Some Transients in the Palomar Observatory Sky Survey (POSS-I) May Be Associated with Above-Ground Nuclear Testing and Reports of Unidentified Anomalous Phenomena
https://www.researchsquare.com/article/rs-6347224/v1External Quote:
Transient star-like objects of unknown origin have been identified in the first Palomar Observatory Sky Survey (POSS-I) conducted prior to the first artificial satellite. We tested speculative hypotheses that some transients are related to nuclear weapons testing or unidentified anomalous phenomena (UAP) reports. A dataset comprising daily data (November 19, 1949 -April 28,1957) regarding identified transients, nuclear testing, and UAP reports was created (n=2,718 days). Results revealed significant (p = .008) associations between nuclear testing and observed transients, with transients 45% more likely on dates within +/- 1 day of nuclear testing. Significant (p<.001) associations were also noted between total number of transients and total independent UAP reports per date, with the largest association observed for dates on which at least one transient was identified (Spearman's rho = 0.14, p = 0.015). For every additional UAP reported on a given date, there was an 8.5% increase in number of transients identified. Small but significant (p = .008) associations between nuclear testing and number of UAP reports were also noted. Findings suggest associations beyond chance between occurrence of transients and both nuclear testing and UAP reports. These findings may help elucidate the nature of POSS-I transients and strengthen empirical support for the UAP phenomenon.
On the Image Profiles of Transients in the Palomar Sky Survey
https://arxiv.org/abs/2507.15896This is quite popular in UFO circles, as supposed evidence of pre-space era satellites or spacecraft that correlate with upticks in UFO sightings.External Quote:The VASCO project has discovered groups of short-lived transients on historical photographic plates that lack conventional explanation. Hambly & Blair (2024) examined nine such transients reported by Villarroel (2021) and found that they exhibit narrower, rounder profiles, attributing this to emulsion flaws. However, well-established optical principles and atmospheric physics imply that unresolved flashes lasting less than a second naturally appear sharper and more circular than stellar images, particularly on long-exposure plates where stars are significantly blurred by seeing and tracking errors. Such profiles are an expected consequence of sub-second optical flashes, making their findings consistent with the transient interpretation.
I'm skeptical.
See also this thread on more detailed analysis.
https://www.metabunk.org/threads/digitized-sky-survey-poss-1.14385/
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