JWST rules out exomoons around LP 890-9 c; Kipping shows how to find them
A new method using repeated observations could detect exomoons despite instrument noise, though this target showed none.
What to know
- JWST has not yet detected any exomoons despite expectations, but a new method by Columbia's David Kipping shows how to find them using repeated observations.
- The technique works by combining data from multiple planet transits to average out instrumental noise and stellar activity, significantly increasing sensitivity.
- Testing on LP 890-9 c ruled out moons larger than 0.1 Earth radii with 95% confidence, representing the most sensitive exomoon search ever conducted outside our solar system.
“Red noise is caused by slow, wandering changes in the detector, such as when it's warming up, its pointing drifts slightly, or even by solar spots on the surface of the star itself.”
Phys.org article · Phys.org
David Kipping Columbia astronomer, Cool Worlds host
How it unfolded 2 developments, newest first · click a bar or a number to jump articlesposts
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Analysis of LP 890-9 c rules out large moons with 95% confidence
Kipping analyzed twelve JWST transits of exoplanet LP 890-9 c, confirming no moons larger than 0.1 Earth radii orbit it—making this the most sensitive exomoon search ever conducted outside our solar system, despite the planet's proximity to its host star making long-term moon survival unlikely.
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Kipping publishes exomoon detection method in arXiv preprint
Columbia astronomer David Kipping released a paper on arXiv showing JWST can detect exomoons by analyzing multiple transits of the same planet to overcome instrumental noise—a departure from previous single-transit approaches.