and calculate the diameter of each transiting planet, with an emphasis on Earth-diameter planets.

What distinguishes the team’s analysis from previous analyses of Kepler data is that they subjected Petigura’s planet-finding algorithms to a battery of tests in order to measure how many habitable zone, Earth-size planets they missed. Petigura actually introduced fake planets into the Kepler data in order to determine which ones his software could detect and which it couldn’t.

The field of view of the Kepler space telescope, located in the constellation Cygnus, just above the plane of the Milky Way Galaxy. Kepler made precise measurements of the brightnesses of 156,000 stars for four years.

“What we’re doing is taking a census of extrasolar planets, but we can’t knock on every door. Only after injecting these fake planets and measuring how many we actually found could we really pin down the number of real planets that we missed,” Petigura said.

“If the stars in the Kepler field are representative of stars in the solar neighborhood, … then the nearest (Earth-size) planet is expected to orbit a star that is less than 12 light-years from Earth and can be seen by the unaided eye,” the researchers wrote in their paper. “Future instrumentation to image and take spectra of these Earths need only observe a few dozen nearby stars to detect a sample of Earth-size planets residing in the habitable zones of their host stars.”


SOURCE   UC Berkeley

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Tuesday, July 16, 2013

Extraterrestrial Civilization

 
Search for Extraterrestrial Life
In a lecture earlier this year, Dr. Jeff Kuhn describes a new idea for completing a nearby extraterrestrial cosmic census and describe some of the large telescope technology that exists today to undertake it. Kuhn proposes looking for heat signatures will help us find extraterrestrial civilizations, or ETCs.




Where are the extrasterrestrial civilizations and do we have the technology to find them?

We now know that we're surrounded by habitable extrasolar planets. Even half a century ago, before we knew of any extrasolar planets, Enrico Fermi speculated that the absence of any "proof" for extraterrestrial civilization could be important new for life on Earth. This is now known as the "Fermi Paradox."

Today his query is even more compelling. In the video below, Dr. Jeff Kuhn describes a new idea for completing a nearby extraterrestrial cosmic census and describe some of the technology that exists today to undertake it.

Can Giant Telescopes Help Answer Fermi's Paradox?

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The detection of an extraterrestrial civilization (ETC), even without further communication, is important in many gnostic and practical aspects. For instance, one of the current burning issues for our civilization is surviving global climate changes because of increasing power generation.

Kuhn proposes that detecting more advanced civilizations will demonstrate a fundamental possibility that civilization can achieve a phase of sustainable global-scale power consumption.

For a half-century we have sought radio frequency evidence and, more recently, optical communications of ETCs. However, these approaches depend on finding alien transmissions, beam "leakage", or what could be called intentional electromagnetic signals from ETCs that are operating cosmic beacons.


Colossus Telescope Concept

The proposed Colossus telescope will employ a strategy for detecting an unintentional signal caused by alien planetary warming. Thanks to its large aperture and unique coronographic properties, it will be capable of detecting the thermodynamic signal from Earth-like ETC's within an interestingly large cosmic volume.

The outcome of such a dual wavelength, visible-IR, search will be largely independent of alien communication modes and will have quantifiable statistical completeness. Even a null result will help us understand the Fermi paradox, "why do we appear to be alone?"

Colossus Telescope Diagram


Detecting an ETC signal is possible with current technology but requires a telescope and sensitive detector that can measure the planet's thermal flux and its reflected optical light, while distinguishing these from the star's scattered light and the terrestrial thermal noise background. Glare from the central star comes from the terrestrial atmosphere's distorting effect on the optical wavefront and from diffraction due to telescope optics. Suppressing this noise requires highly accurate adaptive optics (AO) and a coronagraph system. These requirements are implemented in the Colossus design.

With the Colossus telescope, which Kuhn says can be built in five years with sufficient funding, we will be able to see advanced civilization heat pattern as can be seen in night lights on the Earth from space.



SOURCE  IfA Maui, The Colossus Corporation

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