How do astronomers find planets around other stars when most are too faint to image directly? This series follows the clues: a star’s motion, a repeating dip in its light, checks against false positives, and other methods such as direct imaging, microlensing and atmospheric spectroscopy. Each method answers a different question, and each depends on what the telescope can measure and the model used to interpret it.
12-second teaser. Full film scheduled for October 25, 2026 at 7:00 PM Toronto time (EDT; -04:00).
Watch the full film from release day: https://youtu.be/rA75Ezi7PwE
The cover is an original conceptual illustration, not observational data.
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