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The Search for Extraterrestrial Life encompasses humanity's scientific efforts to detect intelligent civilizations and microbial life beyond Earth. Beginning with early radio astronomy experiments like Project Ozma in 1960, the field has grown through initiatives such as NASA's SETI programs, the Allen Telescope Array, the discovery of thousands of exoplanets, and missions exploring potentially habitable worlds like Mars and the icy moons of Jupiter and Saturn. More Less
1896
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In 1896, Nikola Tesla suggested that an extreme version of his wireless electrical transmission system could be used to contact beings on Mars, marking one of the earliest serious proposals for interplanetary communication.
Image source: Nikola Tesla
1899
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While conducting experiments at his Colorado Springs experimental station in 1899, Nikola Tesla thought he had detected a signal from Mars, as an odd repetitive static signal seemed to cut off when Mars set in the night sky.
Aug 21, 1924 - Aug 23, 1924
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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, prompting efforts to listen for possible radio transmissions from the planet.
Mar 1955
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In the March 1955 issue of Scientific American, John D. Kraus outlined ideas for detecting extraterrestrial radio signals, helping lay groundwork for later systematic searches.
1959
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A 1959 paper by Philip Morrison and Giuseppe Cocconi first pointed out the possibility of searching the microwave spectrum for signals from extraterrestrial civilizations, providing a scientific foundation for modern SETI.
Image source: Search for extraterrestrial intelligence
1960
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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 books, using a radio telescope to listen for signals from nearby Sun-like stars.
Image source: Project Ozma
1971
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In 1971, NASA funded a SETI study involving Frank Drake, Barney Oliver of Hewlett-Packard Laboratories, and others. The Cyclops study discounted optical SETI as too difficult but shaped future radio search strategies.
Image source: Project Cyclops
Aug 15, 1977
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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 Big Ear telescope, which became known as the "Wow!" signal. It was never verified, though a 2020 post suggested an astronomer might have pinpointed its host star.
1979
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SERENDIP (Search for Extraterrestrial Radio Emissions from Nearby Developed Intelligent Populations) is a SETI program launched in 1979 by the Berkeley SETI Research Center, piggybacking on existing radio telescope observations.
1981
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Work led in 1981 to a portable spectrum analyzer named "Suitcase SETI" with a capacity of 131,000 narrow band channels. After field tests into 1982, it was put into use in 1983 with the Harvard/Smithsonian radio telescope at Oak Ridge Observatory.
1983 - 1985
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Using Suitcase SETI at the 26-meter Harvard/Smithsonian radio telescope, the project was named "Sentinel" and continued into 1985, conducting targeted searches of nearby stars.
1985
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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", led by Paul Horowitz at Harvard.
1990
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A second such effort, META II, was begun in Argentina in 1990 to search the southern sky, receiving an equipment upgrade in 1996–1997.
1995 - Mar 2004
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In 1995 the nonprofit SETI Institute resurrected the NASA MOP program under the name Project "Phoenix", backed by private funding. Under Jill Tarter's direction, it studied roughly 1,000 nearby Sun-like stars until approximately 2015, observing at Parkes, Green Bank, and Arecibo, covering frequencies from 1200 to 3000 MHz.
Oct 30, 1995
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The follow-on to META was named "BETA", for "Billion-channel Extraterrestrial Assay", and it commenced observation on October 30, 1995 at the Harvard/Smithsonian radio telescope.
Mar 23, 1999
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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, ending those programs' observations.
Image source: Harvard–Smithsonian Center for Astrophysics
May 1999
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SETI@home, conceived by David Gedye along with Craig Kasnoff, is a popular volunteer computing project launched by the Berkeley SETI Research Center in May 1999, allowing millions of people to analyze radio data on their home computers.
Image source: SETI@home
2004
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In 2004, radio source SHGb02+14a set off media speculation 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.
Oct 2007
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Planned for 2007 completion at a cost of US$25 million, the first portion of the Allen Telescope Array (ATA-42) became operational in October 2007 with 42 antennas. From 2007 to 2015, ATA identified hundreds of millions of technological signals.
Image source: Allen Telescope Array
Dec 12, 2008
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CNET published an article and pictures about the Allen Telescope Array (ATA) on December 12, 2008, bringing public attention to the innovative radio observatory dedicated partly to SETI research.
2010
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By 2010, after 10 years of data collection, SETI@home had listened to one frequency at every point of over 67 percent of the sky observable from Arecibo with at least three scans, covering about 20 percent of the full celestial sphere.
2011
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Berkeley astronomers used the ATA to pursue several science topics, some of which might have transient SETI signals, until 2011, when the collaboration between the University of California, Berkeley and the SETI Institute was terminated.
Apr 2011 - Dec 5, 2011
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In April 2011, the ATA entered an 8-month "hibernation" due to funding shortfalls. Regular operation resumed on December 5, 2011, after new funding arrangements were secured.
2012
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In 2012, the ATA was revitalized with a $3.6 million donation by Franklin Antonio, co-founder and Chief Scientist of QUALCOMM Incorporated, enabling upgrades including new receivers, the first of which was installed and proven by July 2013.
2014 - 2015
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The most recently deployed SERENDIP spectrometer, SERENDIP VI, was installed at both the Arecibo Telescope and the Green Bank Telescope in 2014–2015, continuing Berkeley's long-running piggyback SETI surveys.
Jul 2015
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Announced in July 2015 by Stephen Hawking and Yuri Milner, Breakthrough Listen is a $100 million, 10-year initiative to actively search for intelligent extraterrestrial communications, observing thousands of hours yearly on the Green Bank Observatory and Parkes Observatory telescopes.
Image source: Breakthrough Listen
2016
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Since 2016, UCLA undergraduate and graduate students have been participating in radio searches for technosignatures with the Green Bank Telescope, training a new generation of SETI researchers.
Image source: Green Bank Telescope
Oct 2019
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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 around newly discovered exoplanets.
2020
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Although the SETI Institute does not officially recognize the Wow! signal as being of extraterrestrial origin since it was never verified, a 2020 Twitter post stated that an astronomer might have pinpointed the host star of the famous 1977 signal.
Image source: Wow! signal
Mar 31, 2020
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On March 31, 2020, with 91,454 active users, the project stopped sending out new work to SETI@home users, bringing this pioneering volunteer computing effort to an indefinite hiatus after more than two decades.
Jun 14, 2022
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On June 14, 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 natural radio interference may be the source.
Image source: Five-hundred-meter Aperture Spherical Telescope
Jun 18, 2022
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On June 18, 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.", deflating hopes raised by the FAST detection report.
Image source: Dan Werthimer
1960
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Ronald Bracewell proposed in 1960 that advanced civilizations might send autonomous interstellar probes to monitor and communicate with emerging societies, an alternative to radio-based communication (see Bracewell probe).
Image source: Bracewell probe
1961
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R. N. Schwartz and Charles Hard Townes published a 1961 paper in Nature titled "Interstellar and Interplanetary Communication by Optical Masers", proposing that lasers could be used for interstellar communication and detection.
1978
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The British Interplanetary Society's starship study Project Daedalus in 1978 demonstrated the technical feasibility of sending physical probes between stars, supporting the Bracewell probe approach to interstellar contact.
Image source: Project Daedalus
1979
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In 1979, Freitas and Valdes conducted a photographic search of the Earth-Moon triangular libration points L4 and L5 seeking possible orbiting extraterrestrial probes, finding nothing to a detection limit of about 14th magnitude; a second, more comprehensive search followed in 1982.
Image source: Robert Freitas
1979
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Starting in 1979, Robert Freitas advanced arguments for the proposition that physical space-probes are a superior mode of interstellar communication to radio signals (see Voyager Golden Record).
1983
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In 1983, Charles Hard Townes published a detailed study of optical SETI in the Proceedings of the National Academy of Sciences, which revived interest in laser-based searches within the SETI community.
Image source: Charles H. Townes
Jun 1983
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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 astronomical objects, with emphasis on 53 nearby stars including all visible stars within a 20 light-year radius.
1996
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In recognition that any sufficiently advanced interstellar probe near Earth could easily monitor the terrestrial Internet, 'Invitation to ETI' was established by Allen Tough in 1996 as a Web-based SETI experiment inviting spacefaring probes to establish contact with humanity.
May 2017
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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, renewing momentum for optical SETI searches.
Jan 2020
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In January 2020, two Pulsed All-sky Near-infrared Optical SETI (PANOSETI) project telescopes were installed in the Lick Observatory Astrograph Dome, designed to detect nanosecond optical pulses from across the sky.
2021
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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 extraterrestrial intelligence using existing telescope and receiver technology.
2022
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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 potential challenges and factors for detecting such technosignatures.
Image source: Timeline of quantum computing and communication
1962
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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 Intelligent Life in the Universe (1966).
Image source: Iosif Shklovsky
Nov 1974
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In November 1974, a largely symbolic attempt was made at the Arecibo Observatory to send a message to other worlds, beaming a coded message toward the globular cluster M13.
Image source: Arecibo message
1978
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In 1978, the NASA SETI program was heavily criticized by Senator William Proxmire, and funding for SETI research was removed from the NASA budget by Congress in 1981; funding was restored in 1982 after Carl Sagan convinced Proxmire of the program's value.
Image source: SETI Institute
1980
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In 1980, Carl Sagan, Bruce Murray, and Louis Friedman founded The Planetary Society, which became a major advocate for space exploration and SETI research.
Image source: The Planetary Society
1993
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In 1993, philosopher Roy Mash stated that arguments favoring the existence of extraterrestrial intelligence nearly always contain an overt appeal to big numbers combined with covert reliance on generalization from a single instance, concluding the dispute boils down to a conflict of intuitions.
1994
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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 promoting amateur participation through Project Argus stations.
1999 - 2008
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Further interstellar radio messages — 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 toward nearby star systems.
Oct 2000
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In October 2000, astronomers Iván Almár and Jill Tarter presented the Rio scale to the SETI Permanent Study Group in Rio de Janeiro, an ordinal scale between zero and ten quantifying the impact of any public announcement regarding evidence of extraterrestrial intelligence; it inspired the San Marino Scale (2005) and London Scale (2010) and was revised in 2018.
2006
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George Basalla, Emeritus Professor of History at the University of Delaware, argued in 2006 that "extraterrestrials discussed by scientists are as imaginary as the spirits and gods of religion or myth", and was in turn criticized by Milan M. Ćirković.
2010
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Massimo Pigliucci 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 would cause the hypothesis of Extraterrestrial Intelligence to be abandoned, before eventually concluding SETI is "almost-science".
Image source: Massimo Pigliucci
2012
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In response to critics like Basalla and Mash, Milan M. Ćirković defended SETI's scientific legitimacy in 2012, arguing that the field's methodology and falsifiability place it firmly within mainstream science.
2012
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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, highlighting how modestly funded the entire endeavor remained.
2016
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In a 2016 interview, Jill Tarter pointed out that it is still a misconception that SETI and UFOs are related, emphasizing that SETI searches for verifiable technological signals rather than unexplained sightings.
Image source: Jill Tarter
Sep 2016
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In September 2016, responding to Stephen Hawking's warnings about contacting alien civilizations, astronomer Seth Shostak sought to allay such concerns, arguing that fears of hostile extraterrestrials were overstated.
Image source: Seth Shostak
2021
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Following the publication of the 2021 UFO Report by the U.S. government, the Galileo Project was established to scientifically investigate unidentified aerial phenomena, taking a position distinct from traditional SETI while sharing rigorous scientific methods.
Image source: Galileo project
May 24, 2023
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On May 24, 2023, a test extraterrestrial signal, in the form of a "coded radio signal from Mars", was transmitted to radio telescopes on Earth as part of the 'A Sign in Space' project, allowing the public and scientists to practice decoding a simulated alien transmission.
Image source: Percent sign
Jun 2026
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In June 2026, the International Academy of Astronautics ratified the first update to the protocol for announcing detections of extraterrestrial intelligence, following years of work by the SETI Permanent Study Group and deliberations at IAA meetings.
Image source: International Academy of Astronautics
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