Arecibo Wow! is a search for transient radio signals inspired by the Wow! Signal
Arecibo Wow! is a search for transient radio signals inspired by the Wow! Signal
For a review of transient radio astronomy see Murphy & Kaplan (2025)
The discovery of unexpected narrowband radiation of natural origin would be of great importance in its own right. No radiation can be classed as of intelligent origin until all mechanisms of producing that radiation by natural means have been thoroughly investigated and understood. — John D. Kraus & Robert S. Dixon (1974)
There may exist many as yet undiscovered individual signals in the data archive [of the Ohio SETI program]. No thorough search has yet been made for them. - Robert S. Dixon (1985)
[I] would be just as happy to someday discover the [Wow!] signal was an unknown natural phenomena, because that would also be a new discovery. — Robert S. Dixon (1994)
Carl Sagan [is interested] in seeing the Ohio SETI data from the period of 1977-1984, including the "Wow!" signal, revisited, re-analyzed, compared to past results and published. — Robert S. Dixon (1994)
Either the Wow! Signal was the intercepted radiation from another civilization, or it's a previously undiscovered astrophysical phenomenon. Either possibility is mind-boggling. — H. Paul Shuch (1997)
The only explanation for [the Wow! Signal] seems to be a maser in the shell of a supernova remnant, though in the future [someone] may identify a new mechanism of such pulses. — G. A. Gontcharov (2011)
John Kraus designed and built the Big Ear, the telescope that detected the Wow! Signal. He conducted the first analyses of the signal and publicly announced its discovery in 1979.
Bob Dixon was the driving force behind the SETI project at the Big Ear since 1973. He developed the detection strategies and software that made the discovery of the Wow! Signal possible.
Jerry Ehman discovered the Wow! Signal in the 1977 data. He also helped develop the search software and later performed a more detailed reanalysis of the signal in 1997.
The Ohio State University Radio Observatory (OSURO, 1963–1998) — better known as “Big Ear” — was, in the early 1960s, the third-largest radio telescope in the United States, after the Arecibo Observatory (1963–2020) and the NRAO 300-foot telescope (1962-1998).
Big Ear’s primary mission was to scan the sky for new radio sources as part of the Ohio Sky Survey (OSS), conducted between 1965 and 1971. It cataloged nearly 20,000 radio sources, including what was then the most distant known object in the universe.
The telescope was designed and built by the renowned radio astronomer John Kraus of Ohio State University (OSU). Kraus also invented the helical antenna — now widely used in communication systems — and authored several influential books, including the classic Radio Astronomy textbook.
In 1972, Big Ear lost its National Science Foundation (NSF) funding. The NSF was shifting focus toward national facilities and away from university-managed telescopes. Many similar research projects across the country faced the same fate.
After NASA’s Project Cyclops in 1971 renewed excitement about the Search for Extraterrestrial Intelligence (SETI), staff astronomer Robert Dixon suggested repurposing the now-defunded Big Ear for SETI observations. John Kraus agreed.
Thus, in 1973, the Ohio SETI Project was born. Another staff astronomer, Jerry Ehman, joined the effort. Kraus remained as an astronomer at OSU, but Robert Dixon and Jerry Ehman soon had to find other full-time jobs, operating the telescope primarily in their spare time.
The Ohio SETI Project survived thanks to volunteers and students, with occasional donations and NASA and NSF small grants for equipment upgrades. OSU covered the telescope’s basic operational costs, but there was no funding for salaries.
Four years into the project, Jerry Ehman spotted a remarkable signal in the data — one that matched all the characteristics they were searching for in an extraterrestrial transmission. Astonished, he circled the data and wrote “Wow!” beside it, giving the famous Wow! Signal its name.
John Kraus and Robert Dixon immediately began deeper analyses, improving the telescope’s software and repeatedly reobserving the same region of sky. Despite years of follow-up, the signal was never detected again.
In 1979, the Ohio SETI group went public about the Wow! Signal through Cosmic Search, their own magazine — the first ever dedicated to the search for extraterrestrial life. It featured both introductory and technical articles, including by prominent astronomers such as Frank Drake, Carl Sagan, and Jill Tarter.
Interest in explaining the Wow! Signal persisted, but surprisingly few attempts were made to search for it again. One notable exception was Robert Gray, a data analyst from Chicago, who became fascinated with the signal in the early 1980s. He first tried observing it with a homemade radio dish, and later with several professional radio telescopes, but it never repeated.
The Big Ear holds the record for the longest-running dedicated SETI project, operating for 24 years (1973–1997). Other long-duration efforts include SETI@Home, which ran for 21 years (1999–2020); the META/BETA search at Harvard, active for about 15 years (1985–2000); and Project Phoenix, which operated for 9 years (1995–2004).
Although SETI projects began as early as 1960 with Frank Drake’s Project Ozma, it was Big Ear, ironically the least funded of them all, that detected the most intriguing SETI signal ever recorded. A major reason may be that the Ohio SETI program devoted 100% of the telescope’s time to a continuous all-sky survey, while other SETI efforts are limited to less telescope time and therefore can search only a much smaller portion of the sky.
Nearly 50 years later, the Arecibo Wow! Project was launched to search archived radio-telescope data — including from Arecibo — for Wow-like signals. To their surprise, the team uncovered a promising astrophysical explanation and found that the signal’s true characteristics differed slightly from early estimates, which may explain why it remained so elusive.
Today, the Arecibo Wow! Project brings together scientists from the Arecibo Observatory, surviving members of the Big Ear team, and astronomers who have long studied the Wow! Signal. We now understand much more about this enigmatic event — and may be closer than ever to finally solving a mystery that has captivated generations.
August 26, 2025
Nearly half a century after its detection, the famous “Wow! Signal”, a strong, unexplained radio burst captured by Ohio State University’s SETI project in 1977, remains one of the most tantalizing mysteries in the search for extraterrestrial intelligence.
Now, researchers from the Arecibo Wow! project have re-analyzed decades of previously unpublished observations, producing the most precise characterization yet of the enigmatic signal and revealing new clues to its origin.
The study revisits archival data from the Ohio State University SETI program, including records not examined in earlier analyses, and applies modern signal analysis techniques. The results significantly refine the Wow! Signal’s properties:
Location: Two adjacent sky fields, centered at right ascensions 19h 25m 02s ± 3s or 19h 27m 55s ± 3s, and declination –26° 57′ ± 20′ (J2000). This is both more precise and slightly shifted from earlier estimates.
Intensity: A peak flux density exceeding 250 Janskys, more than four times higher than the commonly cited value.
Frequency: 1420.726 MHz, placing it firmly in the hydrogen line but with a greater radial velocity than previously assumed.
These refinements might help explain why decades of follow-up observations have failed to find the signal’s source.
“Our results don’t solve the mystery of the Wow! Signal,” said lead author Prof. Abel Méndez of the Planetary Habitability Laboratory at the University of Puerto Rico at Arecibo. “But they give us the clearest picture yet of what it was and where it came from. This new precision allows us to target future observations more effectively than ever before.”
"We look at old archives with modern science methodologies. It's a bit like space archaeology," said Dr. Hector Socas Navarro, Director of the European Solar Telescope Foundation and one of the co-authors of this study.
The findings bolster the case for a natural astrophysical origin, while making radio interference an increasingly unlikely explanation. They also highlight the enduring value of historical data in answering today’s astronomical questions.
“This study doesn’t close the case,” Méndez said. “It reopens it, but now with a much sharper map in hand.”
The research will be submitted to the Astrophysical Journal, and is available at this link.
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Members of the Arecibo Wow! Team are Abel Méndez from the PHL @ UPR Arecibo, Kevin Ortiz Ceballos from the Center for Astrophysics, Harvard & Smithsonian, Jorge I. Zuluaga from the SEAP/FACom Institute of Physics, University of Antioquia, Kelby D'Angelo Palencia-Torres, from UPR Rio Piedras, Alisson Smith from UPR Mayagüez, Emmanuel J. Morales Butler from UPR Utuado, Héctor Socas-Navarro from the European Solar Telescope Foundation, David Kipping from Columbia University, Hodari-Sadiki Hubbard-James from Agnes Scott College, Mariangelly Díaz-Rodríguez from Boeing/Florida State University, Alondra Cardona from the University of Arizona, Mai Le from Agnes Scott College, and Alejandro Ricón-Torres from the Interamerican University of Puerto Rico at Bayamón.
Figure 1: Comparison of the previously estimated locations of the Wow! Signal (gray boxes) with the refined positions from the Arecibo Wow! Project (yellow boxes). The signal’s source is presumed to lie within one of these boxes and beyond the foreground Galactic hydrogen clouds shown in bright red. Credit: PHL @ UPR Arecibo
Table 1: Revised Properties of the Wow! Signal.
Figure 2: We hypothesize that the Wow! Signal was caused by a sudden brightening of the hydrogen line in interstellar clouds, triggered by a powerful transient radiation source such as a magnetar flare or soft gamma repeater (SGR). Maser flaring or superradiance mechanisms could have produced a narrowband emission consistent with the characteristics of the Wow! Signal. This hypothesis accounts for all observed properties of the signal and suggests it may represent the first recorded maser-like flare in the hydrogen line (Méndez et al., 2024).
Search Archived Data for Transient Signals: Systematically search historical radio astronomy archives, including those from Arecibo and other observatories, for unexplained broadband and narrowband transient radio signals, including those similar to the Wow! Signal.
Analyze the Wow! Signal: Re-examine the Wow! Signal using modern tools and techniques to evaluate its characteristics, origin hypotheses, and astrophysical context, seeking any clues that might explain its nature.
Preserve and Archive the Big Ear Telescope Data: Digitize, catalog, and safeguard all remaining data and documentation from the Big Ear radio telescope to support future analysis and historical research.
Conduct New Observations to Search for Transient Signals or their Sources: Utilize small and large radio telescopes to observe regions of interest for the sources of transient radio signals.
Engage and Educate the Public on Radio Astronomy Science: Develop educational programs, citizen science initiatives, and public outreach campaigns to promote awareness of the Wow! Signal, radio astronomy, and the ongoing search for extraterrestrial intelligence.
The Arecibo Wow! Observatory is a new radio astronomy initiative currently under development. It integrates archival data from the Arecibo and Big Ear telescopes with new observations collected through the Wow@Home network of small telescopes, the Arecibo 12-meter radio telescope, and other instruments.
Archived data from the Arecibo Telescope (1963-2020)
Archived data from the Big Ear (1963-1998)
Arecibo 12m Telescope (coming soon)
SETI Institute LaserSETI (coming soon)
Abel Méndez, PHL @ UPR Arecibo (abel.mendez@upr.edu)
Kevin Ortiz Ceballos, Center for Astrophysics | Harvard & Smithsonian
Jorge I. Zuluaga, SEAP/FACom Institute of Physics, University of Antioquia
Kelby D'Angelo Palencia-Torres, UPR Rio Piedras
Alisson Smith, UPR Mayagüez
Emmanuel J. Morales Butler, UPR Utuado
Héctor Socas-Navarro, European Solar Telescope Foundation
David Kipping, Columbia University
Hodari-Sadiki Hubbard-James, Agnes Scott College
Mariangelly Díaz-Rodríguez, Boeing/Florida State University
Alondra Cardona, University of Arizona
Mai Le (undergraduate student), Agnes Scott College
Alejandro Ricón-Torres (undergraduate student), Interamerican University of Puerto Rico
Robert S. Dixon, former staff of the Big Ear
Russ Childers, former staff of the Big Ear
Heinz Andernach, Universidad de Guanajuato/Thuringian State Observatory (TLS)
Teegarden's Star
Luyten's Star
Barnard's Star
Ross 128
TRAPPIST-1
Proxima Centauri
Tau Ceti
K2-18