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The screen of Aris Thorne's primary terminal flickered with the low-frequency pulse of a standard deep-space survey. This rhythmic, soul-crushing monotony had defined the last ten years of his tenure at the Mauna Kea observatory. It was 3:14 AM. The mountain air outside was thin and biting, but inside, the climate-controlled data suite felt stifling, smelling faintly of ozone and stale espresso.
Aris leaned in, his eyes tracing the waveform of a gravitational shear occurring in the outer reaches of the Oort Cloud. The standard deviation for such a phenomenon should have been negligible, a minor ripple in the gravitational tapestry of the solar system. Instead, the readout displayed a sharp, jagged peak-a geometric spike that defied the natural entropy of stellar bodies.
He adjusted the gain on the spectral analyzer, expecting to find a calibration error or a processing glitch within the sensor array. He ran the filter again. The spike remained, and then, with terrifying precision, it repeated.
Pulse. Pause. Harmonic shift. Pulse.
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