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CIA-UAP-015, Project Blue Book Special Report No. 14 (Analysis of Reports of Unidentified Aerial Objects)

Central Intelligence Agency · 312 pages · text from the file's own layer

This CIA archives copy, released in 2026, holds Project Blue Book Special Report No. 14 (Analysis of Reports of Unidentified Aerial Objects). The Air Technical Intelligence Center at Wright-Patterson Air Force Base issued it on 5 May 1955. The study reduced about 4,000 sighting reports from 1947 to 1952 to IBM punched cards, with 3,201 cases charted, and applied chi square tests to compare known and unknown sightings. It concludes that it is highly improbable the reports represent technological developments beyond present-day scientific knowledge.

From the source:Release of 2026-06-12 This is the USAF Project Blue Book with a CIA cover sheet stating the document is "Official Record Copy." With the exception of the handwritten note on the first page, the content of this document has been available on CIA's public website.

  • p. 78 …Apparently these are harder to identify. I (3} Shape IIn this case, there is a higher…
I
I (4) Duration of observation
I Here there is an excess of KNOWNS in the less-than-
5-second group. Again, the majority of KNOWNS in
I this group are astronomical. The greater proportion
of UNKNOWNS in the 31- to 60-second and 61-second
to 5-minute groups cannot be explained.
I (5) Speed
I The major contribution to chi square for this char
acteristic is due to a large excess of UNKNOWNS in
I the over 400-mph class. It can be assumed that some
of the excessive speeds are inaccuracies in estimates
by observers. However, some radar sightings, which
I are practically impossible to identify, show objects
I with speeds of 1,000 to 2,000 mph and over, and these
reports account for a number of these UNKNOWNS.
(6) Light brightness
I
I Since this chi square was not significant, it is not
necessary to discuss it here.
I An examination of these discrepancies thus brings up a very interest
ing point. In every case for which there is a significant excess of KNOWNS
over UNKNOWNS, the excess can be attributed to an excess of identifiable
astronomical phenomena. This would seem to lead to the conclusion that
I astronomical phenomena are easy to identify and there are very few left in
I the UNKNOWNS. Accordingly, the astronomical object sightings were
deleted from the KNOWN object sightings and the Chi Square Test was again
applied. The results are shown in Tables VIII through XIII, where in this
case the KNOWNS do not contain astronomical sightings.
I It will be noted that some groups were combined when the adjusted
number of KNOWNS was ten or less, except for the case for which the
I number of objects per sighting was the characteristic studied. These were
borderline cases, and no good combination of groups existed.
I It is apparent that the deletion of astronomical sightings gives a better
fit, although the decision is not clear cut, since for two cases (light bright
I ness and speed}, the chi square increased. However, it can again be pointed
I out that the reporting of these two characteristics is highly subjective and is
open to question. The estimation of speed is especially open to question
because of the impossibility of accurately determining it visually.
I
I 69
I

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Case file, from the pursue collection. The PDF is mirrored here; the original link is above. 312 pages are in the text index: search them above, or from the library's search.