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The Wow! The signal appeared to come from the direction of the constellation Sagittarius and bore the expected hallmarks of extraterrestrial origin.

Astronomer Jerry R. Ehman discovered the anomaly a few days later while reviewing the recorded data. He was so impressed by the result that he circled the reading on the computer printout, "6EQUJ5", and wrote the comment "Wow!

The entire signal sequence lasted for the full second window during which Big Ear was able to observe it, but has not been detected since, despite several subsequent attempts by Ehman and others.

Many hypotheses have been advanced on the origin of the emission, including natural and human-made sources, but none of them adequately explain the signal.

Although the Wow! In a paper, Cornell University physicists Philip Morrison and Giuseppe Cocconi had speculated that any extraterrestrial civilization attempting to communicate via radio signals might do so using a frequency of megahertz 21 centimeters , which is naturally emitted by hydrogen , the most common element in the universe and therefore likely familiar to all technologically advanced civilizations.

In , after completing an extensive survey of extragalactic radio sources , Ohio State University assigned the now-defunct Ohio State University Radio Observatory nicknamed "Big Ear" to the scientific search for extraterrestrial intelligence SETI , in the longest-running program of its kind in history.

By , Ehman was working at the SETI project as a volunteer; his job involved analyzing by hand large amounts of data processed by an IBM computer and recorded on line printer paper.

The string 6EQUJ5, commonly misinterpreted as a message encoded in the radio signal, represents in fact the signal's intensity variation over time, expressed in the particular measuring system adopted for the experiment.

The signal itself appeared to be an unmodulated continuous wave , although any modulation with a period of less than 10 seconds or longer than 72 seconds would not have been detectable.

The signal intensity was measured as signal-to-noise ratio , with the noise or baseline averaged over the previous few minutes. The signal was sampled for 10 seconds and then processed by the computer, which took 2 seconds.

Therefore, every 12 seconds the result for each frequency channel was outputted on the printout as a single character, representing the second average intensity, minus the baseline, expressed as a dimensionless multiple of the signal's standard deviation.

In the chosen alphanumeric measuring system, a space character denotes an intensity between 0 and 1, that is between baseline and one standard deviation above it.

The numbers 1 to 9 denote the correspondingly numbered intensities from 1 to 9 ; intensities of 10 and above are indicated by a letter: "A" corresponds to intensities between 10 and 11, "B" to 11 to 12, and so on.

John Kraus, the director of the observatory, gave a value of 1 An explanation of the difference between Ehman's value and Kraus's can be found in Ehman's paper.

An oscillator , which became the first local oscillator , was ordered for the frequency of 1 However, the university's purchasing department made a typographical error in the order and wrote 1 The software used in the experiment was then written to adjust for this error.

When Ehman computed the frequency of the Wow! The output from each channel was represented in the computer printout as a column of alphanumeric intensity values.

At the time of the observation, the Big Ear radio telescope was only adjustable for altitude or height above the horizon , and relied instead on the rotation of the Earth to scan across the sky.

Given the speed of Earth's rotation and the spatial width of the telescope's observation window, the Big Ear could observe any given point for just 72 seconds.

All these characteristics are present in the Wow! The precise location in the sky where the signal apparently originated is uncertain due to the design of the Big Ear telescope, which featured two feed horns , each receiving a beam from slightly different directions, while following Earth's rotation.

In contrast, the declination was unambiguously determined to be as follows:. The region of the sky in question lies northwest of the globular cluster M55 , in the constellation Sagittarius , roughly 2.

The closest easily visible star is Tau Sagittarii. No nearby sun-like stars were within the antenna coordinates, although in any direction the antenna pattern would encompass about 6 distant stars.

A number of hypotheses have been advanced as to the source and nature of the Wow! None of them have achieved widespread acceptance.

Interstellar scintillation of a weaker continuous signal —similar in effect to atmospheric twinkling—could be an explanation, but that would not exclude the possibility of the signal being artificial in origin.

The significantly more sensitive Very Large Array did not detect the signal, and the probability that a signal below the detection threshold of the Very Large Array could be detected by the Big Ear due to interstellar scintillation is low.

Ehman has said: "We should have seen it again when we looked for it 50 times. Something suggests it was an Earth-sourced signal that simply got reflected off a piece of space debris.

In a podcast, scientific skeptic author Brian Dunning concluded that a radio transmission from deep space in the direction of Sagittarius, as opposed to a near-Earth origin, remains the best technical explanation for the emission, although there is no evidence to conclude that an alien intelligence was the source.

Furthermore, comets do not emit strongly at the frequencies involved, and there is no explanation for why a comet would be observed in one beam but not in the other.

Several attempts were made by Ehman and other astronomers to recover and identify the signal. The signal was expected to occur three minutes apart in each of the telescope's feed horns, but that did not happen.

In and , Robert H. Paul Shuch made several drift-scan observations of the Wow! In and , Gray again searched for the signal using the Very Large Array , which is significantly more sensitive than Big Ear.

In , on the 35th anniversary of the Wow! The transmission consisted of approximately 10, Twitter messages solicited for the purpose by the National Geographic Channel , bearing the hashtag " ChasingUFOs" a promotion for one of the channel's TV series.

To increase the probability that any extraterrestrial recipients would recognize the signal as an intentional communication from another intelligent life form, Arecibo scientists attached a repeating-sequence header to each individual message, and beamed the transmission at roughly 20 times the wattage of the most powerful commercial radio transmitter.

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