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Before Sputnik · source record · paper

A bright triple transient that vanished within 50 min

Solano, E.; Marcy, G. W.; Villarroel, B.; Geier, S.; Streblyanska, A.; Lombardi, G.; Bär, R. E.; Andruk, V. N. · 2024

AI-verified citationSRC-SOLANO-2024
identifier / locator
Monthly Notices of the Royal Astronomical Society 527(3): 6312–6320. DOI: 10.1093/mnras/stad3422. arXiv: 2310.09035
url
https://doi.org/10.1093/mnras/stad3422
verification note
DOI, journal, volume, and pages verified via the Crossref API (2026-08-22 batch); abstract read via Crossref and arXiv 2310.09035.
reliability notes
  • The July 1952 triple-transient paper: three ~16 mag point sources within 10 arcsec, present in one exposure of 1952 July 19 and absent ~50 minutes later, with 2023 Gran Telescopio Canarias follow-up to magnitude 25.5.
  • VASCO-team authorship; no independent physical inspection of the original plate has been published.

Evidence drawn from this source

Supports· moderateTRN-E007

The July 1952 triple transient and its deep follow-up

what the source states
Three optically bright (~16 mag) point sources within 10 arcsec of each other appear on one Palomar exposure of 1952 July 19 and vanished within the hour, based on two consecutive exposures; they remain absent in 71 years of subsequent imaging, including 2023 Gran Telescopio Canarias exposures reaching magnitude 25.5, implying dimming of more than 10 magnitudes within an hour. The most isolated of the three has a profile nearly the same as comparison stars, implying sub-arcsecond angular size and no elongation from movement.
what we infer
A second canonical multi-source event, peer reviewed with modern follow-up. Note the internal tension it creates: these profiles look like stars, while the 1950 nine are distinctly sharper — the canonical events are not morphologically uniform, which any single-mechanism explanation (defect or flash) must eventually accommodate.
limitations
  • Proponent-team report on the same digitized Palomar lineage; no published physical inspection of the 1952 plate material.
Solano, E. (2024)AI-verified citationTRN-C003