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UNITED STATES / 15 August 1977, local observing date

The Wow! signal: six samples, many interpretations

Big Ear recorded a striking narrowband signal represented by six intensity symbols. The file examines the printout, receiver geometry and the limits of an observation without an established repeating source.

Author: EklipsisEdition 1 · 2026-09-294 source entries3 inspector tasks

Delaware, Ohio — Big Ear observing area · Approximate terrestrial receiving-site area. The marker is not the position or distance of the unknown radio source.

Assessment: A documented radio observation; an artificial extraterrestrial transmitter is not established.

Investigation and inspector’s assessment

Observation brief

On the local evening of 15 August 1977, the Big Ear telescope recorded the signal later marked by Jerry Ehman with the handwritten word Wow. The sequence 6EQUJ5 represents binned intensity, not a received sentence. The six entries span about seventy-two seconds of the instrument’s sampling cycle. They describe the passage through the receiving pattern; they do not independently measure the total lifetime of the emitter. [W1] [W2]

Reading the receiver correctly

Ehman’s technical accounts explain the two-horn arrangement and corrections needed to interpret the recorded coordinates. The unresolved horn assignment leaves alternative sky positions. A map pin in Ohio identifies where the data were collected, not an extraterrestrial destination. The distinction matters because a precise-looking coordinate can conceal an unresolved instrumental ambiguity. [W1] [W2]

Inspector’s assessment

The central task is to reproduce what the printout means before explaining its cause. Preserve the original characters, then add a separate column for the intensity intervals each encodes. Do not replace binned values with exact measurements. Distinguish integration time, processing time and elapsed time. A trend that resembles a beam crossing is informative, but the test should also consider what other sources could produce the same sampling pattern.

Limits of a single detection

A one-off observation can be genuine and still be insufficient for source identification. An attractive frequency, apparent strength and an absence of an immediate explanation do not jointly establish intelligence. Compare hypotheses by predictions: recurrence, bandwidth, motion, visibility in both horns and what other instruments should detect. This dossier does not endorse an absolute claim that all natural or terrestrial explanations have been eliminated; it documents the historical measurement and how to interrogate it.

Documentary chronology

  1. 15 August 1977

    Big Ear records the intensity sequence during its survey. [W1] [W2]

  2. Subsequent printout review

    Ehman notices and marks the sequence after data collection. [W2]

  3. 1997–1998

    The twentieth-anniversary account sets out analysis and corrections. [W2]

  4. 2007–2010

    The thirtieth-anniversary report revises and expands the discussion. [W1]

Dates distinguish the event, the creation of a record and its later publication. Approximate dates remain approximate.

Evidence ledger

Documented

6EQUJ5 is a representation of measured intensity.

[W1] [W2]

Incorrect interpretation of the printout

The six characters are a decoded extraterrestrial message.

[W1] [W2]

Not established

The observation supplies one unique source position and distance.

[W1]

Hypothesis review

A transient or intermittent celestial source

Open source class

Supporting considerations
The signal’s behaviour is analysed against the telescope beam pattern.
Limits and objections
A beam-shaped response alone does not identify a source or explain non-repetition.
Discriminating test
Evaluate repeat observations against both candidate sky positions and documented sensitivity.

Terrestrial interference or an instrumental pathway

Alternative source class

Supporting considerations
A complete signal audit must examine receiver and interference possibilities.
Limits and objections
A generic interference label is not an identified transmitter.
Discriminating test
Specify a mechanism and test its expected frequency, timing and horn response.

An artificial extraterrestrial transmission

Unverified interpretation

Supporting considerations
The observation motivated SETI interest.
Limits and objections
No decoded content or independently established transmitter follows from these records.
Discriminating test
Require reproducible detections and independent instrument confirmation before attribution.

Inspector’s next steps

  1. Decode the recording convention

    Convert the six symbols to intervals using the published convention, retaining the source values. Mark this as a derived table rather than raw receiver data.

  2. Keep both location solutions

    Document coordinate epoch, horn assumptions and corrections. Do not average two alternative positions into a fictional third one.

  3. Build a follow-up ledger

    For any follow-up study added later, list its sky coverage, frequency band, sensitivity and observing duration. A null result only constrains what that search could detect.

These are proposed research tasks, not completed fieldwork or requests already sent to an archive.

Documents and source register

Original reports, scans, catalogue records and later analyses are identified separately. Alternate copies of the same document do not add independent evidence. Follow the named archive for full access information.

W1 / Investigator’s technical report

Jerry Ehman: 30th anniversary technical report

Revised in 2010; includes printout reproductions, corrections and a detailed discussion of instrument geometry.

Language: en

Open original source ↗
W2 / Earlier technical report

Jerry Ehman: 20th anniversary report

Earlier version useful for tracing corrections. It is not an independent observation.

Language: en

Open original source ↗
W3 / Observatory reference

Big Ear frequently asked questions

Observatory context and explanations for frequently repeated misunderstandings.

Language: en

Open original source ↗
W4 / Observatory bibliography

Big Ear surveys and technical articles index

Background to the instrument and its surveys. Individual articles have their own scope.

Language: en

Open original source ↗

Downloadable working files

The pack contains the English dossier, a structured case record, source register, chronology, evidence ledger, hypothesis comparison and inspector task sheet. Downloaded source documents, when available for redistribution, are identified in the pack manifest. Other documents remain direct source links.

Eklipsis authored this synthesis and its working sheets. The original archives and researchers retain credit for their documents. This is a documentary investigation, not a claim that Eklipsis conducted the historical fieldwork.

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