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Search for extraterrestrial intelligence

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"SETI" redirects here. For other uses, see SETI (disambiguation).

The search for extraterrestrial intelligence (SETI) is a collective term for scientific searches for intelligent extraterrestrial life, for example, monitoring electromagnetic radiation for signs of transmissions from civilizations on other planets.[1][2][3]

Scientific investigation began shortly after the advent of radio in the early 1900s, and focused international efforts have been ongoing since the 1980s.[4] In 2015, Stephen Hawking and Israeli billionaire Yuri Milner announced the Breakthrough Listen Project, a $100 million 10-year attempt to detect signals from nearby stars.[5]

History

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Early work

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There have been many earlier searches for extraterrestrial intelligence within the Solar System. In 1896, Nikola Tesla suggested that an extreme version of his wireless electrical transmission system could be used to contact beings on Mars.[6] In 1899, while conducting experiments at his Colorado Springs experimental station, he thought he had detected a signal from Mars since an odd repetitive static signal seemed to cut off when Mars set in the night sky. Analysis of Tesla's research has led to a range of explanations including:

  • Tesla simply misunderstood the new technology he was working with,[7]
  • that he may have been observing signals from Marconi's European radio experiments,
  • and even speculation that he could have picked up naturally occurring radio noise caused by a moon of Jupiter (Io) moving through the magnetosphere of Jupiter.[8]

In the early 1900s, Guglielmo Marconi, Lord Kelvin and David Peck Todd also stated their belief that radio could be used to contact Martians, with Marconi stating that his stations had also picked up potential Martian signals.[9][10]

On August 21–23, 1924, Mars entered an opposition closer to Earth than at any time in the century before or the next 80 years.[11] In the United States, a "National Radio Silence Day" was promoted during a 36-hour period from August 21–23, with all radios quiet for five minutes on the hour, every hour. At the United States Naval Observatory, a radio receiver was lifted 3 kilometres (1.9 miles) above the ground in a dirigible tuned to a wavelength between 8 and 9 km, using a "radio-camera" developed by Amherst College and Charles Francis Jenkins. The program was led by David Peck Todd with the military assistance of Admiral Edward W. Eberle (Chief of Naval Operations), with William F. Friedman (chief cryptographer of the United States Army), assigned to translate any potential Martian messages.[12][13]

A 1959 paper by Philip Morrison and Giuseppe Cocconi first pointed out the possibility of searching the microwave spectrum. It proposed frequencies and a set of initial targets.[14][15]

In 1960, Cornell University astronomer Frank Drake performed the first modern SETI experiment, named "Project Ozma" after the Queen of Oz in L. Frank Baum's fantasy books.[16] Drake used a radio telescope 26 metres (85 ft) in diameter at Green Bank, West Virginia, to examine the stars Tau Ceti and Epsilon Eridani near the 1.420 gigahertz marker frequency, a region of the radio spectrum dubbed the "water hole" due to its proximity to the hydrogen and hydroxyl radical spectral lines. A 400 kilohertz band around the marker frequency was scanned using a single-channel receiver with a bandwidth of 100 hertz. He found nothing of interest.

Soviet scientists took a strong interest in SETI during the 1960s and performed a number of searches with omnidirectional antennas in the hope of picking up powerful radio signals. Soviet astronomer Iosif Shklovsky wrote the pioneering book in the field, Universe, Life, Intelligence (1962), which was expanded upon by American astronomer Carl Sagan as the best-selling book Intelligent Life in the Universe (1966).[17]

In the March 1955 issue of Scientific American, John D. Kraus described an idea to scan the cosmos for natural radio signals using a flat-plane radio telescope equipped with a parabolic reflector. Within two years, his concept was approved for construction by Ohio State University. With a total of US$71,000 (equivalent to $770,232 in 2023) in grants from the National Science Foundation, construction began on an 8-hectare (20-acre) plot in Delaware, Ohio. This Ohio State University Radio Observatory telescope was called "Big Ear". Later, it began the world's first continuous SETI program, called the Ohio State University SETI program.

In 1971, NASA funded a SETI study that involved Drake, Barney Oliver of Hewlett-Packard Laboratories, and others. The resulting report proposed the construction of an Earth-based radio telescope array with 1,500 dishes known as "Project Cyclops". The price tag for the Cyclops array was US$10 billion. Cyclops was not built, but the report[18] formed the basis of much SETI work that followed.

The Wow! Signal

The Ohio State SETI program gained fame on August 15, 1977, when Jerry Ehman, a project volunteer, witnessed a startlingly strong signal received by the telescope. He quickly circled the indication on a printout and scribbled the exclamation "Wow!" in the margin. Dubbed the Wow! signal, it is considered by some to be the best candidate for a radio signal from an artificial, extraterrestrial source ever discovered, but it has not been detected again in several additional searches.[19]

On 24 May 2023, a test extraterrestrial signal, in the form of a "coded radio signal from Mars", was transmitted to radio telescopes on Earth, according to a report in The New York Times.[20]

Sentinel, META, and BETA

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In 1980, Carl Sagan, Bruce Murray, and Louis Friedman founded the U.S. Planetary Society, partly as a vehicle for SETI studies.[3]

In the early 1980s, Harvard University physicist Paul Horowitz took the next step and proposed the design of a spectrum analyzer specifically intended to search for SETI transmissions. Traditional desktop spectrum analyzers were of little use for this job, as they sampled frequencies using banks of analog filters and so were restricted in the number of channels they could acquire. However, modern integrated-circuit digital signal processing (DSP) technology could be used to build autocorrelation receivers to check far more channels. This work led in 1981 to a portable spectrum analyzer named "Suitcase SETI" that had a capacity of 131,000 narrow band channels. After field tests that lasted into 1982, Suitcase SETI was put into use in 1983 with the 26-meter (85 ft) Harvard/Smithsonian radio telescope at Oak Ridge Observatory in Harvard, Massachusetts. This project was named "Sentinel" and continued into 1985.

Even 131,000 channels were not enough to search the sky in detail at a fast rate, so Suitcase SETI was followed in 1985 by Project "META", for "Megachannel Extra-Terrestrial Assay". The META spectrum analyzer had a capacity of 8.4 million channels and a channel resolution of 0.05 hertz. An important feature of META was its use of frequency Doppler shift to distinguish between signals of terrestrial and extraterrestrial origin. The project was led by Horowitz with the help of the Planetary Society, and was partly funded by movie maker Steven Spielberg. A second such effort, META II, was begun in Argentina in 1990, to search the southern sky, receiving an equipment upgrade in 1996–1997.[21][22]

The follow-on to META was named "BETA", for "Billion-channel Extraterrestrial Assay", and it commenced observation on October 30, 1995. The heart of BETA's processing capability consisted of 63 dedicated fast Fourier transform (FFT) engines, each capable of performing a 222-point complex FFTs in two seconds, and 21 general-purpose personal computers equipped with custom digital signal processing boards. This allowed BETA to receive 250 million simultaneous channels with a resolution of 0.5 hertz per channel. It scanned through the microwave spectrum from 1.400 to 1.720 gigahertz in eight hops, with two seconds of observation per hop. An important capability of the BETA search was rapid and automatic re-observation of candidate signals, achieved by observing the sky with two adjacent beams, one slightly to the east and the other slightly to the west. A successful candidate signal would first transit the east beam, and then the west beam and do so with a speed consistent with Earth's sidereal rotation rate. A third receiver observed the horizon to veto signals of obvious terrestrial origin. On March 23, 1999, the 26-meter radio telescope on which Sentinel, META and BETA were based was blown over by strong winds and seriously damaged.[23] This forced the BETA project to cease operation.

MOP and Project Phoenix

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Sensitivity vs range for SETI radio searches. The diagonal lines show transmitters of different effective powers. The x-axis is the sensitivity of the search. The y-axis on the right is the range in light-years, and on the left is the number of Sun-like stars within this range. The vertical line labeled SS is the typical sensitivity achieved by a full sky search, such as BETA above. The vertical line labeled TS is the typical sensitivity achieved by a targeted search such as Phoenix.[24]

In 1978, the NASA SETI program had been heavily criticized by Senator William Proxmire, and funding for SETI research was removed from the NASA budget by Congress in 1981;[25] however, funding was restored in 1982, after Carl Sagan talked with Proxmire and convinced him of the program's value.[25] In 1992, the U.S. government funded an operational SETI program, in the form of the NASA Microwave Observing Program (MOP). MOP was planned as a long-term effort to conduct a general survey of the sky and also carry out targeted searches of 800 specific nearby stars. MOP was to be performed by radio antennas associated with the NASA Deep Space Network, as well as the 140-foot (43 m) radio telescope of the National Radio Astronomy Observatory at Green Bank, West Virginia and the 1,000-foot (300 m) radio telescope at the Arecibo Observatory in Puerto Rico. The signals were to be analyzed by spectrum analyzers, each with a capacity of 15 million channels. These spectrum analyzers could be grouped together to obtain greater capacity. Those used in the targeted search had a bandwidth of 1 hertz per channel, while those used in the sky survey had a bandwidth of 30 hertz per channel.

Arecibo Telescope in Puerto Rico with its 300 m (980 ft) dish was one of the world's largest filled-aperture (i.e. full dish) radio telescopes and conducted some SETI searches.

MOP drew the attention of the United States Congress, where the program met opposition[26] and canceled one year after its start.[25] SETI advocates continued without government funding, and in 1995 the nonprofit SETI Institute of Mountain View, California resurrected the MOP program under the name of Project "Phoenix", backed by private sources of funding. In 2012 it cost around $2 million per year to maintain SETI research at the SETI Institute and around 10 times that to support different SETI activities globally.[27] Project Phoenix, under the direction of Jill Tarter, was a continuation of the targeted search program from MOP and studied roughly 1,000 nearby Sun-like stars until approximately 2015.[28] From 1995 through March 2004, Phoenix conducted observations at the 64-meter (210 ft) Parkes radio telescope in Australia, the 140-foot (43 m) radio telescope of the National Radio Astronomy Observatory in Green Bank, West Virginia, and the 1,000-foot (300 m) radio telescope at the Arecibo Observatory in Puerto Rico. The project observed the equivalent of 800 stars over the available channels in the frequency range from 1200 to 3000 MHz. The search was sensitive enough to pick up transmitters with 1 GW EIRP to a distance of about 200 light-years.

Ongoing radio searches

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Microwave window as seen by a ground based system. From NASA report SP-419: SETI – the Search for Extraterrestrial Intelligence

Many radio frequencies penetrate Earth's atmosphere quite well, and this led to radio telescopes that investigate the cosmos using large radio antennas. Furthermore, human endeavors emit considerable electromagnetic radiation as a byproduct of communications such as television and radio. These signals would be easy to recognize as artificial due to their repetitive nature and narrow bandwidths. Earth has been sending radio waves from broadcasts into space for over 100 years.[29] These signals have reached over 1,000 stars, most notably Vega, Aldebaran, Barnard's Star, Sirius, and Proxima Centauri. If intelligent alien life exists on any planet orbiting these nearby stars, these signals could be heard and deciphered, even though some of the signal is garbled by the Earth's ionosphere.

Many international radio telescopes are currently[when?] being used for radio SETI searches, including the Low Frequency Array (LOFAR) in Europe, the Murchison Widefield Array (MWA) in Australia, and the Lovell Telescope in the United Kingdom.[30]

Allen Telescope Array

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Main article: Allen Telescope Array

The SETI Institute collaborated with the Radio Astronomy Laboratory at the Berkeley SETI Research Center to develop a specialized radio telescope array for SETI studies, similar to a mini-cyclops array. Formerly known as the One Hectare Telescope (1HT), the concept was renamed the "Allen Telescope Array" (ATA) after the project's benefactor, Paul Allen. Its sensitivity is designed to be equivalent to a single large dish more than 100 meters in diameter, if fully completed. Presently[when?], the array has 42 operational dishes at the Hat Creek Radio Observatory in rural northern California.[31][32]

The full array (ATA-350) is planned to consist of 350 or more offset-Gregorian radio dishes, each 6.1 meters (20 feet) in diameter. These dishes are the largest producible with commercially available satellite television dish technology. The ATA was planned for a 2007 completion date, at a cost of US$25 million. The SETI Institute provided money for building the ATA while University of California, Berkeley designed the telescope and provided operational funding. The first portion of the array (ATA-42) became operational in October 2007 with 42 antennas. The DSP system planned for ATA-350 is extremely ambitious. Completion of the full 350 element array will depend on funding and the technical results from ATA-42.

ATA-42 (ATA) is designed to allow multiple observers simultaneous access to the interferometer output at the same time. Typically, the ATA snapshot imager (used for astronomical surveys and SETI) is run in parallel with a beamforming system (used primarily for SETI).[33] ATA also supports observations in multiple synthesized pencil beams at once, through a technique known as "multibeaming". Multibeaming provides an effective filter for identifying false positives in SETI, since a very distant transmitter must appear at only one point on the sky.[34][35][36]

SETI Institute's Center for SETI Research (CSR) uses ATA in the search for extraterrestrial intelligence, observing 12 hours a day, 7 days a week. From 2007 to 2015, ATA identified hundreds of millions of technological signals. So far, all these signals have been assigned the status of noise or radio frequency interference because a) they appear to be generated by satellites or Earth-based transmitters, or b) they disappeared before the threshold time limit of ~1 hour.[37][38] Researchers in CSR are working on ways to reduce the threshold time limit, and to expand ATA's capabilities for detection of signals that may have embedded messages.[39]

Berkeley astronomers used the ATA to pursue several science topics, some of which might have transient SETI signals,[40][41][42] until 2011, when the collaboration between the University of California, Berkeley and the SETI Institute was terminated.

CNET published an article and pictures about the Allen Telescope Array (ATA) on December 12, 2008.[43][44]

In April 2011, the ATA entered an 8-month "hibernation" due to funding shortfalls. Regular operation of the ATA resumed on December 5, 2011.[45][46]

In 2012, the ATA was revitalized with a $3.6 million donation by Franklin Antonio, co-founder and Chief Scientist of QUALCOMM Incorporated.[47] This gift supported upgrades of all the receivers on the ATA dishes to have (2× to 10× over the range 1–8 GHz) greater sensitivity than before and supporting observations over a wider frequency range from 1–18 GHz, though initially the radio frequency electronics only go to 12 GHz. As of July 2013, the first of these receivers was installed and proven, with full installation on all 42 antennas being expected for June 2017. ATA is well suited to the search for extraterrestrial intelligence (SETI) and to discovery of astronomical radio sources, such as heretofore unexplained non-repeating, possibly extragalactic, pulses known as fast radio bursts or FRBs.[48][49]

SERENDIP

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Main article: SERENDIP

SERENDIP (Search for Extraterrestrial Radio Emissions from Nearby Developed Intelligent Populations) is a SETI program launched in 1979 by the Berkeley SETI Research Center.[50][51] SERENDIP takes advantage of ongoing "mainstream" radio telescope observations as a "piggy-back" or "commensal" program, using large radio telescopes including the NRAO 90m telescope at Green Bank and, formerly, the Arecibo 305m telescope. Rather than having its own observation program, SERENDIP analyzes deep space radio telescope data that it obtains while other astronomers are using the telescopes. The most recently deployed SERENDIP spectrometer, SERENDIP VI, was installed at both the Arecibo Telescope and the Green Bank Telescope in 2014–2015.[52]

Breakthrough Listen

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Main article: Breakthrough Listen

Breakthrough Listen is a ten-year initiative with $100 million funding begun in July 2015 to actively search for intelligent extraterrestrial communications in the universe, in a substantially expanded way, using resources that had not previously been extensively used for the purpose.[53][54][55][3] It has been described as the most comprehensive search for alien communications to date.[54] The science program for Breakthrough Listen is based at Berkeley SETI Research Center,[56][57] located in the Astronomy Department[58] at the University of California, Berkeley.

Announced in July 2015, the project is observing for thousands of hours every year on two major radio telescopes, the Green Bank Observatory in West Virginia, and the Parkes Observatory in Australia.[59] Previously, only about 24 to 36 hours of telescope time per year were used in the search for alien life.[54] Furthermore, the Automated Planet Finder at Lick Observatory is searching for optical signals coming from laser transmissions. The massive data rates from the radio telescopes (24 GB/s at Green Bank) necessitated the construction of dedicated hardware at the telescopes to perform the bulk of the analysis.[60] Some of the data are also analyzed by volunteers in the SETI@home volunteer computing network.[59] Founder of modern SETI Frank Drake was one of the scientists on the project's advisory committee.[61][53][54]

In October 2019, Breakthrough Listen started a collaboration with scientists from the TESS team (Transiting Exoplanet Survey Satellite) to look for signs of advanced extraterrestrial life. Thousands of new planets found by TESS will be scanned for technosignatures by Breakthrough Listen partner facilities across the globe. Data from TESS monitoring of stars will also be searched for anomalies.[62]

FAST

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Main article: Five-hundred-meter Aperture Spherical Telescope

China's 500 meter Aperture Spherical Telescope (FAST) lists detecting interstellar communication signals as part of its science mission. It is funded by the National Development and Reform Commission (NDRC) and managed by the National Astronomical observatories (NAOC) of the Chinese Academy of Sciences (CAS). FAST is the first radio observatory built with SETI as a core scientific goal.[63] FAST consists of a fixed 500 m (1,600 ft) diameter spherical dish constructed in a natural depression sinkhole caused by karst processes in the region. It is the world's largest filled-aperture radio telescope.[64] According to its website, FAST can search to 28 light-years, and is able to reach 1,400 stars. If the transmitter's radiated power were to be increased to 1,000,000 MW, FAST would be able to reach one million stars. This is compared to the former Arecibo 305 meter telescope detection distance of 18 light-years.[65]

On 14 June 2022, astronomers, working with China's FAST telescope, reported the possibility of having detected artificial (presumably alien) signals, but cautioned that further studies were required to determine if a natural radio interference may be the source.[66] More recently, on 18 June 2022, Dan Werthimer, chief scientist for several SETI-related projects, reportedly noted, "These signals are from radio interference; they are due to radio pollution from earthlings, not from E.T.".[67]

UCLA

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Since 2016, University of California Los Angeles (UCLA) undergraduate and graduate students have been participating in radio searches for technosignatures with the Green Bank Telescope. Targets include the Kepler field, TRAPPIST-1, and solar-type stars.[68] The search is sensitive to Arecibo-class transmitters located within 420 light years of Earth and to transmitters that are 1,000 times more powerful than Arecibo located within 13,000 light years of Earth.[69]

Community SETI projects

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Screen shot of the screensaver for SETI@home, a former volunteer computing project in which volunteers donated idle computer power to analyze radio signals for signs of extraterrestrial intelligence.

SETI@home

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Main article: SETI@home

The SETI@home project used volunteer computing to analyze signals acquired by the SERENDIP project.

SETI@home was conceived by David Gedye along with Craig Kasnoff and is a popular volunteer computing project that was launched by the Berkeley SETI Research Center at the University of California, Berkeley, in May 1999. It was originally funded by The Planetary Society and Paramount Pictures, and later by the state of California. The project is run by director David P. Anderson and chief scientist Dan Werthimer. Any individual could become involved with SETI research by downloading the Berkeley Open Infrastructure for Network Computing (BOINC) software program, attaching to the SETI@home project, and allowing the program to run as a background process that uses idle computer power. The SETI@home program itself ran signal analysis on a "work unit" of data recorded from the central 2.5 MHz wide band of the SERENDIP IV instrument. After computation on the work unit was complete, the results were then automatically reported back to SETI@home servers at University of California, Berkeley. By June 28, 2009, the SETI@home project had over 180,000 active participants volunteering a total of over 290,000 computers. These computers gave SETI@home an average computational power of 617 teraFLOPS.[70] In 2004 radio source SHGb02+14a set off speculation in the media that a signal had been detected but researchers noted the frequency drifted rapidly and the detection on three SETI@home computers fell within random chance.[71][72]

By 2010, after 10 years of data collection, SETI@home had listened to that one frequency at every point of over 67 percent of the sky observable from Arecibo with at least three scans (out of the goal of nine scans), which covers about 20 percent of the full celestial sphere.[73] On March 31, 2020, with 91,454 active users, the project stopped sending out new work to SETI@home users, bringing this particular SETI effort to an indefinite hiatus.[74]

SETI Net

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SETI Network was the only fully operational private search system.[75] The SETI Net station consisted of off-the-shelf, consumer-grade electronics to minimize cost and to allow this design to be replicated as simply as possible. It had a 3-meter parabolic antenna that could be directed in azimuth and elevation, an LNA that covered 100 MHz of the 1420 MHz spectrum, a receiver to reproduce the wideband audio, and a standard personal computer as the control device and for deploying the detection algorithms. The antenna could be pointed and locked to one sky location in Ra and DEC which enabling the system to integrate on it for long periods. The Wow! signal area was monitored for many long periods. All search data was collected and is available on the Internet archive.

SETI Net started operation in the early 1980s as a way to learn about the science of the search, and developed several software packages for the amateur SETI community. It provided an astronomical clock, a file manager to keep track of SETI data files, a spectrum analyzer optimized for amateur SETI, remote control of the station from the Internet, and other packages.

SETI Net went dark and was decommissioned on 2021-12-04. The collected data is available on their website.

The SETI League and Project Argus

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Founded in 1994 in response to the United States Congress cancellation of the NASA SETI program, The SETI League, Incorporated is a membership-supported nonprofit organization with 1,500 members in 62 countries. This grass-roots alliance of amateur and professional radio astronomers is headed by executive director emeritus H. Paul Shuch, the engineer credited with developing the world's first commercial home satellite TV receiver. Many SETI League members are licensed radio amateurs and microwave experimenters. Others are digital signal processing experts and computer enthusiasts.

The SETI League pioneered the conversion of backyard satellite TV dishes 3 to 5 m (10–16 ft) in diameter into research-grade radio telescopes of modest sensitivity.[76] The organization concentrates on coordinating a global network of small, amateur-built radio telescopes under Project Argus, an all-sky survey seeking to achieve real-time coverage of the entire sky.[77] Project Argus was conceived as a continuation of the all-sky survey component of the late NASA SETI program (the targeted search having been continued by the SETI Institute's Project Phoenix). There are currently 143 Project Argus radio telescopes operating in 27 countries. Project Argus instruments typically exhibit sensitivity on the order of 10−23 Watts/square metre, or roughly equivalent to that achieved by the Ohio State University Big Ear radio telescope in 1977, when it detected the landmark "Wow!" candidate signal.[78]

The name "Argus" derives from the mythical Greek guard-beast who had 100 eyes, and could see in all directions at once. In the SETI context, the name has been used for radio telescopes in fiction (Arthur C. Clarke, "Imperial Earth"; Carl Sagan, "Contact"), was the name initially used for the NASA study ultimately known as "Cyclops," and is the name given to an omnidirectional radio telescope design being developed at the Ohio State University.[79]

Optical experiments

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While most SETI sky searches have studied the radio spectrum, some SETI researchers have considered the possibility that alien civilizations might be using powerful lasers for interstellar communications at optical wavelengths.[80][81][82] The idea was first suggested by R. N. Schwartz and Charles Hard Townes in a 1961 paper published in the journal Nature titled "Interstellar and Interplanetary Communication by Optical Masers". However, the 1971 Cyclops study discounted the possibility of optical SETI, reasoning that construction of a laser system that could outshine the bright central star of a remote star system would be too difficult. In 1983, Townes published a detailed study of the idea in the United States journal Proceedings of the National Academy of Sciences,[83] which was met with interest by the SETI community.

There are two problems with optical SETI. The first problem is that lasers are highly "monochromatic", that is, they emit light only on one frequency, making it troublesome to figure out what frequency to look for.[84] However, emitting light in narrow pulses results in a broad spectrum of emission; the spread in frequency becomes higher as the pulse width becomes narrower, making it easier to detect an emission.

The other problem is that while radio transmissions can be broadcast in all directions, lasers are highly directional. Interstellar gas and dust is almost transparent to near infrared, so these signals can be seen from greater distances, but the extraterrestrial laser signals would need to be transmitted in the direction of Earth in order to be detected.[85][86]

Optical SETI supporters have conducted paper studies[87] of the effectiveness of using contemporary high-energy lasers and a ten-meter diameter mirror as an interstellar beacon. The analysis shows that an infrared pulse from a laser, focused into a narrow beam by such a mirror, would appear thousands of times brighter than the Sun to a distant civilization in the beam's line of fire. The Cyclops study proved incorrect in suggesting a laser beam would be inherently hard to see.

Such a system could be made to automatically steer itself through a target list, sending a pulse to each target at a constant rate. This would allow targeting of all Sun-like stars within a distance of 100 light-years. The studies have also described an automatic laser pulse detector system with a low-cost, two-meter mirror made of carbon composite materials, focusing on an array of light detectors. This automatic detector system could perform sky surveys to detect laser flashes from civilizations attempting contact.

Several optical SETI experiments are now in progress. A Harvard-Smithsonian group that includes Paul Horowitz designed a laser detector and mounted it on Harvard's 155-centimeter (61-inch) optical telescope. This telescope is currently being used for a more conventional star survey, and the optical SETI survey is "piggybacking" on that effort. Between October 1998 and November 1999, the survey inspected about 2,500 stars. Nothing that resembled an intentional laser signal was detected, but efforts continue. The Harvard-Smithsonian group is now working with Princeton University to mount a similar detector system on Princeton's 91-centimeter (36-inch) telescope. The Harvard and Princeton telescopes will be "ganged" to track the same targets at the same time, with the intent being to detect the same signal in both locations as a means of reducing errors from detector noise.

The Harvard-Smithsonian SETI group led by Professor Paul Horowitz built a dedicated all-sky optical survey system along the lines of that described above, featuring a 1.8-meter (72-inch) telescope. The new optical SETI survey telescope is being set up at the Oak Ridge Observatory in Harvard, Massachusetts.

The University of California, Berkeley, home of SERENDIP and SETI@home, is also conducting optical SETI searches and collaborates with the NIROSETI program. The optical SETI program at Breakthrough Listen was initially directed by Geoffrey Marcy, an extrasolar planet hunter, and it involves examination of records of spectra taken during extrasolar planet hunts for a continuous, rather than pulsed, laser signal. This survey uses the Automated Planet Finder 2.4-m telescope at the Lick Observatory, situated on the summit of Mount Hamilton, east of San Jose, California.[88] The other Berkeley optical SETI effort is being pursued by the Harvard-Smithsonian group and is being directed by Dan Werthimer of Berkeley, who built the laser detector for the Harvard-Smithsonian group. This survey uses a 76-centimeter (30-inch) automated telescope at Leuschner Observatory and an older laser detector built by Werthimer.

The SETI Institute also runs a program called 'Laser SETI' with an instrument composed of several cameras that continuously survey the entire night sky searching for millisecond singleton laser pulses of extraterrestrial origin.[89][90]

In January 2020, two Pulsed All-sky Near-infrared Optical SETI (PANOSETI) project telescopes were installed in the Lick Observatory Astrograph Dome. The project aims to commence a wide-field optical SETI search and continue prototyping designs for a full observatory. The installation can offer an "all-observable-sky" optical and wide-field near-infrared pulsed technosignature and astrophysical transient search for the northern hemisphere.[91][82]

In May 2017, astronomers reported studies related to laser light emissions from stars, as a way of detecting technology-related signals from an alien civilization. The reported studies included Tabby's Star (designated KIC 8462852 in the Kepler Input Catalog), an oddly dimming star in which its unusual starlight fluctuations may be the result of interference by an artificial megastructure, such as a Dyson swarm, made by such a civilization. No evidence was found for technology-related signals from KIC 8462852 in the studies.[92][93][94]

Quantum communications

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In a 2021 preprint, astronomer Michael Hipke described for the first time how one could search for quantum communication transmissions sent by ETI using existing telescope and receiver technology. He also provides arguments for why future searches of ETI should also target interstellar quantum communication networks.[95][96]

A 2022 paper by Arjun Berera and Jaime Calderón-Figueroa noted that interstellar quantum communication by other civilizations could be possible and may be advantageous, identifying some potential challenges and factors for detecting technosignatures. They may, for example, use X-ray photons for remotely established quantum communication and quantum teleportation as the communication mode.[97][98]

Search for extraterrestrial artifacts

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The possibility of using interstellar messenger probes in the search for extraterrestrial intelligence was first suggested by Ronald N. Bracewell in 1960 (see Bracewell probe), and the technical feasibility of this approach was demonstrated by the British Interplanetary Society's starship study Project Daedalus in 1978. Starting in 1979, Robert Freitas advanced arguments[99][100][101] for the proposition that physical space-probes are a superior mode of interstellar communication to radio signals (see Voyager Golden Record).

In recognition that any sufficiently advanced interstellar probe in the vicinity of Earth could easily monitor the terrestrial Internet, 'Invitation to ETI' was established by Allen Tough in 1996, as a Web-based SETI experiment inviting such spacefaring probes to establish contact with humanity. The project's 100 signatories includes prominent physical, biological, and social scientists, as well as artists, educators, entertainers, philosophers and futurists. H. Paul Shuch, executive director emeritus of The SETI League, serves as the project's Principal Investigator.

Inscribing a message in matter and transporting it to an interstellar destination can be enormously more energy efficient than communication using electromagnetic waves if delays larger than light transit time can be tolerated.[102] That said, for simple messages such as "hello," radio SETI could be far more efficient.[103] If energy requirement is used as a proxy for technical difficulty, then a solarcentric Search for Extraterrestrial Artifacts (SETA)[104] may be a useful supplement to traditional radio or optical searches.[105][106]

Much like the "preferred frequency" concept in SETI radio beacon theory, the Earth-Moon or Sun-Earth libration orbits[107] might therefore constitute the most universally convenient parking places for automated extraterrestrial spacecraft exploring arbitrary stellar systems. A viable long-term SETI program may be founded upon a search for these objects.

In 1979, Freitas and Valdes conducted a photographic search of the vicinity of the Earth-Moon triangular libration points L4 and L5, and of the solar-synchronized positions in the associated halo orbits, seeking possible orbiting extraterrestrial interstellar probes, but found nothing to a detection limit of about 14th magnitude.[107] The authors conducted a second, more comprehensive photographic search for probes in 1982[108] that examined the five Earth-Moon Lagrangian positions and included the solar-synchronized positions in the stable L4/L5 libration orbits, the potentially stable nonplanar orbits near L1/L2, Earth-Moon L3, and also L2 in the Sun-Earth system. Again no extraterrestrial probes were found to limiting magnitudes of 17–19th magnitude near L3/L4/L5, 10–18th magnitude for L1/L2, and 14–16th magnitude for Sun-Earth L2.

In June 1983, Valdes and Freitas used the 26 m radiotelescope at Hat Creek Radio Observatory to search for the tritium hyperfine line at 1516 MHz from 108 assorted astronomical objects, with emphasis on 53 nearby stars including all visible stars within a 20 light-year radius. The tritium frequency was deemed highly attractive for SETI work because (1) the isotope is cosmically rare, (2) the tritium hyperfine line is centered in the SETI water hole region of the terrestrial microwave window, and (3) in addition to beacon signals, tritium hyperfine emission may occur as a byproduct of extensive nuclear fusion energy production by extraterrestrial civilizations. The wideband- and narrowband-channel observations achieved sensitivities of 5–14×10−21 W/m2/channel and 0.7–2×10−24 W/m2/channel, respectively, but no detections were made.[109]

Others have speculated, that we might find traces of past civilizations in our very own Solar System, on planets like Venus or Mars, although the traces would be found most likely underground.[110][111]

Technosignatures

[edit]
See also: Technosignature and Megascale engineering

Technosignatures, including all signs of technology, are a recent avenue in the search for extraterrestrial intelligence.[112][3] Technosignatures may originate from various sources, from megastructures such as Dyson spheres[113][114] and space mirrors or space shaders[115] to the atmospheric contamination created by an industrial civilization,[116] or city lights on extrasolar planets, and may be detectable in the future with large hypertelescopes.[117]

Technosignatures can be divided into three broad categories: astroengineering projects, signals of planetary origin, and spacecraft within and outside the Solar System.

An astroengineering installation such as a Dyson sphere, designed to convert all of the incident radiation of its host star into energy, could be detected through the observation of an infrared excess from a solar analog star,[118] or by the star's apparent disappearance in the visible spectrum over several years.[119] After examining some 100,000 nearby large galaxies, a team of researchers has concluded that none of them display any obvious signs of highly advanced technological civilizations.[120][121]

Another hypothetical form of astroengineering, the Shkadov thruster, moves its host star by reflecting some of the star's light back on itself, and would be detected by observing if its transits across the star abruptly end with the thruster in front.[122] Asteroid mining within the Solar System is also a detectable technosignature of the first kind.[123]

Individual extrasolar planets can be analyzed for signs of technology. Avi Loeb of the Center for Astrophysics | Harvard & Smithsonian has proposed that persistent light signals on the night side of an exoplanet can be an indication of the presence of cities and an advanced civilization.[124][125] In addition, the excess infrared radiation[117][126] and chemicals[127][128] produced by various industrial processes or terraforming efforts[129] may point to intelligence.

Light and heat detected from planets need to be distinguished from natural sources to conclusively prove the existence of civilization on a planet. However, as argued by the Colossus team,[130] a civilization heat signature should be within a "comfortable" temperature range, like terrestrial urban heat islands, i.e., only a few degrees warmer than the planet itself. In contrast, such natural sources as wild fires, volcanoes, etc. are significantly hotter, so they will be well distinguished by their maximum flux at a different wavelength.

Other than astroengineering, technosignatures such as artificial satellites around exoplanets, particularly such in geostationary orbit, might be detectable even with today's technology and data, and would allow, similar to fossils on Earth, to find traces of extrasolar life from long ago.[131]

Extraterrestrial craft are another target in the search for technosignatures. Magnetic sail interstellar spacecraft should be detectable over thousands of light-years of distance through the synchrotron radiation they would produce through interaction with the interstellar medium; other interstellar spacecraft designs may be detectable at more modest distances.[132] In addition, robotic probes within the Solar System are also being sought with optical and radio searches.[133][134]

For a sufficiently advanced civilization, hyper energetic neutrinos from Planck scale accelerators should be detectable at a distance of many Mpc.[135]

Advances for Bio and Technosignature Detection

[edit]

A notable advancement in technosignature detection is the development of an algorithm for signal reconstruction in zero-knowledge one-way communication channels.[136] This algorithm decodes signals from unknown sources without prior knowledge of the encoding scheme, using principles from Algorithmic Information Theory to identify the geometric and topological dimensions of the encoding space. It successfully reconstructed the Arecibo message despite significant noise. The work establishes a connection between syntax and semantics in SETI and technosignature detection, enhancing fields like cryptography and Information Theory. [137]

Based on fractal theory and the Weierstrass function, a known fractal, another method authored by the same group called fractal messaging offers a framework for space-time scale-free communication. This method leverages properties of self-similarity and scale invariance, enabling spatio-temporal scale-independent and parallel infinite-frequency communication. It also embodies the concept of sending a self-encoding/self-decoding signal as a mathematical formula, equivalent to self-executable computer code that unfolds to read a message at all possible time scales and in all possible channels simultaneously.[138]

Fermi paradox

[edit]
Main article: Fermi paradox

Italian physicist Enrico Fermi suggested in the 1950s that if technologically advanced civilizations are common in the universe, then they should be detectable in one way or another. According to those who were there, Fermi either asked "Where are they?" or "Where is everybody?"[139]

The Fermi paradox is commonly understood as asking why extraterrestrials have not visited Earth,[140] but the same reasoning applies to the question of why signals from extraterrestrials have not been heard. The SETI version of the question is sometimes referred to as "the Great Silence".

The Fermi paradox can be stated more completely as follows:

The size and age of the universe incline us to believe that many technologically advanced civilizations must exist. However, this belief seems logically inconsistent with our lack of observational evidence to support it. Either (1) the initial assumption is incorrect and technologically advanced intelligent life is much rarer than we believe, or (2) our current observations are incomplete, and we simply have not detected them yet, or (3) our search methodologies are flawed and we are not searching for the correct indicators, or (4) it is the nature of intelligent life to destroy itself.

There are multiple explanations proposed for the Fermi paradox,[141] ranging from analyses suggesting that intelligent life is rare (the "Rare Earth hypothesis"), to analyses suggesting that although extraterrestrial civilizations may be common, they would not communicate with us, would communicate in a way we have not discovered yet, could not travel across interstellar distances, or destroy themselves before they master the technology of either interstellar travel or communication.

The German astrophysicist and radio astronomer Sebastian von Hoerner suggested[142] that the average duration of civilization was 6,500 years. After this time, according to him, it disappears for external reasons (the destruction of life on the planet, the destruction of only rational beings) or internal causes (mental or physical degeneration). According to his calculations, on a habitable planet (one in three million stars) there is a sequence of technological species over a time distance of hundreds of millions of years, and each of them "produces" an average of four technological species. With these assumptions, the average distance between civilizations in the Milky Way is 1,000 light years.[143][144][145]

Science writer Timothy Ferris has posited that since galactic societies are most likely only transitory, an obvious solution is an interstellar communications network, or a type of library consisting mostly of automated systems. They would store the cumulative knowledge of vanished civilizations and communicate that knowledge through the galaxy. Ferris calls this the "Interstellar Internet", with the various automated systems acting as network "servers". If such an Interstellar Internet exists, the hypothesis states, communications between servers are mostly through narrow-band, highly directional radio or laser links. Intercepting such signals is, as discussed earlier, very difficult. However, the network could maintain some broadcast nodes in hopes of making contact with new civilizations.

Although somewhat dated in terms of "information culture" arguments, not to mention the obvious technological problems of a system that could work effectively for billions of years and requires multiple lifeforms agreeing on certain basics of communications technologies, this hypothesis is actually testable (see below).

Difficulty of detection

[edit]

A significant problem is the vastness of space. Despite piggybacking on the world's most sensitive radio telescope, astronomer and initiator of SERENDIP Charles Stuart Bowyer noted the then world's largest instrument could not detect random radio noise emanating from a civilization like ours,[citation needed] which has been leaking radio and TV signals for less than 100 years.[146] For SERENDIP and most other SETI projects to detect a signal from an extraterrestrial civilization, the civilization would have to be beaming a powerful signal directly at us. It also means that Earth civilization will only be detectable within a distance of 100 light-years.[147]

Post-detection disclosure protocol

[edit]

The International Academy of Astronautics (IAA) has a long-standing SETI Permanent Study Group (SPSG, formerly called the IAA SETI Committee), which addresses matters of SETI science, technology, and international policy. The SPSG meets in conjunction with the International Astronautical Congress (IAC), held annually at different locations around the world, and sponsors two SETI Symposia at each IAC. In 2005, the IAA established the SETI: Post-Detection Science and Technology Taskgroup (chairman, Professor Paul Davies) "to act as a Standing Committee to be available to be called on at any time to advise and consult on questions stemming from the discovery of a putative signal of extraterrestrial intelligent (ETI) origin."[148]

However, the protocols mentioned apply only to radio SETI rather than for METI (Active SETI).[149] The intention for METI is covered under the SETI charter "Declaration of Principles Concerning Sending Communications with Extraterrestrial Intelligence".

In October 2000 astronomers Iván Almár and Jill Tarter presented a paper to The SETI Permanent Study Group in Rio de Janeiro, Brazil which proposed a scale (modelled after the Torino scale) which is an ordinal scale between zero and ten that quantifies the impact of any public announcement regarding evidence of extraterrestrial intelligence;[150] the Rio scale has since inspired the 2005 San Marino Scale (in regard to the risks of transmissions from Earth) and the 2010 London Scale (in regard to the detection of extraterrestrial life).[151] The Rio scale itself was revised in 2018.[152]

The SETI Institute does not officially recognize the Wow! signal as of extraterrestrial origin as it was unable to be verified, although in a 2020 tweet the organization stated that ''an astronomer might have pinpointed the host star''.[153] The SETI Institute has also publicly denied that the candidate signal Radio source SHGb02+14a is of extraterrestrial origin.[154][155] Although other volunteering projects such as Zooniverse credit users for discoveries, there is currently no crediting or early notification by SETI@Home following the discovery of a signal.

Some people, including Steven M. Greer,[156] have expressed cynicism that the general public might not be informed in the event of a genuine discovery of extraterrestrial intelligence due to significant vested interests. Some, such as Bruce Jakosky[157] have also argued that the official disclosure of extraterrestrial life may have far reaching and as yet undetermined implications for society, particularly for the world's religions.

Active SETI

[edit]
Main article: Active SETI

Active SETI, also known as messaging to extraterrestrial intelligence (METI), consists of sending signals into space in the hope that they will be detected by an alien intelligence.

Realized interstellar radio message projects

[edit]

In November 1974, a largely symbolic attempt was made at the Arecibo Observatory to send a message to other worlds. Known as the Arecibo Message, it was sent towards the globular cluster M13, which is 25,000 light-years from Earth. Further IRMs Cosmic Call, Teen Age Message, Cosmic Call 2, and A Message From Earth were transmitted in 1999, 2001, 2003 and 2008 from the Evpatoria Planetary Radar.

Debate

[edit]
See also: Active SETI § Controversy
Example of a high-resolution pictorial message to potential ETI. These messages usually contain information about the location of the solar system in the Milky Way.

Whether or not to attempt to contact extraterrestrials has attracted significant academic debate in the fields of space ethics and space policy.[158][159][160] Physicist Stephen Hawking, in his book A Brief History of Time, suggests that "alerting" extraterrestrial intelligences to our existence is foolhardy, citing humankind's history of treating its own kind harshly in meetings of civilizations with a significant technology gap, e.g., the extermination of Tasmanian aborigines. He suggests, in view of this history, that we "lay low".[161] In one response to Hawking, in September 2016, astronomer Seth Shostak sought to allay such concerns.[162] Astronomer Jill Tarter also disagrees with Hawking, arguing that aliens developed and long-lived enough to communicate and travel across interstellar distances would have evolved a cooperative and less violent intelligence. She however thinks it is too soon for humans to attempt active SETI and that humans should be more advanced technologically first but keep listening in the meantime.[163]

Criticism

[edit]
For criticism of Active SETI, see Active SETI § Controversy.

As various SETI projects have progressed, some have criticized early claims by researchers as being too "euphoric". For example, Peter Schenkel, while remaining a supporter of SETI projects, wrote in 2006 that:

[i]n light of new findings and insights, it seems appropriate to put excessive euphoria to rest and to take a more down-to-earth view [...] We should quietly admit that the early estimates—that there may be a million, a hundred thousand, or ten thousand advanced extraterrestrial civilizations in our galaxy—may no longer be tenable.[1]

Critics claim that the existence of extraterrestrial intelligence has no good Popperian criteria for falsifiability, as explained in a 2009 editorial in Nature, which said:

Seti... has always sat at the edge of mainstream astronomy. This is partly because, no matter how scientifically rigorous its practitioners try to be, SETI can't escape an association with UFO believers and other such crackpots. But it is also because SETI is arguably not a falsifiable experiment. Regardless of how exhaustively the Galaxy is searched, the null result of radio silence doesn't rule out the existence of alien civilizations. It means only that those civilizations might not be using radio to communicate.[4]

Nature added that SETI was "marked by a hope, bordering on faith" that aliens were aiming signals at us, that a hypothetical alien SETI project looking at Earth with "similar faith" would be "sorely disappointed", despite our many untargeted radar and TV signals, and our few targeted Active SETI radio signals denounced by those fearing aliens, and that it had difficulties attracting even sympathetic working scientists and government funding because it was "an effort so likely to turn up nothing".[4]

However, Nature also added, "Nonetheless, a small SETI effort is well worth supporting, especially given the enormous implications if it did succeed" and that "happily, a handful of wealthy technologists and other private donors have proved willing to provide that support".[4]

Supporters of the Rare Earth Hypothesis argue that advanced lifeforms are likely to be very rare, and that, if that is so, then SETI efforts will be futile.[164][165][166] However, the Rare Earth Hypothesis itself faces many criticisms.[166]

In 1993, Roy Mash stated that "Arguments favoring the existence of extraterrestrial intelligence nearly always contain an overt appeal to big numbers, often combined with a covert reliance on generalization from a single instance" and concluded that "the dispute between believers and skeptics is seen to boil down to a conflict of intuitions which can barely be engaged, let alone resolved, given our present state of knowledge".[167] In response, in 2012, Milan M. Ćirković, then research professor at the Astronomical Observatory of Belgrade and a research associate of the Future of Humanity Institute at the University of Oxford,[168] said that Mash was unrealistically over-reliant on excessive abstraction that ignored the empirical information available to modern SETI researchers.[169]

George Basalla, Emeritus Professor of History at the University of Delaware,[170] is a critic of SETI who argued in 2006 that "extraterrestrials discussed by scientists are as imaginary as the spirits and gods of religion or myth",[171][172] and was in turn criticized by Milan M. Ćirković[168] for, among other things, being unable to distinguish between "SETI believers" and "scientists engaged in SETI", who are often sceptical (especially about quick detection), such as Freeman Dyson and, at least in their later years, Iosif Shklovsky and Sebastian von Hoerner, and for ignoring the difference between the knowledge underlying the arguments of modern scientists and those of ancient Greek thinkers.[172]

Massimo Pigliucci, Professor of Philosophy at CUNY – City College,[173] asked in 2010 whether SETI is "uncomfortably close to the status of pseudoscience" due to the lack of any clear point at which negative results cause the hypothesis of Extraterrestrial Intelligence to be abandoned,[174] before eventually concluding that SETI is "almost-science", which is described by Milan M. Ćirković[168] as Pigliucci putting SETI in "the illustrious company of string theory, interpretations of quantum mechanics, evolutionary psychology and history (of the 'synthetic' kind done recently by Jared Diamond)", while adding that his justification for doing so with SETI "is weak, outdated, and reflecting particular philosophical prejudices similar to the ones described above in Mash[167] and Basalla[171]".[175]

Richard Carrigan, a particle physicist at the Fermi National Accelerator Laboratory near Chicago, Illinois, suggested that passive SETI could also be dangerous and that a signal released onto the Internet could act as a computer virus.[176] Computer security expert Bruce Schneier dismissed this possibility as a "bizarre movie-plot threat".[177]

Ufology

[edit]

Ufologist Stanton Friedman has often criticized SETI researchers for, among other reasons, what he sees as their unscientific criticisms of Ufology,[178][179] but, unlike SETI, Ufology has generally not been embraced by academia as a scientific field of study,[180][181] and it is usually characterized as a partial[182] or total[183][184] pseudoscience. In a 2016 interview, Jill Tarter pointed out that it is still a misconception that SETI and UFOs are related.[185] She states, "SETI uses the tools of the astronomer to attempt to find evidence of somebody else's technology coming from a great distance. If we ever claim detection of a signal, we will provide evidence and data that can be independently confirmed. UFOs—none of the above."[185] The Galileo Project headed by Harvard astronomer Avi Loeb is one of the few scientific efforts to study UFOs or UAPs.[186] Loeb criticized that the study of UAP is often dismissed and not sufficiently studied by scientists and should shift from "occupying the talking points of national security administrators and politicians" to the realm of science.[187] The Galileo Project's position after the publication of the 2021 UFO Report by the U.S. Intelligence community is that the scientific community needs to "systematically, scientifically and transparently look for potential evidence of extraterrestrial technological equipment".[188]

See also

[edit]

References

[edit]
  1. ^ a b Schenkel, Peter (May–June 2006). "SETI Requires a Skeptical Reappraisal". Skeptical Inquirer. Vol. 30, no. 3. Archived from the original on 2009-11-05. Retrieved June 28, 2009.
  2. ^ Moldwin, Mark (November 2004). "Why SETI is science and UFOlogy is not" (PDF). Skeptical Inquirer. Archived (PDF) from the original on 2022-06-21. Retrieved 2022-06-11.
  3. ^ a b c d Johnson, Steven (28 June 2017). "Greetings, E.T. (Please Don't Murder Us.)". New York Times. Archived from the original on 19 July 2018. Retrieved 28 June 2017.
  4. ^ a b c d "SETI at 50". Nature. 416 (7262): 316. 2009. Bibcode:2009Natur.461..316.. doi:10.1038/461316a. PMID 19759575. Indeed, SETI is marked by a hope, bordering on faith, that not only are there civilizations broadcasting out there, but that they are somehow intent on beaming their signals at Earth. An alien SETI project relying on a similar faith in Earth would be sorely disappointed. It's true that a random mix of radar and television signals has been expanding outwards from Earth at the speed of light for the past 70 years. But there have been only a few short-lived attempts to target radio messages at other stars – with each attempt arousing concerns over alien reprisals. Understandably, many scientists who support SETI in spirit have instead pursued astronomical targets more likely to offer positive data – and tenure. Governments have also been averse to funding an effort so likely to turn up nothing.
  5. ^ Katz, Gregory (July 20, 2015). "Searching for ET: Hawking to look for extraterrestrial intelligence". AP News. Archived from the original on July 22, 2015. Retrieved July 20, 2015.
  6. ^ Seifer, Marc J. (1996). "Martian Fever (1895–1896)". Wizard : the life and times of Nikola Tesla: biography of a genius. Secaucus, New Jersey: Carol Pub. p. 157. ISBN 978-1-55972-329-9. OCLC 33865102.
  7. ^ Spencer, John (1991). The UFO Encyclopedia. New York: Avon Books. ISBN 978-0-380-76887-5. OCLC 26211869.
  8. ^ W. Bernard Carlson, Tesla: Inventor of the Electrical Age, Princeton University Press – 2013, pp. 276–278.
  9. ^ Corum, Kenneth L.; James F. Corum (1996). Nikola Tesla and the electrical signals of planetary origin (PDF). pp. 1, 6, 14. OCLC 68193760. Archived (PDF) from the original on 2010-11-29. Retrieved 2010-08-23.
  10. ^ Brown, Michael (2005). "Radio Mars: The Transformation of Marconi's Popular Image, 1919–1922". In Winn, J. Emmett; Brinson, Susan (eds.). Transmitting the past: historical and cultural perspectives on broadcasting. University of Alabama Press. ISBN 0-8173-1453-9. OCLC 56198770.
  11. ^ Lasker, Jacques. "A Primer on Mars Oppositions". Archived from the original on 2011-11-13. Retrieved 2014-01-01.
  12. ^ Dick, Steven (1999). The Biological Universe: The Twentieth Century Extraterrestrial Life Debate. Cambridge University Press. ISBN 978-0-521-34326-8.
  13. ^ Prepare for Contact Archived 2018-10-21 at the Wayback Machine. Letters of Note (2009-11-06). Retrieved on 2011-10-14.
  14. ^ Cocconi, Giuseppe & Philip Morrison (1959). "Searching for interstellar communications". Nature. 184 (4690): 844–846. Bibcode:1959Natur.184..844C. doi:10.1038/184844a0. S2CID 4220318. Archived from the original on 2008-05-09. Retrieved 2012-07-03.
  15. ^ "Cosmic Search Vol. 1, No. 1". Archived from the original on 23 October 2008. Retrieved 1 October 2014.
  16. ^ "Science: Project Ozma – TIME". 2011-02-20. Archived from the original on 2011-02-20. Retrieved 2023-10-06.
  17. ^ Sagan, Carl; Shklovskii, Iosif (1966). Intelligent Life in the Universe. Pan Books. ISBN 978-0-330-25125-9.
  18. ^ "Project Cyclops: A Design Study of a System for Detecting Extraterrestrial Intelligent Life" (PDF). NASA. 1971. Archived from the original (PDF) on September 20, 2015. Retrieved October 12, 2014.
  19. ^ Gray, Robert H. (2012). The Elusive WOW: Searching for Extraterrestrial Intelligence. Chicago, Illinois: Palmer Square Press. ISBN 978-0-9839584-4-4.
  20. ^ Overbye, Dennis (24 May 2023). "This Is Not an Extraterrestrial Signal. This Is Just a Test. – You too could be Jodie Foster as astronomers organize a practice run in communicating with aliens". The New York Times. Archived from the original on 24 May 2023. Retrieved 24 May 2023.
  21. ^ Lemarchand, Guillermo. "Progress in the Search for Ultra-Narrow Band Extraterrestrial Arti cial Signals from Argentina" (PDF). Argentina en el Proyecto SETI.
  22. ^ Lemarchand, Guillermo. "15 Years Developing SETI from a Developing Country" (PDF). Argentina en el Proyecto SETI.
  23. ^ MacRobert, Alan M. (29 March 2009). "SETI Searches Today". Sky and Telescope. Archived from the original on 16 April 2021. Retrieved 16 April 2021.
  24. ^ Wolfe, J. H.; et al. (1979). "CP-2156, Chapter 5.5. SETI – The Search for Extraterrestrial Intelligence: Plans and Rationale". NASA. Archived from the original on September 16, 2009. Retrieved July 1, 2009.
  25. ^ a b c Garber, S. J. (1999). "Searching for Good Science – the Cancellation of NASA's SETI Program". Journal of the British Interplanetary Society. 52 (1): 3. Bibcode:1999JBIS...52....3G.
  26. ^ "Ear to the Universe Is Plugged by Budget Cutters". The New York Times. October 7, 1993. Archived from the original on May 12, 2013. Retrieved May 23, 2010.
  27. ^ "Searching for Intelligent Aliens: Q&A with SETI Astronomer Jill Tarter". Space.com. May 22, 2012. Archived from the original on August 14, 2012. Retrieved August 5, 2012.
  28. ^ Shostak, Seth (2021). "Project Phoenix". SETI Institute.
  29. ^ "How Far Radio Signals have travelled". Science Alert. Jan 20, 2021. Archived from the original on January 26, 2021. Retrieved Jan 20, 2021.
  30. ^ Siemion, Andrew (September 29, 2015). "Prepared Statement by Andrew Siemion – Hearing on Astrobiology Status Report – House Committee on Science, Space, and Technology". SpaceRef.com. Archived from the original on October 23, 2015. Retrieved October 19, 2015.
  31. ^ "Allen Telescope Array General Overview". SETI Institute. Archived from the original on 2006-04-28. Retrieved 2006-06-12.
  32. ^ Welch, Jack; et al. (August 2009). "The Allen Telescope Array: The First Widefield, Panchromatic, Snapshot Radio Camera for Radio Astronomy and SETI". Proceedings of the IEEE. 97 (8): 1438–1447. arXiv:0904.0762. Bibcode:2009IEEEP..97.1438W. doi:10.1109/JPROC.2009.2017103. S2CID 7486677.
  33. ^ Gutierrez-Kraybill, Colby; et al. (2010). "Commensal observing with the Allen Telescope array: Software command and control". In Radziwill, Nicole M.; Bridger, Alan (eds.). Proceedings of the SPIE. Software and Cyberinfrastructure for Astronomy. Vol. 7740. pp. 77400Z. arXiv:1010.1567. Bibcode:2010SPIE.7740E..0ZG. doi:10.1117/12.857860. S2CID 119183681.
  34. ^ Harp, G. R. "Customized beam forming at the Allen Telescope Array." ATA Memo Series 51 (2002), available at http://www.seti.org/sites/default/files/ATA-memo-series/memo51.pdf Archived 2015-09-24 at the Wayback Machine.
  35. ^ Barott, William C.; et al. (2011). "Real-time beamforming using high-speed FPGAs at the Allen Telescope Array". Radio Science. 46 (1): n/a. Bibcode:2011RaSc...46.1016B. doi:10.1029/2010RS004442. Archived from the original on 2019-12-21. Retrieved 2019-09-20.
  36. ^ Harp, G. R. (2013). "Using Multiple Beams to Distinguish Radio Frequency Interference from SETI Signals". Radio Science. 40 (5): n/a. arXiv:1309.3826. Bibcode:2005RaSc...40.5S18H. doi:10.1029/2004RS003133. S2CID 117428022.
  37. ^ Tarter, Jill; et al. (2011). "The first SETI observations with the Allen telescope array". Acta Astronautica. 68 (3–4): 340–346. Bibcode:2011AcAau..68..340T. doi:10.1016/j.actaastro.2009.08.014.
  38. ^ Backus, Peter R.; Allen Telescope Array Team (2010). "The ATA Galactic Center Survey: SETI Observations in 2009". American Astronomical Society. 215: 403.02. Bibcode:2010AAS...21540302B.
  39. ^ Harp, Gerald R., et al. A new class of SETI beacons that contain information. Communication with Extraterrestrial Intelligence. State University of New York Press, 2011.
  40. ^ Croft, Steve; et al. (2010). "The Allen Telescope Array Twenty-Centimeter Survey—A 690 Deg2, 12 Epoch Radio Data Set. I. Catalog and Long-Duration Transient Statistics". The Astrophysical Journal. 719 (1): 45–58. arXiv:1006.2003. Bibcode:2010ApJ...719...45C. doi:10.1088/0004-637X/719/1/45. S2CID 118641366.
  41. ^ Siemion, Andrew P. V.; et al. (2012). "The Allen Telescope Array Fly's Eye Survey for Fast Radio Transients". The Astrophysical Journal. 744 (2): 109. arXiv:1109.2659. Bibcode:2012ApJ...744..109S. doi:10.1088/0004-637X/744/2/109. S2CID 118713622.
  42. ^ Siemion, Andrew; et al. (2011). "Results from the Fly's Eye Fast Radio Transient Search at the Allen Telescope Array". American Astronomical Society. 217: 240.06. Bibcode:2011AAS...21724006S.
  43. ^ Terdiman, Daniel. (2008-12-12) SETI's large-scale telescope scans the skies | Geek Gestalt – CNET News Archived 2014-02-01 at the Wayback Machine. News.cnet.com. Retrieved on 2011-10-14.
  44. ^ Rendering of 350 image – Photos: Searching the heavens for life – CNET News. News.cnet.com (2008-12-12). Retrieved on 2011-10-14.
  45. ^ The Great Beyond. Nature Blogs, ed. (25 April 2011). "SETI scope suspends search". Archived from the original on 2 May 2011. Retrieved 26 April 2011.
  46. ^ "SETI Search Resumes at Allen Telescope Array". SETI Institute. Archived from the original on 2011-12-08. Retrieved 2019-07-24.
  47. ^ Arthur, Damon. "New Hat Creek receivers will let SETI delve deeper into space". Archived from the original on 2014-03-30.
  48. ^ Siemion, Andrew P. V.; Bower, Geoffrey C.; Foster, Griffin; McMahon, Peter L.; Wagner, Mark I.; Werthimer, Dan; Backer, Don; Cordes, Jim; van Leeuwen, Joeri (2011-12-20). "The Allen Telescope Array Fly's Eye Survey for Fast Radio Transients". The Astrophysical Journal. 744 (2): 109. arXiv:1109.2659. doi:10.1088/0004-637x/744/2/109. ISSN 0004-637X. S2CID 118713622.
  49. ^ Harp, G. R.; Richards, Jon; Tarter, Jill C.; Dreher, John; Jordan, Jane; Shostak, Seth; Smolek, Ken; Kilsdonk, Tom; Wilcox, Bethany R.; Wimberly, M. K. R.; Ross, John; Barott, W. C.; Ackermann, R. F.; Blair, Samantha (2016-11-22). "Seti Observations of Exoplanets with the Allen Telescope Array". The Astronomical Journal. 152 (6): 181. arXiv:1607.04207. Bibcode:2016AJ....152..181H. doi:10.3847/0004-6256/152/6/181. ISSN 1538-3881. S2CID 118561727.
  50. ^ "SERENDIP". UC Berkeley. Archived from the original on 2017-07-09. Retrieved 2006-08-20.
  51. ^ Werthimer, Dan; Anderson, David; Bowyer, C. Stuart; Cobb, Jeff; Heien, Eric; Korpela, Eric J.; Lampton, Michael L.; Lebofsky, Matt; Marcy, Geoff W.; McGarry, Meghan; Treffers, Dick (2001-08-03). Kingsley, Stuart A.; Bhathal, Ragbir (eds.). "Berkeley radio and optical SETI programs: SETI@home, SERENDIP, and SEVENDIP". The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum III. 4273. SPIE: 104–109. Bibcode:2001SPIE.4273..104W. doi:10.1117/12.435384. S2CID 122003925.
  52. ^ "Mid June Update (Jun 23 2015)". setiathome.berkeley.edu. Retrieved 2023-02-01.
  53. ^ a b Feltman, Rachel (20 July 2015). "Stephen Hawking announces $100 million hunt for alien life". Washington Post. Archived from the original on 22 July 2015. Retrieved 20 July 2015.
  54. ^ a b c d Merali, Zeeya (2015). "Search for extraterrestrial intelligence gets a $100-million boost". Nature. 523 (7561): 392–3. Bibcode:2015Natur.523..392M. doi:10.1038/nature.2015.18016. PMID 26201576.
  55. ^ Rundle, Michael (20 July 2015). "$100m Breakthrough Listen is 'largest ever' search for alien civilisations". Wired UK. Archived from the original on 22 July 2015. Retrieved 20 July 2015.
  56. ^ "Berkeley SETI". seti.berkeley.edu. Archived from the original on 2017-09-24. Retrieved 2017-09-21.
  57. ^ "Breakthrough Initiatives". breakthroughinitiatives.org. Archived from the original on 2017-09-30. Retrieved 2017-09-21.
  58. ^ "Breakthrough Listen Initiative – News from Department of Astronomy". astro.berkeley.edu. Archived from the original on 2017-09-09. Retrieved 2017-09-21.
  59. ^ a b Sample, Ian (20 July 2015). "Anybody out there? $100m radio wave project to scan far regions for alien life". The Guardian. Archived from the original on 20 July 2015. Retrieved 20 July 2015.
  60. ^ MacMahon, David H. E.; Price, Danny C.; Lebofsky, Matthew; Siemion, Andrew P. V.; Croft, Steve; DeBoer, David; Enriquez, J. Emilio; Gajjar, Vishal; Hellbourg, Gregory (2017-07-19). "The Breakthrough Listen Search for Intelligent Life: A Wideband Data Recorder System for the Robert C. Byrd Green Bank Telescope". Publications of the Astronomical Society of the Pacific. 130 (986): 044502. arXiv:1707.06024. Bibcode:2018PASP..130d4502M. doi:10.1088/1538-3873/aa80d2. S2CID 59378232.
  61. ^ "Breakthrough Initiatives". breakthroughinitiatives.org. Archived from the original on 2017-09-04. Retrieved 2017-09-22.
  62. ^ "Breakthrough Initiatives". breakthroughinitiatives.org. Archived from the original on 2019-11-09. Retrieved 2019-11-12.
  63. ^ "What Happens If China Makes First Contact?". The Atlantic. 8 November 2017. Archived from the original on 5 June 2018. Retrieved 5 June 2018.
  64. ^ Brinks, Elias (11 July 2016). "China Opens the Aperture to the Cosmos". The Conversation. U.S. News & World Report. Archived from the original on 26 August 2016. Retrieved 12 August 2016.
  65. ^ "Science SETI, FAST website". Archived from the original on 2017-10-17. Retrieved 2017-02-19.
  66. ^ Byrd, Deborah (4 June 2022). "Has China's FAST telescope detected alien intelligence?". Earth & Sky. Archived from the original on 15 June 2022. Retrieved 15 June 2022.
  67. ^ Overbye, Dennis (18 June 2022). "A Chinese Telescope Did Not Find an Alien Signal. The Search Continues. China's astronomers have been initiated into the search for extraterrestrial intelligence with the kind of false alarm that others in the field have experienced for decades". The New York Times. Archived from the original on 16 January 2023. Retrieved 19 June 2022.
  68. ^ "Researchers Just Scanned 14 Worlds From the Kepler Mission for "Technosignatures", Evidence of Advanced Civilizations". Universe Today. 9 February 2018. Archived from the original on 2018-02-10. Retrieved 2020-05-02.
  69. ^ Margot, Jean-Luc; Greenberg, Adam H.; Pinchuk, Pavlo; Shinde, Akshay; Alladi, Yashaswi; MN, Srinivas Prasad; Bowman, M. Oliver; Fisher, Callum; Gyalay, Szilard; McKibbin, Willow; Miles, Brittany; Nguyen, Donald; Power, Conor; Ramani, Namrata; Raviprasad, Rashmi; Santana, Jesse; Lynch, Ryan S. (25 April 2018). "A Search for Technosignatures from 14 Planetary Systems in the Field with the Green Bank Telescope at 1.15–1.73 GHz". The Astronomical Journal. 155 (5): 209. arXiv:1802.01081. Bibcode:2018AJ....155..209M. doi:10.3847/1538-3881/aabb03. S2CID 13710050.
  70. ^ de Zutter, Willy. "SETI@home – Credit Overview". BOINCstats. Archived from the original on December 15, 2009. Retrieved June 28, 2009.
  71. ^ Whitehouse, David (2004-09-02). "Astronomers deny ET signal report". BBC News. Archived from the original on 2006-06-15. Retrieved 24 April 2013.
  72. ^ Alexander, Amir (2004-09-02). "SETI@home Leaders Deny Reports of Likely Extraterrestrial Signal". The Planetary Society. Archived from the original on 2011-07-26. Retrieved 2006-06-12.
  73. ^ Alan M. MacRobert. "SETI Searches Today" Archived 2014-01-03 at the Wayback Machine. Sky and Telescope (2010?).
  74. ^ Overbye, Dennis (2020-03-23). "The Search for E.T. Goes on Hold, for Now". The New York Times. ISSN 0362-4331. Archived from the original on 2020-04-07. Retrieved 2020-03-23.
  75. ^ "Searching For Extraterrestrial Intelligence (SETI) with a HackRF". rtl-sdr.com. 2020-11-27. Archived from the original on 2022-05-29. Retrieved 2022-05-30.
  76. ^ Chown, Marcus (April 1997). "The Alien Spotters". New Scientist: 28. Archived from the original on 2023-01-16. Retrieved 2008-04-13.
  77. ^ Shuch, H. Paul. "The SETI League, Inc.: Project Argus". Archived from the original on 2014-12-29. Retrieved 2014-12-30.
  78. ^ "Project Argus and the Challenge of Real-Time All-Sky SETI". www.setileague.org. Archived from the original on 2019-11-28. Retrieved 2019-12-13.
  79. ^ Shostak, Seth (2006-07-19). "The Future of SETI". Sky & Telescope. Archived from the original on 2019-05-24. Retrieved 2019-12-13.
  80. ^ Kingsley, Stuart A. (1993-08-06). "The search for extraterrestrial intelligence (SETI) in the optical spectrum: A review". In Kingsley, Stuart A (ed.). The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum. Vol. 1867. SPIE. pp. 75–113. doi:10.1117/12.150129. S2CID 119615013. {{cite book}}: |journal= ignored (help)
  81. ^ Schuetz, Marlin; Vakoch, Douglas A.; Shostak, Seth; Richards, Jon (2016-06-24). "Optical Seti Observations of the Anomalous Star Kic 8462852". The Astrophysical Journal. 825 (1): L5. arXiv:1512.02388. Bibcode:2016ApJ...825L...5S. doi:10.3847/2041-8205/825/1/l5. ISSN 2041-8213. S2CID 119194869.
  82. ^ a b Wright, Shelley A.; Horowitz, Paul; Maire, Jérôme; Chaim-Weismann, Samuel A.; Cosens, Maren; Drake, Frank D.; Howard, Andrew W.; Marcy, Geoffrey W.; Siemion, Andrew P. V.; Stone, Remington P. S.; Treffers, Richard R.; Uttamchandani, Avinash; Werthimer, Dan (2018-07-23). "Panoramic optical and near-infrared SETI instrument: Overall specifications and science program". In Simard, Luc; Evans, Christopher J; Takami, Hideki (eds.). Ground-based and Airborne Instrumentation for Astronomy VII. Vol. 10702. SPIE. p. 201. arXiv:1808.05772. Bibcode:2018SPIE10702E..5IW. doi:10.1117/12.2314268. ISBN 9781510619579. S2CID 55939829.
  83. ^ Townes, C. H. (1983). "At what wavelengths should we search for signals from extraterrestrial intelligence?". Proceedings of the National Academy of Sciences. 80 (4): 1147–1151. Bibcode:1983PNAS...80.1147T. doi:10.1073/pnas.80.4.1147. PMC 393547. PMID 16593279.
  84. ^ Marcy, Geoffrey W.; Tellis, Nathaniel K.; Wishnow, Edward H. (2022-07-13). "A search for monochromatic light towards the Galactic Centre". Monthly Notices of the Royal Astronomical Society. 515 (3): 3898–3910. arXiv:2208.13561. doi:10.1093/mnras/stac1933. ISSN 0035-8711.
  85. ^ University of California – San Diego. "Search for extraterrestrial intelligence extends to new realms". phys.org. Retrieved 2023-02-01.
  86. ^ Clark, James R.; Cahoy, Kerri (2018-11-05). "Optical Detection of Lasers with Near-term Technology at Interstellar Distances". The Astrophysical Journal. 867 (2): 97. Bibcode:2018ApJ...867...97C. doi:10.3847/1538-4357/aae380. hdl:1721.1/135859. ISSN 1538-4357. S2CID 125463857.
  87. ^ Exers, Ronald; Cullers, D.; Billingham, J.; Scheffer, L., eds. (2003). SETI 2020: A Roadmap for the Search for Extraterrestrial Intelligence. SETI Press. ISBN 978-0-9666335-3-5.
  88. ^ Vogt, Steven S.; Radovan, Matthew; Kibrick, Robert; Butler, R. Paul; Alcott, Barry; Allen, Steve; Arriagada, Pamela; Bolte, Mike; Burt, Jennifer; Cabak, Jerry; Chloros, Kostas; Cowley, David; Deich, William; Dupraw, Brian; Earthman, Wayne (April 2014). "APF – The Lick Observatory Automated Planet Finder". Publications of the Astronomical Society of the Pacific. 126 (938): 359–379. arXiv:1402.6684. Bibcode:2014PASP..126..359V. doi:10.1086/676120. S2CID 12067979.
  89. ^ SETI, Institute. "Why We Need a New Type of SETI Instrument". Archived from the original on 2021-12-26. Retrieved 2022-05-30.
  90. ^ David, Leonard (2017-08-07). "New 'Laser SETI' Approach Seeks Crowdfunding to Seek Out Alien Life". Space.com. Archived from the original on 2023-01-16. Retrieved 2022-05-30.
  91. ^ "PANOSETI". oirlab.ucsd.edu. Retrieved 2023-02-01.
  92. ^ Koren, Marina (17 April 2017). "Searching the Skies for Alien Laser Beams – A new study scanned 5,600 stars for tiny emissions of light, which may be the best way for an extraterrestrial civilization to signal its existence". The Atlantic. Archived from the original on 15 June 2017. Retrieved 3 June 2017.
  93. ^ Tellis, Nathaniel K.; Marcy, Geoffrey W. (April 2017). "A Search for Laser Emission with Megawatt Thresholds from 5600 FGKM Stars". The Astronomical Journal. 153 (6): 251. arXiv:1704.02535. Bibcode:2017AJ....153..251T. doi:10.3847/1538-3881/aa6d12. S2CID 119088358.
  94. ^ Tellis, Nathaniel K.; Marcy, Geoffrey W. (12 May 2017). "A Search for Laser Emission with Megawatt Thresholds from 5600 FGKM Stars". The Astronomical Journal. 153 (6): 251. arXiv:1704.02535. Bibcode:2017AJ....153..251T. doi:10.3847/1538-3881/aa6d12. S2CID 119088358.
  95. ^ "We could detect alien civilizations through their interstellar quantum communication". phys.org. Archived from the original on 9 May 2021. Retrieved 9 May 2021.
  96. ^ Hippke, Michael (13 April 2021). "Searching for Interstellar Quantum Communications". The Astronomical Journal. 162 (1): 1. arXiv:2104.06446. Bibcode:2021AJ....162....1H. doi:10.3847/1538-3881/abf7b7. S2CID 233231350.
  97. ^ Conover, Emily (5 July 2022). "Aliens could send quantum messages to Earth, calculations suggest". Science News. Archived from the original on 13 July 2022. Retrieved 13 July 2022.
  98. ^ Berera, Arjun; Calderón-Figueroa, Jaime (28 June 2022). "Viability of quantum communication across interstellar distances". Physical Review D. 105 (12): 123033. arXiv:2205.11816. Bibcode:2022PhRvD.105l3033B. doi:10.1103/PhysRevD.105.123033. S2CID 249017926.
  99. ^ Freitas, Robert A. Jr. (1980). "Interstellar probes – A new approach to SETI". Archived from the original on January 1, 2019. Retrieved June 28, 2009.
  100. ^ Freitas, Robert A. Jr. (1983). "Debunking the Myths of Interstellar Probes". Archived from the original on August 14, 2016. Retrieved June 28, 2009.
  101. ^ Freitas, Robert A. Jr. (1983). "The Case for Interstellar Probes". Archived from the original on March 13, 2020. Retrieved June 28, 2009.
  102. ^ Rose, C. & Wright, G. (2 September 2004). "Inscribed matter as an energy efficient means of communication with an extraterrestrial civilization" (PDF). Nature. 431 (7004): 47–9. Bibcode:2004Natur.431...47R. doi:10.1038/nature02884. PMID 15343327. S2CID 4382105. Archived (PDF) from the original on 12 May 2005. Retrieved 29 July 2005.
  103. ^ Sullivan, Woodruff T. (2 September 2004). "Message in a bottle". Nature Magazine. 431 (7004): 27–28. Bibcode:2004Natur.431...27S. doi:10.1038/431027a. PMID 15343314. S2CID 5464290.
  104. ^ Freitas, Robert A. Jr. (November 1983). "The Search for Extraterrestrial Artifacts (SETA)". Archived from the original on September 17, 2009. Retrieved June 28, 2009.
  105. ^ "New York Times Editorial". The New York Times. 8 September 2004. Archived from the original on 16 January 2023. Retrieved 18 February 2017.
  106. ^ Rose, Christopher (September 2004). "Cosmic Communications". Archived from the original on July 1, 2010. Retrieved August 1, 2010.
  107. ^ a b Freitas, Robert A. Jr.; Valdes, Francisco (1980). "A Search for Natural or Artificial Objects Located at the Earth-Moon Libration Points". Archived from the original on August 26, 2019. Retrieved June 28, 2009.
  108. ^ Valdes, Francisco; Freitas, Robert A. Jr. (1983). "A Search for Objects near the Earth-Moon Lagrangian Points". Archived from the original on 2019-08-31. Retrieved 2004-11-12.
  109. ^ Valdes, Francisco; Freitas, Robert A. Jr. (1986). "A Search for the Tritium Hyperfine Line from Nearby Stars". Archived from the original on 2005-02-06. Retrieved 2004-11-12.
  110. ^ Koren, Marina (2017-04-26). "Was the Solar System Previously Home to Another Intelligence?". The Atlantic. Retrieved 2023-04-21. "For all we know, maybe Venus had cities all over it a billion years ago and now they're gone," he [Jason Wright] said.
  111. ^ Wright, Jason T. (2017-06-01). "Prior indigenous technological species". International Journal of Astrobiology. 17 (1). Cambridge University Press (CUP): 96–100. arXiv:1704.07263. doi:10.1017/s1473550417000143. ISSN 1473-5504. S2CID 119028817.
  112. ^ Frank, Adam (31 December 2020). "A new frontier is opening in the search for extraterrestrial life - The reason we haven't found life elsewhere in the universe is simple: We haven't really looked until now". The Washington Post. Archived from the original on 27 December 2021. Retrieved 1 January 2021.
  113. ^ Zackrisson, Erik; Calissendorff, Per; Asadi, Saghar; Nyholm, Anders (2015-08-27). "Extragalactic SETI: the Tully–fisher Relation as a Probe of Dysonian Astroengineering in Disk Galaxies". The Astrophysical Journal. 810 (1): 23. arXiv:1508.02406. Bibcode:2015ApJ...810...23Z. doi:10.1088/0004-637x/810/1/23. ISSN 1538-4357. S2CID 118642500.
  114. ^ Hsiao, Tiger Yu-Yang; Goto, Tomotsugu; Hashimoto, Tetsuya; Santos, Daryl Joe D; On, Alvina Y L; Kilerci-Eser, Ece; Wong, Yi Hang Valerie; Kim, Seong Jin; Wu, Cossas K-W; Ho, Simon C-C; Lu, Ting-Yi (2021-07-01). "A Dyson sphere around a black hole". Monthly Notices of the Royal Astronomical Society. 506 (2): 1723–1732. arXiv:2106.15181. doi:10.1093/mnras/stab1832. ISSN 0035-8711.
  115. ^ Korpela, Eric (2015). "Modeling Indications of Technology in Planetary Transit Light Curves – Dark-side illumination". The Astrophysical Journal. 809 (2): 139. arXiv:1505.07399. Bibcode:2015ApJ...809..139K. doi:10.1088/0004-637X/809/2/139. S2CID 119113487.
  116. ^ Almár, Iván (2011). "SETI and astrobiology: The Rio Scale and the London Scale". Acta Astronautica. 69 (9–10): 899–904. Bibcode:2011AcAau..69..899A. doi:10.1016/j.actaastro.2011.05.036.
  117. ^ a b "Heat-Seeking, Alien-Hunting Telescope Could Be Ready In 5 Years". Space.com. 2013-06-07. Archived from the original on 2013-07-01. Retrieved 2013-07-10.
  118. ^ Dyson, Freeman J. (1960). "Search for Artificial Stellar Sources of Infra-Red Radiation". Science. 131 (3414): 1667–1668. Bibcode:1960Sci...131.1667D. doi:10.1126/science.131.3414.1667. PMID 17780673. S2CID 3195432. Archived from the original on 2019-07-14. Retrieved 2012-09-25.
  119. ^ Hall, Shannon. "Impossible vanishing stars could be signs of advanced alien life". New Scientist. Retrieved 2023-02-02.
  120. ^ Billings, Lee. "Alien Supercivilizations Absent from 100,000 Nearby Galaxies". Scientific American. Archived from the original on 2015-04-18. Retrieved 2015-04-18.
  121. ^ Griffith, Roger L.; Wright, Jason T.; Maldonado, Jessica; Povich, Matthew S.; Sigurđsson, Steinn; Mullan, Brendan (15 April 2015). "The Ĝ Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. III. The Reddest Extended Sources in WISE". The Astrophysical Journal Supplement Series. 217 (2): 25. arXiv:1504.03418. Bibcode:2015ApJS..217...25G. doi:10.1088/0067-0049/217/2/25. S2CID 118463557.
  122. ^ Villard, Ray (2013). "Alien 'Star Engine' Detectable in Exoplanet Data?". Archived from the original on 2013-07-05. Retrieved 2013-07-08.
  123. ^ Forgan, Duncan; Elvis, Martin (2011). "Extrasolar Asteroid Mining as Forensic Evidence for Extraterrestrial Intelligence". International Journal of Astrobiology. 10 (4): 307. arXiv:1103.5369. Bibcode:2011IJAsB..10..307F. doi:10.1017/S1473550411000127. S2CID 119111392.
  124. ^ "SETI search urged to look for city lights". UPI.com. 2011-11-03. Archived from the original on 2013-11-09. Retrieved 2013-07-10.
  125. ^ Extrasolar Planets: Formation, Detection and Dynamics, Rudolf Dvorak, p. 14, John Wiley & Sons, 2007
  126. ^ Povich, Matthew (11 August 2014). "Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies". astro-ph.GA. Astrobiology Web. Archived from the original on 2014-08-19. Retrieved 2014-08-19.
  127. ^ "Satellite sniffs out chemical traces of atmospheric pollution / Observing the Earth / Our Activities / ESA". Esa.int. 2000-12-18. Archived from the original on 2013-11-09. Retrieved 2013-07-10.
  128. ^ "Haze on Saturn's Moon Titan Is Similar to Earth's Pollution". Space.com. 2013-06-06. Archived from the original on 2013-07-13. Retrieved 2013-07-10.
  129. ^ "Alien Hairspray May Help Us Find E.T." Space.com. 2012-11-26. Archived from the original on 2021-03-09. Retrieved 2013-07-10.
  130. ^ "How to Find ET with Infrared Light". Astronomy.com. June 2013. Archived from the original on 2013-11-09.
  131. ^ Shostak, Seth (2018-04-16). "Alien satellites might offer a new way to find E.T." SETI Institute. Archived from the original on 2022-11-27. Retrieved 2022-09-22.
  132. ^ Zubrin, Robert (1995). "Detection of Extraterrestrial Civilizations via the Spectral Signature of Advanced Interstellar Spacecraft". In Shostak, Seth (ed.). Astronomical Society of the Pacific Conference Series. Progress in the Search for Extraterrestrial Life. Astronomical Society of the Pacific. pp. 487–496. Bibcode:1995ASPC...74..487Z.
  133. ^ Freitas, Robert (November 1983). "The Case for Interstellar Probes". Journal of the British Interplanetary Society. 36: 490–495. Bibcode:1983JBIS...36..490F. Archived from the original on 2020-03-13. Retrieved 2004-11-12.
  134. ^ Tough, Allen (1998). "Small Smart Interstellar Probes" (PDF). Journal of the British Interplanetary Society. 51: 167–174. Archived (PDF) from the original on 2021-02-26. Retrieved 2012-06-02.
  135. ^ Lacki, Brian C. (2015). "SETI at Planck Energy: When Particle Physicists Become Cosmic Engineers". arXiv:1503.01509 [(astro-ph.HE].
  136. ^ Zenil, Hector; Adams, Alyssa; Abrahão, Felipe S. (2023). "An Optimal, Universal and Agnostic Decoding Method for Message Reconstruction, Bio and Technosignature Detection". arXiv:2303.16045 [cs.IT].
  137. ^ Hutson, Matthew (June 21, 2023). "Here's how we could begin decoding an alien message using math". Science News. Society for Science. Retrieved May 27, 2024.
  138. ^ Zenil, Hector; de Sena Monteiro Ozelim, Luan Carlos (2024). "Fractal Spatio-temporal Scale-free Messaging: Amplitude Modulation of Self-executable Carriers Given by the Weierstrass Function's Components". arXiv:2403.06633 [cs.IT].
  139. ^ Jones, Eric (March 1985). ""Where is everybody?", An account of Fermi's question" (PDF). Los Alamos National Laboratory. Archived (PDF) from the original on November 5, 2015. Retrieved June 28, 2009.
  140. ^ Ben Zuckerman and Michael H. Hart (editors), Extraterrestrials: Where Are They? Elsevier Science & Technology Books (1982), ISBN 9780080263427
  141. ^ Stephen Webb, Where is Everybody? Fifty Solutions to Fermi's Paradox, Copernicus, 2002 edition, 978-0387955018
  142. ^ von Hoerner, Sebastian (December 8, 1961). "The Search for Signals from Other Civilizations". Science. 134 (3493): 1839–43. Bibcode:1961Sci...134.1839V. doi:10.1126/science.134.3493.1839. ISSN 0036-8075. PMID 17831111.
  143. ^ Hoerner, Sebastian von (1919–2003). Archived from the original on 2020-07-20. Retrieved 2020-07-26. {{cite encyclopedia}}: |website= ignored (help)
  144. ^ Shklovsky, Iosif (1987). Вселенная. Жизнь. Разум (in Russian). Moscow: Наука. pp. 250–252. Archived from the original on 2020-11-25. Retrieved 2020-07-26.
  145. ^ Lem, Stanisław (2013). "Space Civilizations". Summa Technologiae. Minneapolis: University of Minnesota Press. ISBN 978-0816675777.
  146. ^ "Eavesdropping on the Earth" (PDF). astrosociety.org. 1979. Archived (PDF) from the original on 2018-08-14. Retrieved 2018-08-14.
  147. ^ "SETI Insentitive To Earth-like Signals". spacedaily.com. 1998. Archived from the original on April 13, 2013. Retrieved February 8, 2013.
  148. ^ Norris, Ray (2022-12-14). "Terms of reference of the SETI Post-Detection Committee". www.atnf.csiro.au. Retrieved 2023-02-02.
  149. ^ "What to do if we find extraterrestrial life". NBC News. 15 October 2010. Archived from the original on October 30, 2020. Retrieved 2023-02-02.
  150. ^ "The Rio Scale". International Academy of Astronautics. Archived from the original on 2016-09-02. Retrieved 2016-08-29.
  151. ^ Almár, Iván (November–December 2011). "SETI and Astrobiology: The Rio Scale and the London Scale". Acta Astronautica. 69 (9–10): 899–904. Bibcode:2011AcAau..69..899A. doi:10.1016/j.actaastro.2011.05.036.
  152. ^ "Scientists revise the Rio Scale for reported alien encounters. July 2018". Archived from the original on 2018-07-24. Retrieved 2018-07-24.
  153. ^ SETI Institute (2020). "Where did the famous mystery Wow! signal, detected in 1977, come from?". Twitter. Archived from the original on 2022-05-30. Retrieved 2022-05-30.
  154. ^ Alexander, Amir (2004-09-02). "SETI@home Leaders Deny Reports of Likely Extraterrestrial Signal". The Planetary Society. Archived from the original on 2011-07-26. Retrieved 2006-06-12.
  155. ^ Whitehouse, David (2004-09-02). "Astronomers deny ET signal report". BBC News. Archived from the original on 2006-06-15. Retrieved 2006-06-12.
  156. ^ Vance, Ashlee. "SETI urged to fess up over alien signals". www.theregister.com. Retrieved 2023-02-02.
  157. ^ "NAI News Article: The Meaning of Life". 2004-11-01. Archived from the original on 2004-11-01. Retrieved 2023-02-02.
  158. ^ Billingham, J.; Benford, J. (2016). "Costs and difficulties of interstellar 'Messaging' and the need for international debate on potential risks". Journal of the British Interplanetary Society. 19: 17–23.
  159. ^ Gertz, J. (2016). "Reviewing METI: A critical analysis of the arguments". Journal of the British Interplanetary Society. 69: 31–36. arXiv:1605.05663. Bibcode:2016JBIS...69...31G.
  160. ^ Haramia, Chelsea; DeMarines, Julia (2019-01-02). "The Imperative to Develop an Ethically-Informed METI Analysis". Theology and Science. 17 (1): 38–48. doi:10.1080/14746700.2019.1557800. ISSN 1474-6700. S2CID 171404637.
  161. ^ Vakoch, Douglas A. (2017-04-03). "Hawking's fear of an alien invasion may explain the Fermi Paradox". Theology and Science. 15 (2): 134–138. doi:10.1080/14746700.2017.1299380. ISSN 1474-6700. S2CID 219627161.
  162. ^ Shostak, Seth (27 September 2016). "Why Stephen Hawking is light years from the truth about 'dangerous aliens'". The Guardian. Archived from the original on 27 September 2016. Retrieved 28 September 2016.
  163. ^ Orwig, Jessica. "A world leading scientist on the search for extraterrestrials pointed out a flaw in Stephen Hawking's fear of finding intelligent aliens". Business Insider. Archived from the original on 21 February 2018. Retrieved 8 February 2018.
  164. ^ Ward, Peter D.; Brownlee, Donald (2007). Rare Earth: Why Complex Life is Uncommon in the Universe. Springer. p. 250. ISBN 9780387218489. Archived from the original on 2023-01-16. Retrieved 2020-10-10. Unfortunately, it is very difficult to know if SETI is an effective use of resources. If the Rare Earth Hypothesis is correct, then it clearly is a futile effort. Revised edition (first published in 2000)
  165. ^ Denton, Peter H.; Restivo, Sal (2008). Battleground: Science and Technology [2 volumes]. ABC-CLIO. p. 403. ISBN 9781567207439. Archived from the original on 2023-01-16. Retrieved 2020-10-10. SETI enthusiasts believe that the human race is characterized by mediocrity rather than excellence. According to Frank Drake and his followers, this means that intelligent life is common in the universe. Peter Ward and Donald Brownlee challenge the principle of mediocrity with the rare Earth hypothesis in their book Rare Earth: Why Complex Life Is Uncommon in the Universe (2000).
  166. ^ a b Losch, Andreas (2017). What is Life? On Earth and Beyond. Cambridge University Press. p. 167. ISBN 9781107175891. Archived from the original on 2023-01-16. Retrieved 2020-10-10. In many ways, the rare-Earth hypothesis has since become somewhat of a default position in many astrobiological circles, and – since it predicts the absence of rationale for SETI – a mainstay of SETI scepticism. [...] There are many criticisms rightly raised against the rare-Earth Hypothesis, but here I shall mention just one.
  167. ^ a b Mash, Roy (1993). "Big numbers and induction in the case for extraterrestrial intelligence". Philosophy of Science. 60 (2): 204–222. doi:10.1086/289729. JSTOR 188351. S2CID 120672390.
  168. ^ a b c Ćirković, Milan M. (2012-06-21). About the author (2012). Cambridge University Press. ISBN 9780521197755. Archived from the original on 2023-01-16. Retrieved 2017-12-13. Milan M. Ćirković is a research professor at the Astronomical Observatory of Belgrade, (Serbia) and a research associate of the Future of Humanity Institute at the University of Oxford.
  169. ^ Ćirković, Milan M. (2012-06-21). The Astrobiological Landscape: Philosophical Foundations of the Study of Cosmic Life. Cambridge University Press. ISBN 978-0-521-19775-5.
  170. ^ Basalla, George (2006-01-19). About the author (2006). Oxford University Press. ISBN 9780198038351. Archived from the original on 2023-01-16. Retrieved 2017-12-13.
  171. ^ a b Basalla, George (2006). Civilized Life in the Universe: Scientists on Intelligent Extraterrestrials. Oxford University Press. p. 14. ISBN 9780198038351. Retrieved 2017-12-13. Despite all their scientific trappings, the extraterrestrials discussed by scientists are as imaginary as the spirits and gods of religion or myth.
  172. ^ a b Ćirković (2012), p. 172 Archived 2023-01-16 at the Wayback Machine, "It is Basalla, the critic of SETI and not its practitioners, who violates the spirit of Hull's dictum, for instance, when he writes that 'extraterrestrials discussed by scientists are as imaginary as the spirits and gods of religion or myth'.[54] Second, the approach to this sociology of science criticism is obviously marred by Basalla's insistence on personal quirks and idiosyncrasies as the main motivation of scientific activity, an attitude that is not only demeaning to the many scientists mentioned, ..."
  173. ^ "Cuny – City College – Philosophy Department". 2015-07-05. Archived from the original on 2020-08-20. Retrieved 2017-12-13.
  174. ^ Pigliucci, Massimo (2010). Nonsense on Stilts: How to Tell Science from Bunk. University of Chicago Press. p. 34. ISBN 9780226667874. Archived from the original on 2023-01-16. Retrieved 2017-12-13. But in the case of SETI, negative results are what is expected most of the time, perhaps even forever, regardless of the truth of the central hypothesis. This raises the question: when will SETI researchers think that enough negatives have been accumulated to reject the hypothesis of existence of other technological civilizations? If the answer is that such hypothesis can never be rejected, regardless of the empirical results, that pushes SETI uncomfortably close to the status of pseudoscience. There is another way to look at the problem, based on an additional element (besides empirical evidence and testability) ...
  175. ^ Ćirković (2012), p175 Archived 2023-01-16 at the Wayback Machine, "However, in the second chapter, tellingly entitled 'Almost Science', the author (a distinguished philosopher, mainly involved in the philosophy of biology) devotes several subsections to the fields which are, in his opinion, neither pseudosciences, nor fully legitimate members of the scientific family. Here he puts SETI studies in the illustrious company of string theory, interpretations of quantum mechanics, evolutionary psychology and history (of the 'synthetic' kind done recently by Jared Diamond). While the club is fun to be in – and only a staunch conservative does not expect great breakthroughs to come out of one or more of these domains in the next few decades – the justification offered by Pigliucci in the case of SETI is weak, outdated, and reflecting particular philosophical prejudices similar to the ones described above in Mash and Basalla.[60]"
  176. ^ Carrigan, Robert A. Jr. (June 2006). "Do potential SETI signals need to be decontaminated?" (PDF). Fermi National Accelerator Laboratory. Archived (PDF) from the original on 2008-08-28. Retrieved 2009-06-29.
  177. ^ "A Science-Fiction Movie-Plot Threat". 29 November 2005. Archived from the original on June 4, 2011. Retrieved March 13, 2011.
  178. ^ Friedman, Stanton T. (2002-05-13). "UFOs: Challenge to SETI Specialists". Archived from the original on 2017-12-17. Retrieved 2017-12-17.
  179. ^ Friedman, Stanton T. (2009-05-30). "Pseudo-Science of Anti-Ufology". The UFO Chronicles. Archived from the original on 2017-09-18. Retrieved 2017-12-17.
  180. ^ Denzler, Brenda (2003). The lure of the edge: scientific passions, religious beliefs, and the pursuit of UFOs. University of California Press. p. 69. ISBN 978-0-520-23905-0.
  181. ^ Moldwin, Mark (12 November 2004). "Why SETI Is Science and UFOlogy Is Not – A Space Science Perspective on Boundaries". Archived from the original on 2011-05-23.
  182. ^ Tuomela, Raimo (1985). Science, action, and reality. Springer. p. 234. ISBN 978-90-277-2098-6.
  183. ^ Feist, Gregory J. (2006). The psychology of science and the origins of the scientific mind. Yale University Press. p. 219. ISBN 978-0-300-11074-6.
  184. ^ Restivo, Sal P. (2005). Science, technology, and society: an encyclopedia. Oxford University Press US. p. 176. ISBN 978-0-19-514193-1.
  185. ^ a b Tramiel, Leonard (23 August 2016). "Life as We Know It: An Interview with Jill Tarter". CSI. Center for Inquiry. Archived from the original on 2 January 2018. Retrieved 1 January 2018.
  186. ^ "Activities". projects.iq.harvard.edu. Archived from the original on 25 July 2021. Retrieved 25 July 2021.
  187. ^ Loeb, Avi. "A Possible Link between 'Oumuamua and Unidentified Aerial Phenomena". Scientific American. Archived from the original on 29 July 2021. Retrieved 25 July 2021.
  188. ^ "The Galileo Project for the Systematic Scientific Search for Evidence of Extraterrestrial Technological Artifacts". projects.iq.harvard.edu. Archived from the original on 24 July 2021. Retrieved 25 July 2021.

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