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NASA’s Nancy Grace Roman Space Telescope is built to do something unusually quiet: map invisible mass. It can’t see dark matter directly, so it measures tiny, almost imperceptible distortions in the shapes of distant galaxies, and lets those small signals add up into something readable. In this episode, you’ll gently explore: • What “weak lensing” really means (in a way you can follow with half-closed eyes) • Why one galaxy tells you almost nothing, but millions can reveal a pattern • How Roman’s wide, stable surveys turn faint distortions into a cosmic map • And what that map quietly suggests about how structure forms across the universe This is a slow, science-heavy journey, calm enough for sleep, and clear enough to leave you with one steady idea: we can learn the unseen by measuring what it changes. If you’d like more long-form, unhurried science like this, consider subscribing to Quiet Science Journeys. And wherever you are tonight, may your night be gentle, and your sleep arrive in its own time.