Time-domain astronomy studies how brightness, spectrum, or position changes with time.
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Different physical processes create characteristic time signatures: orbital geometry produces eclipses, stellar oscillations create pulsations, explosions produce rise-and-decay curves, and rotating spots modulate brightness.
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TESS continuously monitors changing sources in broad sky sectors, while Rubin's LSST repeatedly surveys the southern sky to detect and classify enormous numbers of changing or moving objects.
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