No Earth-shadow deficit in 107,608 POSS-I transients (VASCO-ML 8.5° anti-Sun cone; Palomar umbra at 15,000–60,000 km) when per-plate transient counts set the expected rate
Two studies report fewer POSS-I transients in the Earth's shadow than expected. They interpret this as evidence for sunlit objects in orbit before 1957. We tested this claim with the public VASCO-ML catalog of 107,875 candidates. We assigned 107,608 transients to 635 POSS-I red plates. For each plate, the expected count in the shadow is the number of transients on the plate multiplied by the fraction of the plate footprint that the shadow covers. We used five footprint models and a plate bootstrap. In the VASCO-ML 8.5° anti-Sun cone, we observe 501 transients and expect 510.8 (O/E = 0.981, 95% interval 0.80–1.23). The published rate (0.692%) gives each plate the same weight. This overestimates the expected count by 42–52%. Placebo cones show that the equal-weight statistic is not calibrated (placebo O/E 0.37–2.79). In the topocentric umbra seen from Palomar at 15,000–60,000 km, O/E is 0.94–1.09 for all footprint models. At 42,164 km, O/E = 1.07 (95% interval 0.96–1.54). A within-plate permutation test of the highest-score decile (D9) gives contrast ratios of 0.89–1.03 (one-sided p ≥ 0.13). The released catalog does not reproduce the published decile table (D9 in the cone: 22, not 31). We also found that the POSS-I DATE-OBS field 'HH:XX' holds decimal hours. The STScI full-plate headers read it as minutes, which gives time errors of up to 39 min. Limitations: few plates contribute at large distances. At 42,164 km, the 95% intervals include deficits of up to 4% (empirical footprint) or 13% (other footprints). We used the released catalog and did not examine the plate images. The supporting ZIP holds all code, derived data, run logs and figures.
POSS-I · Palomar Observatory Sky Survey · Earth shadow · umbra · transients · vanishing sources · VASCO · photographic plates · Digitized Sky Survey · DATE-OBS · plate observation time · geosynchronous distance · glints · placebo test · plate bootstrap · permutation test · reproduction · null result · pre-Sputnik
References
7- challengesdoi:10.1038/s41598-026-66148-2
We reuse its released VASCO-ML catalog, observing dates and control sample. With per-plate transient counts in the expectation, its reported cone deficit is not present (O/E 0.98), and the released catalog gives 22, not 31, D9 transients in the cone.
- challengesdoi:10.1088/1538-3873/ae0afe
It reports a transient deficit in the Earth's shadow at 42,164 km. In the topocentric umbra from Palomar with per-plate expectations, we find O/E = 1.07 (0.96-1.54) at this distance.
- usesdoi:10.1093/mnras/stac1552
Source of the original POSS-I vanishing-source candidates that the VASCO-ML catalog scores.
- supportsdoi:10.48550/arXiv.2601.21946
It finds no significant shadow deficit with a heterogeneous null model. Our per-plate expectation also gives no deficit.
- challengesdoi:10.48550/arXiv.2602.15171
It is a reply that defends the shadow deficit. Our test with per-plate expectations does not find a deficit.
- challengesdoi:10.48550/arXiv.2604.00056
It reports 0.46% of the 107,875 transients in the umbra at geosynchronous distance against 0.78% expected from plate coverage. With per-plate transient counts in the expectation, we find O/E = 1.07 (0.96-1.54) at 42,164 km.
- challengesdoi:10.48550/arXiv.2609.05105
It infers an altitude of 20,000-25,000 km from the shadow deficit. At 20,000 km and 31,371 km we find O/E of 0.99-1.01.
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